Hubble Space Telescope

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Hubble Space Telescope
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{{short description|Space telescope}}{{redirect|Hubble}}{{pp-move-indef}}{{Use mdy dates|date=February 2019}}{{Use American English|date=March 2018}}

, flying Servicing Mission 4 (STS-125), the fifth and final Hubble mission>style=padding: 2px 0;}}| image_alt = The Hubble Space Telescope in orbit| image_size = 300px| mission_type = AstronomyNASA{{·}}European Space Agency>ESA{{·}}STScI| COSPAR_ID = 1990-037B| SATCAT =}} {{}}24 April 1990 12:33:51sep=,}}Lockheed Missiles and Space Company>Lockheed (spacecraft) Perkin-Elmer (optics)11110lbWORK=HUBBLESITE.ORG ARCHIVEDATE=JULY 6, 2016, 13.24.2ftabbr=on}}| power = 2,800 wattsTITLE=STS-31 LAST=RYBA ACCESSDATE=MAY 7, 2017 ARCHIVE-DATE=MAY 7, 2017, 103}} (STS-31)Kennedy Space Center>Kennedy LC-39B| deployment_date = April 25, 1990| entered_service = May 20, 1990| disposal_type = | deactivated = | last_contact = | decay_date = estimated 2030–2040| orbit_reference = GeocentricLow Earth orbit>Low Earth6917.1mi|abbr=on}}| orbit_eccentricity = 0.000283537.0mi|abbr=on}}540.9mi|abbr=on}}| orbit_inclination = 28.47°| orbit_period = 95.42 minutes| orbit_RAAN = 80.34°| orbit_arg_periapsis = 64.90°| orbit_mean_anomaly = 23.78°| orbit_mean_motion = 15.09 rev/day7.59abbr=on}}WORK=HEAVENS ABOVE ACCESSDATE=AUGUST 16, 2018, | orbit_rev_number = 35,441| apsis = geeRitchey–Chrétien telescope>Ritchey–Chrétien reflector94.5m ftorder=outPUBLISHER=NASA/LOCKHEED MARTIN LAST=NELSON PAGES=1–5, 2009, 189morder=flip|abbr=on}}24}}4.525ft2abbr=on}}| telescope_wavelength = Near-infrared, visible light, ultraviolet| instruments_list =

}}The Hubble Space Telescope (often referred to as HST or Hubble) is a space telescope that was launched into low Earth orbit in 1990 and remains in operation. It was not the first space telescope, but it is one of the largest and most versatile and is well known as both a vital research tool and a public relations boon for astronomy. The Hubble telescope is named after astronomer Edwin Hubble and is one of NASA's Great Observatories, along with the Compton Gamma Ray Observatory, the Chandra X-ray Observatory, and the Spitzer Space Telescope.WEB,weblink NASA's Great Observatories, NASA, Canright, Shelley, April 26, 2008, Hubble features a {{convert|2.4|m|ft|adj=on|sp=us}} mirror, and its four main instruments observe in the ultraviolet, visible, and near infrared regions of the electromagnetic spectrum. Hubble's orbit outside the distortion of Earth's atmosphere allows it to take extremely high-resolution images with substantially lower background light than ground-based telescopes. It has recorded some of the most detailed visible light images, allowing a deep view into space. Many Hubble observations have led to breakthroughs in astrophysics, such as determining the rate of expansion of the universe.The Hubble telescope was built by the United States space agency NASA with contributions from the European Space Agency. The Space Telescope Science Institute (STScI) selects Hubble's targets and processes the resulting data, while the Goddard Space Flight Center controls the spacecraft.WEB,weblink Hubble Essentials,, March 3, 2016, Space telescopes were proposed as early as 1923. Hubble was funded in the 1970s, with a proposed launch in 1983, but the project was beset by technical delays, budget problems, and the Challenger disaster (1986). It was finally launched by {{OV|Discovery}} in 1990, but its main mirror had been ground incorrectly and created a spherical aberration, compromising the telescope's capabilities. The optics were corrected to their intended quality by a servicing mission in 1993.Hubble is the only telescope designed to be maintained in space by astronauts. Five Space Shuttle missions have repaired, upgraded, and replaced systems on the telescope, including all five of the main instruments. The fifth mission was canceled on safety grounds following the Columbia disaster (2003), but NASA administrator Michael D. Griffin approved the fifth servicing mission which was completed in 2009. The telescope is operating {{as of|2019|lc=y}}, and could last until 2030–2040. Its successor is the James Webb Space Telescope (JWST) which is scheduled to be launched in March 2021. WEB,weblink NASA Completes Webb Telescope Review, Commits to Launch in Early 2021, National Aeronautics And Administration, June 27, 2018, June 28, 2018,

Conception, design and aim

Proposals and precursors

(File:Astronaut Owen Garriott Performs EVA During Skylab 3 - GPN-2002-000065.jpg|thumb|Astronaut Owen Garriott works next to Skylab's manned solar space observatory, 1973)In 1923, Hermann Oberth—considered a father of modern rocketry, along with Robert H. Goddard and Konstantin Tsiolkovsky—published ("The Rocket into Planetary Space"), which mentioned how a telescope could be propelled into Earth orbit by a rocket.BOOK, Die Rakete zu den Planetenräumen, Oberth, Hermann, R. Oldenbourg-Verlay, 85, 1923, The history of the Hubble Space Telescope can be traced back as far as 1946, to the astronomer Lyman Spitzer's paper "Astronomical advantages of an extraterrestrial observatory".Spitzer, Lyman Jr., "Report to Project Rand: Astronomical Advantages of an Extra-Terrestrial Observatory", reprinted in NASA SP-2001-4407: Exploring the Unknown, Chapter 3, Document III-1, p. 546. In it, he discussed the two main advantages that a space-based observatory would have over ground-based telescopes. First, the angular resolution (the smallest separation at which objects can be clearly distinguished) would be limited only by diffraction, rather than by the turbulence in the atmosphere, which causes stars to twinkle, known to astronomers as seeing. At that time ground-based telescopes were limited to resolutions of 0.5–1.0 arcseconds, compared to a theoretical diffraction-limited resolution of about 0.05 arcsec for a telescope with a mirror {{convert|2.5|m|ft|abbr=on}} in diameter. Second, a space-based telescope could observe infrared and ultraviolet light, which are strongly absorbed by the atmosphere.Spitzer devoted much of his career to pushing for the development of a space telescope. In 1962, a report by the US National Academy of Sciences recommended the development of a space telescope as part of the space program, and in 1965 Spitzer was appointed as head of a committee given the task of defining scientific objectives for a large space telescope.WEB,weblink About Lyman Spitzer, Jr, Caltech, April 26, 2008,weblink" title="">weblink March 27, 2008, Space-based astronomy had begun on a very small scale following World War II, as scientists made use of developments that had taken place in rocket technology. The first ultraviolet spectrum of the Sun was obtained in 1946,JOURNAL, Solar Ultraviolet Spectrum to 88 Kilometers, Baum, WA, 4, Johnson, FS, Oberly, JJ, Rockwood, CC, Strain, CV, Tousey, R., Phys. Rev., 70, 781–782, November 1946, 10.1103/PhysRev.70.781, American Physical Society, 9–10, 1946PhRv...70..781B, and the National Aeronautics and Space Administration (NASA) launched the Orbiting Solar Observatory (OSO) to obtain UV, X-ray, and gamma-ray spectra in 1962.WEB,weblink The First Orbiting Solar Observatory, June 26, 2003,, NASA Goddard Space Flight Center, September 25, 2011, An orbiting solar telescope was launched in 1962 by the United Kingdom as part of the Ariel space program, and in 1966 NASA launched the first Orbiting Astronomical Observatory (OAO) mission. OAO-1's battery failed after three days, terminating the mission. It was followed by OAO-2, which carried out ultraviolet observations of stars and galaxies from its launch in 1968 until 1972, well beyond its original planned lifetime of one year.WEB,weblink OAO, NASA, April 26, 2008, dead,weblink" title="">weblink September 16, 2008, The OSO and OAO missions demonstrated the important role space-based observations could play in astronomy. In 1968, NASA developed firm plans for a space-based reflecting telescope with a mirror {{convert|3|m|ft|abbr=on}} in diameter, known provisionally as the Large Orbiting Telescope or Large Space Telescope (LST), with a launch slated for 1979. These plans emphasized the need for manned maintenance missions to the telescope to ensure such a costly program had a lengthy working life, and the concurrent development of plans for the reusable Space Shuttle indicated that the technology to allow this was soon to become available.{{sfn|Spitzer|1979|p=32}}

Quest for funding

The continuing success of the OAO program encouraged increasingly strong consensus within the astronomical community that the LST should be a major goal. In 1970, NASA established two committees, one to plan the engineering side of the space telescope project, and the other to determine the scientific goals of the mission. Once these had been established, the next hurdle for NASA was to obtain funding for the instrument, which would be far more costly than any Earth-based telescope. The U.S. Congress questioned many aspects of the proposed budget for the telescope and forced cuts in the budget for the planning stages, which at the time consisted of very detailed studies of potential instruments and hardware for the telescope. In 1974, public spending cuts led to Congress deleting all funding for the telescope project.{{sfn|Spitzer|1979|pp=33–34}}In response a nationwide lobbying effort was coordinated among astronomers. Many astronomers met congressmen and senators in person, and large scale letter-writing campaigns were organized. The National Academy of Sciences published a report emphasizing the need for a space telescope, and eventually the Senate agreed to half of the budget that had originally been approved by Congress.{{sfn|Spitzer|1979|p=34}}The funding issues led to something of a reduction in the scale of the project, with the proposed mirror diameter reduced from 3 m to 2.4 m, both to cut costsBOOK, Andersen, Geoff, The telescope: its history, technology, and future, 2007, Princeton University Press, 978-0-691-12979-2, 116,weblink and to allow a more compact and effective configuration for the telescope hardware. A proposed precursor {{convert|1.5|m|ft|abbr=on}} space telescope to test the systems to be used on the main satellite was dropped, and budgetary concerns also prompted collaboration with the European Space Agency. ESA agreed to provide funding and supply one of the first generation instruments for the telescope, as well as the solar cells that would power it, and staff to work on the telescope in the United States, in return for European astronomers being guaranteed at least 15% of the observing time on the telescope."Memorandum of Understanding Between The European Space Agency and The United States National Aeronautics and Space Administration", reprinted in NASA SP-2001-4407: Exploring the Unknown, Chapter 3, Document III-29, p. 671. Congress eventually approved funding of {{US$|36 million}} for 1978, and the design of the LST began in earnest, aiming for a launch date of 1983.{{sfn|Spitzer|1979|p=34}} In 1983 the telescope was named after Edwin Hubble,WEB,weblink Okolski, Gabriel, A Chronology of the Hubble Space Telescope, NASA, April 26, 2008, who confirmed one of the greatest scientific breakthroughs of the 20th century made by Georges Lemaître that the universe is expanding.WEB,weblink The Path to Hubble Space Telescope, NASA, April 26, 2008,weblink" title="">weblink May 24, 2008,

Construction and engineering

(File:Hubble mirror polishing.jpg|thumb|Grinding of Hubble's primary mirror at Perkin-Elmer, March 1979)Once the Space Telescope project had been given the go-ahead, work on the program was divided among many institutions. Marshall Space Flight Center (MSFC) was given responsibility for the design, development, and construction of the telescope, while Goddard Space Flight Center was given overall control of the scientific instruments and ground-control center for the mission.{{sfn|Dunar|Waring|1999|pp=487–488}} MSFC commissioned the optics company Perkin-Elmer to design and build the Optical Telescope Assembly (OTA) and Fine Guidance Sensors for the space telescope. Lockheed was commissioned to construct and integrate the spacecraft in which the telescope would be housed.{{sfn|Dunar|Waring|1999|p=489}}

Optical Telescope Assembly

Optically, the HST is a Cassegrain reflector of Ritchey–Chrétien design, as are most large professional telescopes. This design, with two hyperbolic mirrors, is known for good imaging performance over a wide field of view, with the disadvantage that the mirrors have shapes that are hard to fabricate and test. The mirror and optical systems of the telescope determine the final performance, and they were designed to exacting specifications. Optical telescopes typically have mirrors polished to an accuracy of about a tenth of the wavelength of visible light, but the Space Telescope was to be used for observations from the visible through the ultraviolet (shorter wavelengths) and was specified to be diffraction limited to take full advantage of the space environment. Therefore, its mirror needed to be polished to an accuracy of {{convert|10|nm|uin |abbr=off|lk=on|sigfig=1|sp=us}}, or about 1/65 of the wavelength of red light.JOURNAL, Hubble: The Case of the Single-Point Failure, Science Magazine, MM, Waldrop, August 17, 1990, 249, 4970, 735–736, 10.1126/science.249.4970.735, 17756776, 1990Sci...249..735W, On the long wavelength end, the OTA was not designed with optimum IR performance in mind—for example, the mirrors are kept at stable (and warm, about 15 Â°C) temperatures by heaters. This limits Hubble's performance as an infrared telescope.(File:Hubble backup mirror.jpg|thumb|rightt|The backup mirror, by Kodak; its inner support structure can be seen because it is not coated with a reflective surface)Perkin-Elmer intended to use custom-built and extremely sophisticated computer-controlled polishing machines to grind the mirror to the required shape.{{sfn|Dunar|Waring|1999|p=489}} However, in case their cutting-edge technology ran into difficulties, NASA demanded that PE sub-contract to Kodak to construct a back-up mirror using traditional mirror-polishing techniques.{{sfn|Allen|Angel|Mangus|Rodney|1990|pp=3–4}} (The team of Kodak and Itek also bid on the original mirror polishing work. Their bid called for the two companies to double-check each other's work, which would have almost certainly caught the polishing error that later caused such problems.NEWS,weblink Losing Bid Offered 2 Tests on Hubble, Associated Press, July 28, 1990, The New York Times, April 26, 2008, ) The Kodak mirror is now on permanent display at the National Air and Space Museum.PRESS RELEASE, Hubble Space Telescope Stand-in Gets Starring Role, September 21, 2001,weblink Goddard Space Flight Center, April 26, 2008,weblink" title="">weblink February 26, 2008, WEB, Backup Mirror, Hubble Space Telescope,weblink National Air and Space Museum, November 4, 2012,weblink" title="">weblink November 2, 2012, An Itek mirror built as part of the effort is now used in the 2.4 m telescope at the Magdalena Ridge Observatory.TECHREPORT, Magdalena Ridge Observatory, 2.4m Observatory Technical Note, January 1, 2008,weblink January 21, 2013, 2, 1.6, Construction of the Perkin-Elmer mirror began in 1979, starting with a blank manufactured by Corning from their ultra-low expansion glass. To keep the mirror's weight to a minimum it consisted of top and bottom plates, each {{convert|1|in|mm|spell=in}} thick, sandwiching a honeycomb lattice. Perkin-Elmer simulated microgravity by supporting the mirror from the back with 130 rods that exerted varying amounts of force.CONFERENCE, Design and fabrication of the NASA 2.4-meter space telescope, Daniel J., McCarthy, Terence A., Facey, Proc. SPIE 0330, Optical Systems Engineering II, 139–143, 1982, International Society for Optics and Photonics, 10.1117/12.934268, This ensured that the mirror's final shape would be correct and to specification when finally deployed. Mirror polishing continued until May 1981. NASA reports at the time questioned Perkin-Elmer's managerial structure, and the polishing began to slip behind schedule and over budget. To save money, NASA halted work on the back-up mirror and put the launch date of the telescope back to October 1984.{{sfn|Dunar|Waring|1999|p=496}} The mirror was completed by the end of 1981; it was washed using {{convert|2400|USgal|L}} of hot, deionized water and then received a reflective coating of {{convert|65|nm|uin |abbr=on|adj=mid|-thick}} aluminum and a protective coating of {{convert|25|nm|uin |abbr=on|adj=mid|-thick}} magnesium fluoride.JOURNAL, The Performance of HST as an Infrared Telescope, M., Robberto, A., 4, Sivaramakrishnan, J. J., Bacinski, D., Calzetti, J. E., Krist, J. W., MacKenty, J., Piquero, M., Stiavelli,weblink Proc. SPIE, 4013, 386–393, 2000, 10.1117/12.394037, UV, Optical, and IR Space Telescopes and Instruments, Breckinridge, James B, Jakobsen, Peter, 2000SPIE.4013..386R, BOOK, The Space Telescope, Michael Friedman, New York, David, Ghitelman, 32, 1987, 978-0831779719,weblink (File:Early stages of Hubble construction.jpg|thumb|The OTA, metering truss, and secondary baffle are visible in this image of Hubble during early construction.)Doubts continued to be expressed about Perkin-Elmer's competence on a project of this importance, as their budget and timescale for producing the rest of the OTA continued to inflate. In response to a schedule described as "unsettled and changing daily", NASA postponed the launch date of the telescope until April 1985. Perkin-Elmer's schedules continued to slip at a rate of about one month per quarter, and at times delays reached one day for each day of work. NASA was forced to postpone the launch date until March and then September 1986. By this time, the total project budget had risen to {{US$|1.175 billion}}.{{sfn|Dunar|Waring|1999|p=504}}

Spacecraft systems

The spacecraft in which the telescope and instruments were to be housed was another major engineering challenge. It would have to withstand frequent passages from direct sunlight into the darkness of Earth's shadow, which would cause major changes in temperature, while being stable enough to allow extremely accurate pointing of the telescope. A shroud of multi-layer insulation keeps the temperature within the telescope stable and surrounds a light aluminum shell in which the telescope and instruments sit. Within the shell, a graphite-epoxy frame keeps the working parts of the telescope firmly aligned.WEB,weblink Hubble Space Telescope Systems, Goddard Space Flight Center, April 26, 2008,weblink" title="">weblink March 17, 2003, Because graphite composites are hygroscopic, there was a risk that water vapor absorbed by the truss while in Lockheed's clean room would later be expressed in the vacuum of space; resulting in the telescope's instruments being covered by ice. To reduce that risk, a nitrogen gas purge was performed before launching the telescope into space.Ghitelman, David (1987). The Space Telescope. New York: Michael Friedman Publishing. p. 50.While construction of the spacecraft in which the telescope and instruments would be housed proceeded somewhat more smoothly than the construction of the OTA, Lockheed still experienced some budget and schedule slippage, and by the summer of 1985, construction of the spacecraft was 30% over budget and three months behind schedule. An MSFC report said that Lockheed tended to rely on NASA directions rather than take their own initiative in the construction.{{sfn|Dunar|Waring|1999|p=508}}

Computer systems and data processing

missing image!
- DF-224.jpg -
DF-224 in Hubble, before it was replaced in 1999
The two initial, primary computers on the HST were the 1.25 MHz DF-224 system, built by Rockwell Autonetics, which contained three redundant CPUs, and two redundant NSSC-1 (NASA Standard Spacecraft Computer, Model 1) systems, developed by Westinghouse and GSFC using diode–transistor logic (DTL). A co-processor for the DF-224 was added during Servicing Mission 1 in 1993, which consisted of two redundant strings of an Intel-based 80386 processor with an 80387 math co-processor.WEB,weblink Co-Processor, NASA Facts, NASA, June 1993, NF-193, The DF-224 and its 386 co-processor were replaced by a 25 MHz Intel-based 80486 processor system during Servicing Mission 3A in 1999.WEB,weblink Hubble Space Telescope Servicing Mission 3A: New Advanced Computer, NASA Facts, NASA, 1999, FS-1999-06-009-GSFC, The new computer is 20 times faster, with six times more memory, than the DF-224 it replaced. It increases throughput by moving some computing tasks from the ground to the spacecraft and saves money by allowing the use of modern programming languages.TECHREPORT,weblink PDF, Hubble Space Telescope Servicing Mission 3A Media Reference Guide, NASA, Lockheed Martin Missiles and Space, April 27, 2008, 5–9 and Section 7.1.1, Additionally, some of the science instruments and components had their own embedded microprocessor-based control systems. The MATs (Multiple Access Transponder) components, MAT-1 and MAT-2, utilize Hughes Aircraft CDP1802CD microprocessors.JOURNAL,weblink How Long Can the Hubble Space Telescope Operate Reliably? – A Total Dose Perspective, IEEE Transactions on Nuclear Science, M. A., Xapsos, C., Stauffer, T., Jordan, C., Poivey, D. N., Haskins, G., Lum, A. M., Pergosky, D. C., Smith, K. A., LaBel, 4, 61, 6, 3356–3362, December 2014, 2014ITNS...61.3356X, 10.1109/TNS.2014.2360827, The Wide Field and Planetary Camera (WFPC) also utilized an RCA 1802 microprocessor (or possibly the older 1801 version).MAGAZINE,weblink Hubble Space Telescope's Wide Field/Planetary Camera, Shutterbug, A., Afshari, January 1993, dead,weblink" title="">weblink October 6, 2016, The WFPC-1 was replaced by the WFPC-2 during Servicing Mission 1 in 1993, which was then replaced by the Wide Field Camera 3 (WFC3) during Servicing Mission 4 in 2009.

Initial instruments

File:HubbleExploded edit 1.svg|thumb|Exploded viewExploded viewWhen launched, the HST carried five scientific instruments: the Wide Field and Planetary Camera (WF/PC), Goddard High Resolution Spectrograph (GHRS), High Speed Photometer (HSP), Faint Object Camera (FOC) and the Faint Object Spectrograph (FOS). WF/PC was a high-resolution imaging device primarily intended for optical observations. It was built by NASA's Jet Propulsion Laboratory, and incorporated a set of 48 filters isolating spectral lines of particular astrophysical interest. The instrument contained eight charge-coupled device (CCD) chips divided between two cameras, each using four CCDs. Each CCD has a resolution of 0.64 megapixels.WEB,weblink WFPC2, STScI, May 18, 2012, The "wide field camera" (WFC) covered a large angular field at the expense of resolution, while the "planetary camera" (PC) took images at a longer effective focal length than the WF chips, giving it a greater magnification.TECHREPORT, The Space Telescope Observatory, CP-2244, NASA, Donald N. B., Hall,weblink 1982, 40 MB PDF file.The GHRS was a spectrograph designed to operate in the ultraviolet. It was built by the Goddard Space Flight Center and could achieve a spectral resolution of 90,000.JOURNAL, Brandt, JC, 1994, The Goddard High Resolution Spectrograph: Instrument, goals, and science results, Publications of the Astronomical Society of the Pacific, 106, 890–908, 1994PASP..106..890B, 10.1086/133457, vanc, 4, Heap, SR, Beaver, EA, Boggess, A, Carpenter, KG, Ebbets, DC, Hutchings, JB, Jura, M, Leckrone, DS, Also optimized for ultraviolet observations were the FOC and FOS, which were capable of the highest spatial resolution of any instruments on Hubble. Rather than CCDs these three instruments used photon-counting digicons as their detectors. The FOC was constructed by ESA, while the University of California, San Diego, and Martin Marietta Corporation built the FOS.The final instrument was the HSP, designed and built at the University of Wisconsin–Madison. It was optimized for visible and ultraviolet light observations of variable stars and other astronomical objects varying in brightness. It could take up to 100,000 measurements per second with a photometric accuracy of about 2% or better.Bless, RC; Walter, LE; White RL (1992). High Speed Photometer Instrument Handbook v 3.0. STSci.HST's guidance system can also be used as a scientific instrument. Its three Fine Guidance Sensors (FGS) are primarily used to keep the telescope accurately pointed during an observation, but can also be used to carry out extremely accurate astrometry; measurements accurate to within 0.0003 arcseconds have been achieved.CONFERENCE, Benedict, G. Fritz, McArthur, Barbara E., 2005, High-precision stellar parallaxes from Hubble Space Telescope fine guidance sensors, Transits of Venus: New Views of the Solar System and Galaxy, IAU Colloquium #196, DW Kurtz, Cambridge University Press, 333–346, 2005tvnv.conf..333B, 10.1017/S1743921305001511,

Ground support

(File:Hubble Control Centre.jpg|thumb|Hubble Control Center at Goddard Space Flight Center, 1999)The Space Telescope Science Institute (STScI) is responsible for the scientific operation of the telescope and the delivery of data products to astronomers. STScI is operated by the Association of Universities for Research in Astronomy (AURA) and is physically located in Baltimore, Maryland on the Homewood campus of Johns Hopkins University, one of the 39 US universities and seven international affiliates that make up the AURA consortium. STScI was established in 1981BOOK,weblink AURA and Its US National Observatories, Cambridge University Press, Frank K., Edmondson, 244, 1997, 9780521553452, WEB,weblink About AURA, AURA, November 6, 2012, after something of a power struggle between NASA and the scientific community at large. NASA had wanted to keep this function in-house, but scientists wanted it to be based in an academic establishment.{{sfn|Dunar|Waring|1999|pp=486–487}}Roman, Nancy Grace. "Exploring the Universe: Space-Based Astronomy and Astrophysics", in NASA SP-2001-4407: Exploring the Unknown (PDF). NASA. Chapter 3, p. 536. The Space Telescope European Coordinating Facility (ST-ECF), established at Garching bei München near Munich in 1984, provided similar support for European astronomers until 2011, when these activities were moved to the European Space Astronomy Centre.{{multiple image |align=right |direction=horizontal |total_width=400
|image1=Diagram of Hubble's orbit.jpg |caption1=Hubble's low orbit means many targets are visible for slightly more than half of an orbit's elapsed time, since they are blocked from view by the Earth for almost one-half of each orbit.
|image2=Animation of Hubble Space Telescope trajectory.gif |caption2=Animation of Hubble's orbit from October 31, 2018, to December 25, 2018. Earth is not shown.
}}One rather complex task that falls to STScI is scheduling observations for the telescope.WEB,weblink Team Hubble, STScI, November 6, 2012, Hubble is in a low-Earth orbit to enable servicing missions, but this means that most astronomical targets are occulted by the Earth for slightly less than half of each orbit. Observations cannot take place when the telescope passes through the South Atlantic Anomaly due to elevated radiation levels, and there are also sizable exclusion zones around the Sun (precluding observations of Mercury), Moon and Earth. The solar avoidance angle is about 50°, to keep sunlight from illuminating any part of the OTA. Earth and Moon avoidance keeps bright light out of the FGSs, and keeps scattered light from entering the instruments. If the FGSs are turned off, however, the Moon and Earth can be observed. Earth observations were used very early in the program to generate flat-fields for the WFPC1 instrument. There is a so-called continuous viewing zone (CVZ), at roughly 90° to the plane of Hubble's orbit, in which targets are not occulted for long periods. Due to the precession of the orbit, the location of the CVZ moves slowly over a period of eight weeks. Because the (wikt:Limb|limb) of the Earth is always within about 30° of regions within the CVZ, the brightness of scattered earthshine may be elevated for long periods during CVZ observations.Hubble orbits in low Earth orbit at an altitude of approximately {{convert|540|km|sp=us}} and an inclination of 28.5°. The position along its orbit changes over time in a way that is not accurately predictable. The density of the upper atmosphere varies according to many factors, and this means that Hubble's predicted position for six weeks' time could be in error by up to {{convert|4000|km|abbr=on}}. Observation schedules are typically finalized only a few days in advance, as a longer lead time would mean there was a chance that the target would be unobservable by the time it was due to be observed.{{sfn|Strolger|Rose|2017|p=46}}Engineering support for HST is provided by NASA and contractor personnel at the Goddard Space Flight Center in Greenbelt, Maryland, {{convert|48|km|abbr=on}} south of the STScI. Hubble's operation is monitored 24 hours per day by four teams of flight controllers who make up Hubble's Flight Operations Team.

Challenger disaster, delays, and eventual launch

File:STS-31 Hubble launch roll and pitch.jpg|thumb|upright|STS-31STS-31(File:1990 s31 IMAX view of HST release.jpg|thumb|Hubble being deployed from Discovery in 1990.)By early 1986, the planned launch date of October that year looked feasible, but the Challenger accident brought the U.S. space program to a halt, grounding the Space Shuttle fleet and forcing the launch of Hubble to be postponed for several years. The telescope had to be kept in a clean room, powered up and purged with nitrogen, until a launch could be rescheduled. This costly situation (about {{US$|6 million}} per month) pushed the overall costs of the project even higher. This delay did allow time for engineers to perform extensive tests, swap out a possibly failure-prone battery, and make other improvements.{{sfn|Tatarewicz|1998|p=371}} Furthermore, the ground software needed to control Hubble was not ready in 1986, and was barely ready by the 1990 launch.NEWS, Telescope Is Set to Peer at Space and Time, John, Wilford,weblink The New York Times, April 9, 1990, January 19, 2009, Eventually, following the resumption of shuttle flights in 1988, the launch of the telescope was scheduled for 1990. On April 24, 1990, {{OV|Discovery}} successfully launched the telescope into its planned orbit during the STS-31 mission.WEB,weblink STS-31, NASA, April 26, 2008, From its original total cost estimate of about {{US$|400 million}}, the telescope cost about {{US$|4.7 billion}} by the time of its launch. Hubble's cumulative costs were estimated to be about {{US$|10 billion}} in 2010, twenty years after launch.WEB,weblink James Webb Space Telescope (JWST) Independent Comprehensive Review Panel (ICRP) Final Report, 32, NASA, September 4, 2012,

List of Hubble instruments

Hubble accommodates five science instruments at a given time, plus the Fine Guidance Sensors, which are mainly used for aiming the telescope but are occasionally used for scientific astrometry measurements. Early instruments were replaced with more advanced ones during the Shuttle servicing missions. COSTAR was a corrective optics device rather than a science instrument, but occupied one of the five instrument bays.Since the final servicing mission in 2009, the four active instruments have been ACS, COS, STIS and WFC3. NICMOS is kept in hibernation, but may be revived if WFC3 were to fail in the future. Of the former instruments, three (COSTAR, FOS and WFPC2) are displayed in the Smithsonian National Air and Space Museum. The FOC is in the Dornier museum, Germany. The HSP is in the Space Place at the University of Wisconsin–Madison. The first WFPC was dismantled, and some components were then re-used in WFC3.

Flawed mirror

File:Hubble PSF with flawed optics.jpg|thumb|An extract from a WF/PC image shows the light from a star spread over a wide area instead of being concentrated on a few pixels.]]Within weeks of the launch of the telescope, the returned images indicated a serious problem with the optical system. Although the first images appeared to be sharper than those of ground-based telescopes, Hubble failed to achieve a final sharp focus and the best image quality obtained was drastically lower than expected. Images of point sources spread out over a radius of more than one arcsecond, instead of having a point spread function (PSF) concentrated within a circle 0.1 arcsec in diameter as had been specified in the design criteria.JOURNAL, The imaging performance of the Hubble Space Telescope, Astrophysical Journal Letters, Christopher J., Burrows, Jon A., 4, Holtzman, S. M., Faber, Pierre Y., Bely, Hashima, Hasan, C. R., Lynds, Daniel, Schroeder, 369, L21–L25, March 10, 1991, 10.1086/185950, 1991ApJ...369L..21B, WEB,weblink WFPC2 Instrument Handbook, Chapter 5.1, STScI, 2004, Heyer, Biretta, etal, Baltimore, 9.0, April 26, 2008, Analysis of the flawed images showed that the cause of the problem was that the primary mirror had been polished to the wrong shape. Although it was probably the most precisely figured optical mirror ever made, smooth to about {{convert|10|nm|uin |abbr=on|sigfig=1}}, at the perimeter it was too flat by about {{convert|2200|nm|um uin |abbr=off|lk=on|sp=us}}.WEB,weblink Servicing Mission 1, NASA, March 28, 2016,weblink" title="">weblink April 20, 2008, This difference was catastrophic, introducing severe spherical aberration, a flaw in which light reflecting off the edge of a mirror focuses on a different point from the light reflecting off its center.{{sfn|Tatarewicz|1998|p=375}}The effect of the mirror flaw on scientific observations depended on the particular observation—the core of the aberrated PSF was sharp enough to permit high-resolution observations of bright objects, and spectroscopy of point sources was only affected through a sensitivity loss. However, the loss of light to the large, out-of-focus halo severely reduced the usefulness of the telescope for faint objects or high-contrast imaging. This meant that nearly all of the cosmological programs were essentially impossible, since they required observation of exceptionally faint objects.{{sfn|Tatarewicz|1998|p=375}} NASA and the telescope became the butt of many jokes, and the project was popularly regarded as a white elephant. For instance, in the 1991 comedy (The Naked Gun 2½: The Smell of Fear), in a scene where high-profile disasters were displayed, Hubble was pictured with Lusitania, the Hindenburg, and the Edsel.WEB,weblink The Naked Gun 2½: The Smell of Fear, Internet Movie Database, April 26, 2008, Nonetheless, during the first three years of the Hubble mission, before the optical corrections, the telescope still carried out a large number of productive observations of less demanding targets.JOURNAL, Goodwin, Irwin, 1994, Hubble repair improves vision and helps restore NASA's image, Physics Today, 47, 3, 42, Cioffi, Denis F., 10.1063/1.2808434, 1994PhT....47c..42G, The error was well characterized and stable, enabling astronomers to partially compensate for the defective mirror by using sophisticated image processing techniques such as deconvolution.{{sfn|Dunar|Waring|1999|pp=514–515}}

Origin of the problem

File:PIA22913-HubbleSpaceTelescope-ComparisonOfCameraImages-20181204.jpg|thumb|upright=1.5|Optical evolution of Hubble's primary camera system. These images show spiral galaxy M100 as seen with WFPC1 in 1993 before corrective optics (left), with WFPC2 in 1994 after correction (center), and with WFC3 in 2018 (right).]]A commission headed by Lew Allen, director of the Jet Propulsion Laboratory, was established to determine how the error could have arisen. The Allen Commission found that a reflective null corrector, a testing device used to achieve a properly shaped non-spherical mirror, had been incorrectly assembled—one lens was out of position by {{convert|1.3|mm|in|abbr=on}}.{{sfn|Allen|Angel|Mangus|Rodney|1990|p=7-1|ps=: The spacing of the field lens in the corrector was to have been done by laser measurements off the end of an invar bar. Instead of illuminating the end of the bar, however, the laser in fact was reflected from a worn spot on a black-anodized metal cap placed over the end of the bar to isolate its center (visible through a hole in the cap). The technician who performed the test noted an unexpected gap between the field lens and its supporting structure in the corrector and filled it in with an ordinary metal washer.}} During the initial grinding and polishing of the mirror, Perkin-Elmer analyzed its surface with two conventional refractive null correctors. However, for the final manufacturing step (figuring), they switched to the custom-built reflective null corrector, designed explicitly to meet very strict tolerances. The incorrect assembly of this device resulted in the mirror being ground very precisely but to the wrong shape. A few final tests, using the conventional null correctors, correctly reported spherical aberration. But these results were dismissed, thus missing the opportunity to catch the error, because the reflective null corrector was considered more accurate.{{sfn|Dunar|Waring|1999|p=512|ps=: "the firm's optical operations personnel dismissed the evidence as itself flawed. They believed the other two null correctors were less accurate than the reflective null corrector and so could not verify its reliability. Since they assumed the perfection of the mirror and reflective null corrector, they rejected falsifying information from independent tests, believed no problems existed, and reported only good news."}}The commission blamed the failings primarily on Perkin-Elmer. Relations between NASA and the optics company had been severely strained during the telescope construction, due to frequent schedule slippage and cost overruns. NASA found that Perkin-Elmer did not review or supervise the mirror construction adequately, did not assign its best optical scientists to the project (as it had for the prototype), and in particular did not involve the optical designers in the construction and verification of the mirror. While the commission heavily criticized Perkin-Elmer for these managerial failings, NASA was also criticized for not picking up on the quality control shortcomings, such as relying totally on test results from a single instrument.{{sfn|Allen|Angel|Mangus|Rodney|1990|p=10-1}}

Design of a solution

(File:Hs-2009-25-e-full.jpg|thumb|upright|Some of the Carina nebula by WFC3)The design of the telescope had always incorporated servicing missions, and astronomers immediately began to seek potential solutions to the problem that could be applied at the first servicing mission, scheduled for 1993. While Kodak had ground a back-up mirror for Hubble, it would have been impossible to replace the mirror in orbit, and too expensive and time-consuming to bring the telescope back to Earth for a refit. Instead, the fact that the mirror had been ground so precisely to the wrong shape led to the design of new optical components with exactly the same error but in the opposite sense, to be added to the telescope at the servicing mission, effectively acting as "spectacles" to correct the spherical aberration.Chaisson, Eric (1994). The Hubble Wars; Astrophysics Meets Astropolitics in the Two-Billion-Dollar Struggle Over the Hubble Space Telescope. Harper Collins. {{ISBN|0-06-017114-6}}, p. 184.JOURNAL, Popular Science,weblink October 1990, The Trouble with Hubble, Arthur, Fisher, 100, November 8, 2012, The first step was a precise characterization of the error in the main mirror. Working backwards from images of point sources, astronomers determined that the conic constant of the mirror as built was {{val|−1.01390|0.0002|fmt=none}}, instead of the intended {{val|−1.00230|fmt=none}}.TECHREPORT, Image inversion analysis of the HST OTA (Hubble Space Telescope Optical Telescope Assembly), phase A, TRW, Inc. Space and Technology Group, M. M., Litvac, 1991, 1991trw..rept.....L, JOURNAL, Optical Prescription of the HST, Calibrating Hubble Space Telescope. Post Servicing Mission, 132,weblink 2014/31621, July 1995, NASA JPL, Redding, David C., Sirlin, S., Boden, A., Mo, J., Hanisch, B., Furey, L., dead,weblink" title="">weblink May 1, 2015, 1995chst.conf..132R, The same number was also derived by analyzing the null corrector used by Perkin-Elmer to figure the mirror, as well as by analyzing interferograms obtained during ground testing of the mirror.{{sfn|Allen|Angel|Mangus|Rodney|1990|pp=E-1}}(File:Feustel moving COSTAR.jpg|thumb|right|COSTAR being removed in 2009)Because of the way the HST's instruments were designed, two different sets of correctors were required. The design of the Wide Field and Planetary Camera 2, already planned to replace the existing WF/PC, included relay mirrors to direct light onto the four separate charge-coupled device (CCD) chips making up its two cameras. An inverse error built into their surfaces could completely cancel the aberration of the primary. However, the other instruments lacked any intermediate surfaces that could be figured in this way, and so required an external correction device.{{sfn|Tatarewicz|1998|p=376}}The Corrective Optics Space Telescope Axial Replacement (COSTAR) system was designed to correct the spherical aberration for light focused at the FOC, FOS, and GHRS. It consists of two mirrors in the light path with one ground to correct the aberration.JOURNAL, Jedrzejewski, RI, 1994, In-orbit performance of the COSTAR-corrected Faint Object Camera, Astrophysical Journal Letters, 435, L7–L10, Hartig, G, Jakobsen, P, Ford, HC, 1994ApJ...435L...7J, 10.1086/187581, To fit the COSTAR system onto the telescope, one of the other instruments had to be removed, and astronomers selected the High Speed Photometer to be sacrificed.{{sfn|Tatarewicz|1998|p=376}} By 2002, all of the original instruments requiring COSTAR had been replaced by instruments with their own corrective optics. COSTAR was removed and returned to Earth in 2009 where it is exhibited at the National Air and Space Museum. The area previously used by COSTAR is now occupied by the Cosmic Origins Spectrograph.WEB,weblink Hubble Essentials, STScI, November 8, 2012, {{clear}}

Servicing missions and new instruments

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BackgroundColors= canvas:lightGrayPeriod = from:1990 till:2016TimeAxis = orientation:horizontalScaleMajor= unit:year increment:5 start:1990 gridcolor:darkgrayPlotData=

from:1990 till:1993 color:Ren text:WFPC
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from:2009 till:end color:Cla text:WFC3


from:1990 till:1997 color:Ren text:GHRS
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from:1990 till:1993 color:Ren text:HSP
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from:1990 till:2002 color:Ren text:FOC
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from:1990 till:1997 color:Ren text:FOS
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Hubble was designed to accommodate regular servicing and equipment upgrades while in orbit. Instruments and limited life items were designed as orbital replacement units.weblink" title="">Orbital Replacement Units HST Five servicing missions (SM 1, 2, 3A, 3B, and 4) were flown by NASA space shuttles, the first in December 1993 and the last in May 2009.WEB,weblink The Secret to Hubble's Success, National Geographic, Jason, Treat, Anna, Scalamogna, Eve, Conant, 2015, April 25, 2015, Servicing missions were delicate operations that began with maneuvering to intercept the telescope in orbit and carefully retrieving it with the shuttle's mechanical arm. The necessary work was then carried out in multiple tethered spacewalks over a period of four to five days. After a visual inspection of the telescope, astronauts conducted repairs, replaced failed or degraded components, upgraded equipment, and installed new instruments. Once work was completed, the telescope was redeployed, typically after boosting to a higher orbit to address the orbital decay caused by atmospheric drag.WEB,weblink Hubble Reflects the Cosmos, The New York Times, Jason, Overbye, Jonathan, Corum, Jason, Drakeford, April 24, 2015, April 25, 2015,

Servicing Mission 1

(File:Upgrading Hubble during SM1.jpg|thumb|right|Astronauts Musgrave and Hoffman install corrective optics during SM1)After the problems with Hubble's mirror were discovered, the first servicing mission assumed greater importance, as the astronauts would need to do extensive work to install corrective optics. The seven astronauts for the mission were trained to use about a hundred specialized tools.{{sfn|Tatarewicz|1998|pp=384–387}} SM1 flew aboard Endeavour in December 1993, and involved installation of several instruments and other equipment over ten days.Most importantly, the High Speed Photometer was replaced with the COSTAR corrective optics package, and WFPC was replaced with the Wide Field and Planetary Camera 2 (WFPC2) with an internal optical correction system. The solar arrays and their drive electronics were also replaced, as well as four gyroscopes in the telescope pointing system, two electrical control units and other electrical components, and two magnetometers. The onboard computers were upgraded with added coprocessors, and Hubble's orbit was boosted.On January 13, 1994, NASA declared the mission a complete success and showed the first sharper images.JOURNAL, The on-orbit performance of WFPC2, Astrophysical Journal Letters, J. T., Trauger, G. E., Ballester, C. J., Burrows, S., Casertano, J. T., Clarke, D., Crisp, R. W., Evans, J. S., Gallagher III, R. E., Griffiths, 4, 435, L3–L6, 1994, 1994ApJ...435L...3T, 10.1086/187580, The mission was one of the most complex performed up until that date, involving five long extra-vehicular activity periods. Its success was a boon for NASA, as well as for the astronomers who now had a more capable space telescope.

Servicing Mission 2

(File:Hubble 01.jpg|thumb|Hubble as seen from Discovery during its second servicing mission)Servicing Mission 2, flown by Discovery in February 1997, replaced the GHRS and the FOS with the Space Telescope Imaging Spectrograph (STIS) and the Near Infrared Camera and Multi-Object Spectrometer (NICMOS), replaced an Engineering and Science Tape Recorder with a new Solid State Recorder, and repaired thermal insulation.WEB,weblink Servicing Mission 2, NASA, April 26, 2008,weblink" title="">weblink April 19, 2008, NICMOS contained a heat sink of solid nitrogen to reduce the thermal noise from the instrument, but shortly after it was installed, an unexpected thermal expansion resulted in part of the heat sink coming into contact with an optical baffle. This led to an increased warming rate for the instrument and reduced its original expected lifetime of 4.5 years to about 2 years.WEB,weblink NICMOS Thermal History, STScI, April 26, 2008,

Servicing Mission 3A

Servicing Mission 3A, flown by Discovery, took place in December 1999, and was a split-off from Servicing Mission 3 after three of the six onboard gyroscopes had failed. The fourth failed a few weeks before the mission, rendering the telescope incapable of performing scientific observations. The mission replaced all six gyroscopes, replaced a Fine Guidance Sensor and the computer, installed a Voltage/temperature Improvement Kit (VIK) to prevent battery overcharging, and replaced thermal insulation blankets.WEB,weblink Servicing Mission 3A Overview, NASA, April 26, 2008,

Servicing Mission 3B

Servicing Mission 3B flown by Columbia in March 2002 saw the installation of a new instrument, with the FOC (which, except for the Fine Guidance Sensors when used for astrometry, was the last of the original instruments) being replaced by the Advanced Camera for Surveys (ACS). This meant that COSTAR was no longer required, since all new instruments had built-in correction for the main mirror aberration.WEB, Corrective Optics Space Telescope Axial Replacement, HST,weblink STScI, November 4, 2012, The mission also revived NICMOS by installing a closed-cycle cooler and replaced the solar arrays for the second time, providing 30 percent more power.WEB,weblink Servicing Mission 3, NASA, April 26, 2008,weblink" title="">weblink April 7, 2008, {{clear}}

Servicing Mission 4

{{multiple image
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|caption1 = Hubble during Servicing Mission 4
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}}Plans called for Hubble to be serviced in February 2005, but the Columbia disaster in 2003, in which the orbiter disintegrated on re-entry into the atmosphere, had wide-ranging effects on the Hubble program. NASA Administrator Sean O'Keefe decided that all future shuttle missions had to be able to reach the safe haven of the International Space Station should in-flight problems develop. As no shuttles were capable of reaching both HST and the space station during the same mission, future crewed service missions were canceled.WEB,weblinkweblink" title="">weblink dead, May 30, 2012, Servicing Mission 4 Cancelled, STScI, January 16, 2004, April 28, 2008, This decision was criticised by numerous astronomers who felt that Hubble was valuable enough to merit the human risk.WEB,weblink Assessment of Options for Extending the Life of the Hubble Space Telescope: Final Report, The National Academies, 2005, Chapter 7, "Given the intrinsic value of a serviced Hubble, and the high likelihood of success for a shuttle servicing mission, the committee judges that such a mission is worth the risk." HST's planned successor, the James Webb Telescope (JWST), was not expected to launch until at least 2021. A gap in space-observing capabilities between a decommissioning of Hubble and the commissioning of a successor was of major concern to many astronomers, given the significant scientific impact of HST.WEB,weblink 2004 Annual Report, Astronomy and Astrophysics Advisory Committee, Section 3.1 â€“ The Scientific Impact of the HST SM4 Cancellation, March 15, 2004, November 5, 2012, The consideration that JWST will not be located in low Earth orbit, and therefore cannot be easily upgraded or repaired in the event of an early failure, only made concerns more acute. On the other hand, many astronomers felt strongly that the servicing of Hubble should not take place if the expense were to come from the JWST budget.In January 2004, O'Keefe said he would review his decision to cancel the final servicing mission to HST, due to public outcry and requests from Congress for NASA to look for a way to save it. The National Academy of Sciences convened an official panel, which recommended in July 2004 that the HST should be preserved despite the apparent risks. Their report urged "NASA should take no actions that would preclude a space shuttle servicing mission to the Hubble Space Telescope".NEWS,weblink Panel Urges NASA to Save Hubble Space Telescope, The New York Times, Warren E. Leary, July 14, 2004, November 8, 2012, In August 2004, O'Keefe asked Goddard Space Flight Center to prepare a detailed proposal for a robotic service mission. These plans were later canceled, the robotic mission being described as "not feasible".NEWS,weblink Nominee Backs a Review of NASA's Hubble Decision, Guy, Gugliotta, April 12, 2005, January 10, 2007, The Washington Post, In late 2004, several Congressional members, led by Senator Barbara Mikulski, held public hearings and carried on a fight with much public support (including thousands of letters from school children across the U.S.) to get the Bush Administration and NASA to reconsider the decision to drop plans for a Hubble rescue mission.PRESS RELEASE,weblink Mikulski Vows To Fight For Hubble, February 7, 2005, Barbara Mikulski, April 26, 2008,weblink" title="">weblink April 30, 2008, (File:218582main Batt FS img1 lg.jpg|thumb|Nickel–hydrogen battery pack for Hubble)The nomination in April 2005 of a new NASA Administrator with an engineering rather than accounting background, Michael D. Griffin, changed the situation, as Griffin stated he would consider a manned servicing mission.NEWS,weblink NASA gives green light to Hubble rescue, Alan, Boyle, MSNBC, October 31, 2006, January 10, 2007, Soon after his appointment Griffin authorized Goddard to proceed with preparations for a manned Hubble maintenance flight, saying he would make the final decision after the next two shuttle missions. In October 2006 Griffin gave the final go-ahead, and the 11-day mission by Atlantis was scheduled for October 2008. Hubble's main data-handling unit failed in September 2008,WEB,weblink Hubble suddenly quiet, Cowen, Ron, ScienceNews, September 29, 2008, November 8, 2012, halting all reporting of scientific data until its back-up was brought online on October 25, 2008.WEB,weblink Hubble re-opens an eye, Courtland, Rachel, New Scientist, October 28, 2008, October 29, 2008,weblink" title="">weblink October 29, 2008, Since a failure of the backup unit would leave the HST helpless, the service mission was postponed to incorporate a replacement for the primary unit.Servicing Mission 4 (SM4), flown by Atlantis in May 2009, was the last scheduled shuttle mission for HST.WEB,weblink NASA Sets Target Shuttle Launch Date for Hubble Servicing Mission, NASA, December 4, 2008, December 5, 2008, SM4 installed the replacement data-handling unit, repaired the ACS and STIS systems, installed improved nickel hydrogen batteries, and replaced other components. SM4 also installed two new observation instruments—Wide Field Camera 3 (WFC3) and the Cosmic Origins Spectrograph (COS)WEB,weblink Hubble Opens New Eyes on the Universe, NASA, September 9, 2009, May 28, 2012, —and the Soft Capture and Rendezvous System, which will enable the future rendezvous, capture, and safe disposal of Hubble by either a crewed or robotic mission.WEB,weblink The Soft Capture and Rendezvous System, NASA, May 20, 2009, Except for the ACS's High Resolution Channel, which could not be repaired and was disabled,NEWS,weblink After Hubble Repair, New Images From Space, The New York Times, Dennis, Overbye, September 9, 2009, August 1, 2015, NEWS,weblink After a Yank, 'Surgery' on Hubble Optics, The New York Times, Dennis, Overbye, May 17, 2009, August 1, 2015, WEB,weblink Repair of the Advanced Camera for Surveys,, August 1, 2015, the work accomplished during SM4 rendered the telescope fully functional, and it remains so {{as of|2019|lc=y}}.WEB,weblink This week on HST, Space Telescope Science Institute, January 2, 2017, January 23, 2017,

Major projects

File:Pillars of creation 2014 HST WFC3-UVIS full-res denoised.jpg|thumb|One of Hubble's most famous images, Pillars of Creation, shows stars forming in the Eagle NebulaEagle NebulaSince the start of the program, a number of research projects have been carried out, some of them almost solely with Hubble, others coordinated facilities such as Chandra X-ray Observatory and ESO's Very Large Telescope. Although the Hubble observatory is nearing the end of its life, there are still major projects scheduled for it. One example is the upcoming Frontier Fields program,WEB,weblink Hubble Deep Fields Initiative 2012 Science Working Group Report,, 2012, June 29, 2015, inspired by the results of Hubble's deep observation of the galaxy cluster Abell 1689.WEB,weblink New Hubble image of galaxy cluster Abell 1689,, heic1317, September 12, 2013, October 4, 2013,

Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

In an August 2013 press release, CANDELS was referred to as "the largest project in the history of Hubble". The survey "aims to explore galactic evolution in the early Universe, and the very first seeds of cosmic structure at less than one billion years after the Big Bang."WEB,weblink Hubble explores the origins of modern galaxies,, heic1315, August 15, 2013, October 4, 2013, The CANDELS project site describes the survey's goals as the following:WEB,weblink Survey Description, CANDELS,, October 4, 2013, dead,weblink" title="">weblink October 20, 2013, The Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey is designed to document the first third of galactic evolution from z = 8 to 1.5 via deep imaging of more than 250,000 galaxies with WFC3/IR and ACS. It will also find the first Type Ia SNe beyond z > 1.5 and establish their accuracy as standard candles for cosmology. Five premier multi-wavelength sky regions are selected; each has multi-wavelength data from Spitzer and other facilities, and has extensive spectroscopy of the brighter galaxies. The use of five widely separated fields mitigates cosmic variance and yields statistically robust and complete samples of galaxies down to 109 solar masses out to z ~ 8.

Frontier Fields program

File:Color image of galaxy cluster MCS J0416.1–2403.jpg|thumb|right|alt=Color image of galaxy cluster MCS J0416.1–2403, studied by the Hubble Frontier Fields program|The Frontier Fields program studied MACS0416.1-2403MACS0416.1-2403The program, officially named "Hubble Deep Fields Initiative 2012", is aimed to advance the knowledge of early galaxy formation by studying high-redshift galaxies in blank fields with the help of gravitational lensing to see the "faintest galaxies in the distant universe." The Frontier Fields web page describes the goals of the program being:
  • to reveal hitherto inaccessible populations of z = 5–10 galaxies that are 10 to 50 times fainter intrinsically than any presently known
  • to solidify our understanding of the stellar masses and star formation histories of sub-L galaxies at the earliest times
  • to provide the first statistically meaningful morphological characterization of star forming galaxies at z > 5
  • to find z > 8 galaxies stretched out enough by cluster lensing to discern internal structure and/or magnified enough by cluster lensing for spectroscopic follow-up.WEB,weblink Hubble Space Telescope: Frontier Fields,, October 4, 2013,

Cosmic Evolution Survey (COSMOS)

The Cosmic Evolution Survey (COSMOS)WEB,weblink Cosmic Evolution Survey (COSMOS), is an astronomical survey designed to probe the formation and evolution of galaxies as a function of both cosmic time (redshift) and the local galaxy environment. The survey covers a 2 square degree equatorial field with spectroscopy and X-ray to radio imaging by most of the major space-based telescopes and a number of large ground based telescopes,WEB,weblink COSMOS Data Description For Astronomers, making it a key focus region of extragalactic astrophysics. COSMOS was launched in 2006 as the largest project pursued by the Hubble Space Telescope at the time, and still is the largest continuous area of sky covered for the purposes of mapping deep space in blank fields, 2.5 times the area of the moon on the sky and 17 times larger than the largest of the CANDELS regions. The COSMOS scientific collaboration that was forged from the initial COSMOS survey is the largest and longest-running extragalactic collaboration, known for its collegiality and openness. The study of galaxies in their environment can only be done with large areas of the sky, larger than a half square degree.WEB,weblink HUBBLE MAPS THE COSMIC WEB OF "CLUMPY" DARK MATTER IN 3-D, Over 2 million galaxies are detected, spanning 90% of the age of the Universe. The COSMOS collaboration is led by Caitlin Casey, Jeyhan Kartaltepe, and Vernesa Smolcic and involves more than 200 scientists in a dozen countries.WEB,weblink Cosmic Evolution Survey (COSMOS),

Public use

File:EmissionNebula NGC6357.jpg|thumb|upright|Star cluster Pismis 24 with nebula ]]


Anyone can apply for time on the telescope; there are no restrictions on nationality or academic affiliation, but funding for analysis is only available to US institutions.{{sfn|Strolger|Rose|2017|p=11}} Competition for time on the telescope is intense, with about one-fifth of the proposals submitted in each cycle earning time on the schedule.WEB,weblink HST Overview, NASA, June 21, 2010, November 4, 2012, Mission Operations and Observations, WEB,weblink Team Hubble, STScI, November 5, 2012, Each year more than 1,000 proposals are reviewed and approximately 200 are selected.,


Calls for proposals are issued roughly annually, with time allocated for a cycle lasting about one year. Proposals are divided into several categories; "general observer" proposals are the most common, covering routine observations. "Snapshot observations" are those in which targets require only 45 minutes or less of telescope time, including overheads such as acquiring the target. Snapshot observations are used to fill in gaps in the telescope schedule that cannot be filled by regular GO programs.{{sfn|Strolger|Rose|2017|p=21}}Astronomers may make "Target of Opportunity" proposals, in which observations are scheduled if a transient event covered by the proposal occurs during the scheduling cycle. In addition, up to 10% of the telescope time is designated "director's discretionary" (DD) time. Astronomers can apply to use DD time at any time of year, and it is typically awarded for study of unexpected transient phenomena such as supernovae.{{sfn|Strolger|Rose|2017|p=37}}Other uses of DD time have included the observations that led to views of the Hubble Deep Field and Hubble Ultra Deep Field, and in the first four cycles of telescope time, observations that were carried out by amateur astronomers.Public image processing of Hubble data is encouraged as most of the data in the archives has not been processed into color imagery.WEB,weblink Hubble Image Processors: Raiders of the Hubble Archive,, November 23, 2016,

Use by amateur astronomers

(File:Hubble Space Telescope, time exposure May 4, 2018.jpg|thumb|upright|The HST is sometimes visible from the ground, as in this 10-second exposure.)The first director of STScI, Riccardo Giacconi, announced in 1986 that he intended to devote some of his director discretionary time to allowing amateur astronomers to use the telescope. The total time to be allocated was only a few hours per cycle but excited great interest among amateur astronomers.WEB,weblink Amateur Astronomers Will Use NASA's Hubble Space Telescope, STScI, September 10, 1992, April 26, 2008, Proposals for amateur time were stringently reviewed by a committee of amateur astronomers, and time was awarded only to proposals that were deemed to have genuine scientific merit, did not duplicate proposals made by professionals, and required the unique capabilities of the space telescope. Thirteen amateur astronomers were awarded time on the telescope, with observations being carried out between 1990 and 1997.JOURNAL,weblink The Demise of the HST Amateur Program, Sky & Telescope, Stephen James, O'Meara, Edwin L., Aguirre, 96, 6, 97, June 1997, 1997S&T....93f..97O, One such study was "Transition Comets—UV Search for OH". The very first proposal, "A Hubble Space Telescope Study of Posteclipse Brightening and Albedo Changes on Io", was published in Icarus,JOURNAL, A Hubble Space Telescope Study of Posteclipse Brightening and Albedo Changes on Io, Icarus, James J., Secosky, Michael, Potter, 111, 1, 73–78, September 1994, 10.1006/icar.1994.1134, 1994Icar..111...73S, a journal devoted to solar system studies. A second study from another group of amateurs was also published in Icarus.JOURNAL,weblink Imaging Observations of Asteroids with Hubble Space Telescope, Icarus, Alex, Storrs, Ben, Weiss, Ben, Zellner, Win, Burleson, Rukmini, Sichitiu, Eddie, Wells, Charles, Kowal, David, Tholen, 4, 137, 2, 260–268, February 1999, 10.1006/icar.1999.6047, 1999Icar..137..260S, dead,weblink" title="">weblink February 25, 2012, After that time, however, budget reductions at STScI made the support of work by amateur astronomers untenable, and no additional amateur programs have been carried out.NEWS,weblink Open Mic Night at the Hubble Telescope, Motherboard, Matthew, Walthert, April 24, 2015, April 25, 2015, {{clear}}

Scientific results

File:NASA-HubbleLegacyFieldZoomOut-20190502.webm|thumb|upright=2.7|center|Hubble space telescope - (Hubble ultra deep field|Ultra deep field galaxies]] to Legacy field zoom out (video 00:50; May 2, 2019))

Key projects

In the early 1980s, NASA and STScI convened four panels to discuss key projects. These were projects that were both scientifically important and would require significant telescope time, which would be explicitly dedicated to each project. This guaranteed that these particular projects would be completed early, in case the telescope failed sooner than expected. The panels identified three such projects: 1) a study of the nearby intergalactic medium using quasar absorption lines to determine the properties of the intergalactic medium and the gaseous content of galaxies and groups of galaxies;JOURNAL, Bahcall, JN, Bergeron, J, Boksenberg, A, Hartig, GF, Jannuzi, BT, Kirhakos, S, Sargent, WLW, Savage, BD, Schneider, DP, 8, The Hubble Space Telescope Quasar Absorption Line Key Project. I. First Observational Results, Including Lyman-Alpha and Lyman-Limit Systems, The Astrophysical Journal Supplement Series, 87, 1–43, 0067-0049, 1993, 1993ApJS...87....1B, 10.1086/191797, 2) a medium deep survey using the Wide Field Camera to take data whenever one of the other instruments was being usedJOURNAL, The Hubble Space Telescope Medium Deep Survey Cluster Sample: Methodology and Data,weblink Ostrander, EJ, Nichol, RC, Kavan Ratnatunga, Ratnatunga, KU, Griffiths, RE, The Astronomical Journal, 116, 6, 2644–2658, 1998, 10.1086/300627, 1998AJ....116.2644O, astro-ph/9808304, and 3) a project to determine the Hubble constant within ten percent by reducing the errors, both external and internal, in the calibration of the distance scale.WEB,weblink The Hubble Constant, January 11, 2011, John Huchra, Huchra, John,

Important discoveries

(File:Saturn.Aurora.HST.UV-Vis.jpg|thumb|Hubble's STIS UV and ACS visible light are combined to reveal Saturn's southern aurora.)Hubble has helped resolve some long-standing problems in astronomy, while also raising new questions. Some results have required new theories to explain them.

Age of the universe

Among its primary mission targets was to measure distances to Cepheid variable stars more accurately than ever before, and thus constrain the value of the Hubble constant, the measure of the rate at which the universe is expanding, which is also related to its age. Before the launch of HST, estimates of the Hubble constant typically had errors of up to 50%, but Hubble measurements of Cepheid variables in the Virgo Cluster and other distant galaxy clusters provided a measured value with an accuracy of ±10%, which is consistent with other more accurate measurements made since Hubble's launch using other techniques.JOURNAL, 2001ApJ...553...47F, Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant, Freedman, W. L., Madore, B. F., Gibson, B.K., Ferrarese, L., Kelson, D. D., Sakai, S., Mould, J. R., Kennicutt, R. C. Jr., etal, The Astrophysical Journal, 553, 1, 47–72, 10.1086/320638, 2001, astro-ph/0012376, Preprint available here. The estimated age is now about 13.7 billion years, but before the Hubble Telescope, scientists predicted an age ranging from 10 to 20 billion years.WEB,weblink 25 of the Greatest Hubble Telescope Discoveries From the Past 25 Years, World Science Festival, Roxanne, Palmer, April 24, 2015, February 23, 2016, dead,weblink" title="">weblink March 6, 2016,

Expansion of the universe

While Hubble helped to refine estimates of the age of the universe, it also cast doubt on theories about its future. Astronomers from the High-z Supernova Search Team and the Supernova Cosmology Project used ground-based telescopes and HST to observe distant supernovae and uncovered evidence that, far from decelerating under the influence of gravity, the expansion of the universe may in fact be accelerating. Three members of these two groups have subsequently been awarded Nobel Prizes for their discovery.BOOK, Cosmology, Steven, Weinberg, Oxford University Press, 2008, 9780198526827, The cause of this acceleration remains poorly understood;JOURNAL,weblink Does Dark Energy Really Exist?, Clifton, Timothy, Ferreira, Pedro G, Scientific American, March 23, 2009, June 16, 2009, the most common cause attributed is dark energy.JOURNAL, Science, June 20, 2003, 300, 12817137, 5627, 1896–1897, 10.1126/science.300.5627.1896, Dark Energy Tiptoes Toward the Spotlight, Charles, Seife, File:Jupiter showing SL9 impact sites.jpg|thumb|right|Brown spots mark Comet Shoemaker–Levy 9 impact sites on JupiterJupiter

Black holes

The high-resolution spectra and images provided by the HST have been especially well-suited to establishing the prevalence of black holes in the nuclei of nearby galaxies. While it had been hypothesized in the early 1960s that black holes would be found at the centers of some galaxies, and astronomers in the 1980s identified a number of good black hole candidates, work conducted with Hubble shows that black holes are probably common to the centers of all galaxies.WEB,weblink Hubble Confirms Existence of Massive Black Hole at Heart of Active Galaxy, Goddard Space Flight Center, May 25, 1994, April 26, 2008, JOURNAL, A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion, 4, Gebhardt, K, Bender, R, Bower, G, Dressler, A, Faber, SM, Filippenko, AV, Green, R, Grillmair, C, Ho, LC, Kormendy, J, The Astrophysical Journal, 539, L13–L16, 2000, 10.1086/312840, 1, 2000ApJ...539L..13G, astro-ph/0006289, JOURNAL, A Fundamental Relationship between Supermassive Black Holes and their Host Galaxies, Ferrarese, Laura, Merritt, David, David Merritt, The Astrophysical Journal, 539, L9–L12, 2000, 2000ApJ...539L...9F, 10.1086/312838, 1, astro-ph/0006053, The Hubble programs further established that the masses of the nuclear black holes and properties of the galaxies are closely related. The legacy of the Hubble programs on black holes in galaxies is thus to demonstrate a deep connection between galaxies and their central black holes.

Extending visible wavelength images

File:Hubble Extreme Deep Field (full resolution).png|thumb|Hubble Extreme Deep Field image of space in the constellation FornaxFornaxA unique window on the Universe enabled by Hubble are the Hubble Deep Field, Hubble Ultra-Deep Field, and Hubble Extreme Deep Field images, which used Hubble's unmatched sensitivity at visible wavelengths to create images of small patches of sky that are the deepest ever obtained at optical wavelengths. The images reveal galaxies billions of light years away, and have generated a wealth of scientific papers, providing a new window on the early Universe. The Wide Field Camera 3 improved the view of these fields in the infrared and ultraviolet, supporting the discovery of some of the most distant objects yet discovered, such as MACS0647-JD.The non-standard object SCP 06F6 was discovered by the Hubble Space Telescope in February 2006.JOURNAL,weblink How they wonder what you are, Nature News, September 19, 2008, November 4, 2012, Brumfiel, Geoff, 10.1038/news.2008.1122, JOURNAL, Gänsicke, BT, Levan, AJ, Marsh, TR, Wheatley, PJ, SCP06F6: A carbon-rich extragalactic transient at redshift z~0.14?, 2009, The Astrophysical Journal, 10.1088/0004-637X/697/2/L129, 0809.2562, 697, 1, L129–L132, 2009ApJ...697L.129G, On March 3, 2016, researchers using Hubble data announced the discovery of the farthest known galaxy to date: GN-z11. The Hubble observations occurred on February 11, 2015, and April 3, 2015, as part of the CANDELS/GOODS-North surveys.WEB,weblink Hubble Team Breaks Cosmic Distance Record,, March 3, 2016, March 3, 2016, STScI-2016-07, NEWS,weblink Hubble Spies Most Distant, Oldest Galaxy Ever, Discovery News, Irene, Klotz, March 3, 2016, March 3, 2016,

Solar system discoveries

HST has also been used to study objects in the outer reaches of the Solar System, including the dwarf planets PlutoAPOD, March 11, 1996, Hubble Telescope Maps Pluto, April 26, 2008, and Eris.PRESS RELEASE,weblink Astronomers Measure Mass of Largest Dwarf Planet, STScI, June 14, 2007, April 26, 2008, The collision of Comet Shoemaker-Levy 9 with Jupiter in 1994 was fortuitously timed for astronomers, coming just a few months after Servicing Mission 1 had restored Hubble's optical performance. Hubble images of the planet were sharper than any taken since the passage of Voyager 2 in 1979, and were crucial in studying the dynamics of the collision of a comet with Jupiter, an event believed to occur once every few centuries. During June and July 2012, US astronomers using Hubble discovered a tiny fifth moon orbiting around Pluto.NEWS,weblinkweblink" title="">weblink dead, January 26, 2013, Hubble discovers fifth and tiniest Pluto moon, The Indian Express, July 12, 2012, In March 2015, researchers announced that measurements of aurorae around Ganymede, one of Jupiter's moons, revealed that it has a subsurface ocean. Using Hubble to study the motion of its aurorae, the researchers determined that a large saltwater ocean was helping to suppress the interaction between Jupiter's magnetic field and that of Ganymede. The ocean is estimated to be {{convert|100|km|mi|-1|abbr=on}} deep, trapped beneath a {{convert|150|km|mi|-1|abbr=on}} ice crust.PRESS RELEASE,weblink NASA's Hubble Observations Suggest Underground Ocean on Jupiter's Largest Moon, Space Telescope Science Institute, March 12, 2015, March 13, 2015, JOURNAL, The search for a subsurface ocean in Ganymede with Hubble Space Telescope observations of its auroral ovals, Journal of Geophysical Research, Joachim, Saur, Stefan, Duling, Lorenz, Roth, Xianzhe, Jia, Darrell F., Strobel, Paul D., Feldman, Ulrich R., Christensen, Kurt D., Retherford, Melissa A., McGrath, Fabrizio, Musacchio, Alexandre, Wennmacher, Fritz M., Neubauer, Sven, Simon, Oliver, Hartkorn, 4, 120, 3, March 2015, 10.1002/2014JA020778, 2015JGRA..120.1715S, 1715–1737,weblink File:Hubble and ALMA image of MACS J1149.5+2223.jpg|thumb|Hubble and ALMA image of MACS J1149.5+2223MACS J1149.5+2223

Supernova reappearance

On December 11, 2015, Hubble captured an image of the first-ever predicted reappearance of a supernova, dubbed "Refsdal", which was calculated using different mass models of a galaxy cluster whose gravity is warping the supernova's light. The supernova was previously seen in November 2014 behind galaxy cluster MACS J1149.5+2223 as part of Hubble's Frontier Fields program. Astronomers spotted four separate images of the supernova in an arrangement known as an Einstein Cross. The light from the cluster has taken about five billion years to reach Earth, though the supernova exploded some 10 billion years ago. The detection of Refsdal's reappearance served as a unique opportunity for astronomers to test their models of how mass, especially dark matter, is distributed within this galaxy cluster.WEB,weblink Caught in the act: Hubble captures first-ever predicted exploding star,, December 16, 2015, December 19, 2015,

Mass and size of Milky Way

In March 2019, observations from Hubble and data from the European Space Agency's Gaia space observatory were combined to determine that the Milky Way Galaxy weighs approximately 1.5 trillion solar units and has a radius of 129,000 light years.WEB,weblink Hubble and Gaia accurately weigh the Milky Way, March 7, 2019,, March 20, 2019,

Other discoveries

Other discoveries made with Hubble data include proto-planetary disks (proplyds) in the Orion Nebula;WEB,weblink Hubble Confirms Abundance of Protoplanetary Disks around Newborn Stars, STScI, June 13, 1994, April 26, 2008, evidence for the presence of extrasolar planets around Sun-like stars;WEB,weblink Hubble Finds Extrasolar Planets Far Across Galaxy, NASA, October 4, 2006, April 26, 2008, and the optical counterparts of the still-mysterious gamma-ray bursts.WEB,weblink Autopsy of an Explosion, NASA, March 26, 1999, April 26, 2008, dead,weblink April 15, 2008,

Impact on astronomy

File:Hubble Probes the Early Universe.jpg|thumb|upright=1.5|alt=Depiction of progress in the detection of the early Universe|Evolution of detecting the early Universe ]]Many objective measures show the positive impact of Hubble data on astronomy. Over 15,000 papers based on Hubble data have been published in peer-reviewed journals,WEB,weblink HST Publication Statistics, STScI, December 26, 2017, and countless more have appeared in conference proceedings. Looking at papers several years after their publication, about one-third of all astronomy papers have no citations, while only 2% of papers based on Hubble data have no citations. On average, a paper based on Hubble data receives about twice as many citations as papers based on non-Hubble data. Of the 200 papers published each year that receive the most citations, about 10% are based on Hubble data.JOURNAL,weblink Hubble Science Metrics, Newsletter, Space Telescope Science Institute, Georges, Meylan, Juan, Madrid, Duccio, Macchetto, 20, 2, Spring 2003, Although the HST has clearly helped astronomical research, its financial cost has been large. A study on the relative astronomical benefits of different sizes of telescopes found that while papers based on HST data generate 15 times as many citations as a {{convert|4|m|ft|abbr=on|adj=on}} ground-based telescope such as the William Herschel Telescope, the HST costs about 100 times as much to build and maintain.JOURNAL, Benn, CR, Sánchez, SF, 2001, Scientific Impact of Large Telescopes, Publications of the Astronomical Society of the Pacific, 113, 781, 385–396, 10.1086/319325, 2001PASP..113..385B, astro-ph/0010304, Deciding between building ground- versus space-based telescopes is complex. Even before Hubble was launched, specialized ground-based techniques such as aperture masking interferometry had obtained higher-resolution optical and infrared images than Hubble would achieve, though restricted to targets about 108 times brighter than the faintest targets observed by Hubble.JOURNAL, 1987Natur.328..694H, Haniff, CA, 4, Mackay, CD, Titterington, DJ, Sivia, D, Baldwin, JE, The first images from optical aperture synthesis, Nature (journal), Nature, 328, August 1987, 6132, 694–696, 10.1038/328694a0, JOURNAL, 1990MNRAS.245P...7B, Buscher, DF, Baldwin, JE, Warner, PJ, Haniff, CA, Detection of a bright feature on the surface of Betelgeuse, Monthly Notices of the Royal Astronomical Society, 245, July 1990, 7, Since then, advances in adaptive optics have extended the high-resolution imaging capabilities of ground-based telescopes to the infrared imaging of faint objects. The usefulness of adaptive optics versus HST observations depends strongly on the particular details of the research questions being asked. In the visible bands, adaptive optics can only correct a relatively small field of view, whereas HST can conduct high-resolution optical imaging over a wide field. Only a small fraction of astronomical objects are accessible to high-resolution ground-based imaging; in contrast Hubble can perform high-resolution observations of any part of the night sky, and on objects that are extremely faint.

Impact on aerospace engineering

In addition to its scientific results, Hubble has also made significant contributions to aerospace engineering, in particular the performance of systems in low Earth orbit. These insights result from Hubble's long lifetime on orbit, extensive instrumentation, and return of assemblies to the Earth where they can be studied in detail. In particular, Hubble has contributed to studies of the behavior of graphite composite structures in vacuum, optical contamination from residual gas and human servicing, radiation damage to electronics and sensors, and the long term behavior of multi-layer insulation.JOURNAL, Experience with the Hubble Space Telescope: 20 years of an archetype, Optical Engineering, Matthew D., Lallo, 51, 1, 011011, January 2012, 10.1117/1.OE.51.1.011011, 2012OptEn..51a1011L, 1203.0002, One lesson learned was that gyroscopes assembled using pressurized oxygen to deliver suspension fluid were prone to failure due to electric wire corrosion. Gyroscopes are now assembled using pressurized nitrogen.

Hubble data

File:Hubble stretches the stellar tape measure ten times further.jpg|thumb|Hubble precision stellar distance measurement has been extended 10 times further into the Milky WayMilky Way

Transmission to Earth

Hubble data was initially stored on the spacecraft. When launched, the storage facilities were old-fashioned reel-to-reel tape recorders, but these were replaced by solid state data storage facilities during servicing missions 2 and 3A. About twice daily, the Hubble Space Telescope radios data to a satellite in the geosynchronous Tracking and Data Relay Satellite System (TDRSS), which then downlinks the science data to one of two 60-foot (18-meter) diameter high-gain microwave antennas located at the White Sands Test Facility in White Sands, New Mexico.WEB,weblink Team Hubble, STScI, Data Management, November 5, 2012, From there they are sent to the Space Telescope Operations Control Center at Goddard Space Flight Center, and finally to the Space Telescope Science Institute for archiving. Each week, HST downlinks approximately 140 gigabits of data.

Color images

(File:Cumulative-absorption-spectrum-hubble-telescope.jpg|thumb|right|Data analysis of a spectrum reveals the chemistry of hidden clouds)All images from Hubble are monochromatic grayscale, taken through a variety of filters, each passing specific wavelengths of light, and incorporated in each camera. Color images are created by combining separate monochrome images taken through different filters. This process can also create false-color versions of images including infrared and ultraviolet channels, where infrared is typically rendered as a deep red and ultraviolet is rendered as a deep blue.WEB,weblink The Secret Science of the Hubble Space Telescope's Amazing Images,, Rosen, Raphael, July 24, 2013, July 26, 2013, AV MEDIA,weblink Iconic Space Images Are Actually Black-and-White, National Geographic, March 15, 2015, March 27, 2015, WEB,weblink How Hubble Sees, Nova ScienceNow, PBS, Jeff, Hester, July 1, 2008, August 17, 2015,


All Hubble data is eventually made available via the Mikulski Archive for Space Telescopes at STScI,WEB,weblink The Hubble Telescope, STScI, April 26, 2008, CADCWEB,weblink CADC's Hubble Space Telescope Archive, CADC, April 26, 2008, and ESA/ESAC.WEB,weblink European HST Archive at ESA/ESAC, ESA/ESAC, February 14, 2013, dead,weblink" title="">weblink May 25, 2013, Data is usually proprietary—available only to the principal investigator (PI) and astronomers designated by the PI—for six months after being taken. The PI can apply to the director of the STScI to extend or reduce the proprietary period in some circumstances.{{sfn|Strolger|Rose|2017|p=53}}Observations made on Director's Discretionary Time are exempt from the proprietary period, and are released to the public immediately. Calibration data such as flat fields and dark frames are also publicly available straight away. All data in the archive is in the FITS format, which is suitable for astronomical analysis but not for public use.{{sfn|Rose|2017|p=69}} The Hubble Heritage Project processes and releases to the public a small selection of the most striking images in JPEG and TIFF formats.WEB,weblink The Hubble Heritage Project, STScI, November 5, 2012,

Pipeline reduction

Astronomical data taken with CCDs must undergo several calibration steps before they are suitable for astronomical analysis. STScI has developed sophisticated software that automatically calibrates data when they are requested from the archive using the best calibration files available. This 'on-the-fly' processing means that large data requests can take a day or more to be processed and returned. The process by which data is calibrated automatically is known as 'pipeline reduction', and is increasingly common at major observatories. Astronomers may if they wish retrieve the calibration files themselves and run the pipeline reduction software locally. This may be desirable when calibration files other than those selected automatically need to be used.{{sfn|Rose|2017|pp=67–69}}

Data analysis

Hubble data can be analyzed using many different packages. STScI maintains the custom-made Space Telescope Science Data Analysis System (STSDAS) software, which contains all the programs needed to run pipeline reduction on raw data files, as well as many other astronomical image processing tools, tailored to the requirements of Hubble data. The software runs as a module of IRAF, a popular astronomical data reduction program.{{sfn|Rose|2017|pp=68–69}}

Outreach activities

File:Horsehead-Hubble.jpg|thumb|In 2001, NASA polled internet users to find out what they would most like Hubble to observe; they overwhelmingly selected the Horsehead NebulaHorsehead Nebula
missing image!
- Hubble Space Telescope Scale Model.JPG -
A 1/4 scale model of the Hubble Space Telescope located at the courthouse in Marshfield, Missouri, a hometown of telescope namesake Edwin Hubble
It has always been important for the Space Telescope to capture the public's imagination, given the considerable contribution of taxpayers to its construction and operational costs.WEB,weblink National Aeronautics and Space Administration 2003 Strategic Plan, NASA, November 5, 2012,weblink" title="">weblink November 16, 2012, After the difficult early years when the faulty mirror severely dented Hubble's reputation with the public, the first servicing mission allowed its rehabilitation as the corrected optics produced numerous remarkable images.Several initiatives have helped to keep the public informed about Hubble activities.In the United States, outreach efforts are coordinated by the Space Telescope Science Institute (STScI) Office for Public Outreach, which was established in 2000 to ensure that U.S. taxpayers saw the benefits of their investment in the space telescope program. To that end, STScI operates the website. The Hubble Heritage Project, operating out of the STScI, provides the public with high-quality images of the most interesting and striking objects observed. The Heritage team is composed of amateur and professional astronomers, as well as people with backgrounds outside astronomy, and emphasizes the aesthetic nature of Hubble images. The Heritage Project is granted a small amount of time to observe objects which, for scientific reasons, may not have images taken at enough wavelengths to construct a full-color image.{{anchor|Hubblecast}}Since 1999, the leading Hubble outreach group in Europe has been the Hubble European Space Agency Information Centre (HEIC).WEB,weblink The European Homepage for the NASA/ESA Hubble Space Telescope, European Space Agency, April 26, 2008, This office was established at the Space Telescope European Coordinating Facility in Munich, Germany. HEIC's mission is to fulfill HST outreach and education tasks for the European Space Agency. The work is centered on the production of news and photo releases that highlight interesting Hubble results and images. These are often European in origin, and so increase awareness of both ESA's Hubble share (15%) and the contribution of European scientists to the observatory. ESA produces educational material, including a videocast series called Hubblecast designed to share world-class scientific news with the public.WEB,weblink Hubblecast, European Space Agency, April 26, 2015, The Hubble Space Telescope has won two Space Achievement Awards from the Space Foundation, for its outreach activities, in 2001 and 2010.PRESS RELEASE,weblink Historic Hubble Space Telescope Repair Mission Team Honored by the Space Foundation with 2010 Space Achievement Award, 26th National Space Symposium, March 29, 2010, November 5, 2012,weblink" title="">weblink March 6, 2012, A replica of the Hubble Space Telescope is on the courthouse lawn in Marshfield, Missouri, the hometown of namesake Edwin P. Hubble.

Celebration images

{{Further|List of Hubble anniversary images}}File:HH 901 and HH 902 in the Carina nebula (captured by the Hubble Space Telescope).jpg|thumb|A pillar of gas and dust in the Carina Nebula. This Wide Field Camera 3 image, dubbed Mystic MountainMystic MountainThe Hubble Space Telescope celebrated its 20th anniversary in space on April 24, 2010. To commemorate the occasion, NASA, ESA, and the Space Telescope Science Institute (STScI) released an image from the Carina Nebula.PRESS RELEASE,weblink Starry-Eyed Hubble Celebrates 20 Years of Awe and Discovery, Space Telescope Science Institute, April 22, 2010, November 4, 2012, To commemorate Hubble's 25th anniversary in space on April 24, 2015, STScI released images of the Westerlund 2 cluster, located about {{convert|20000|ly|pc}} away in the constellation Carina, through its Hubble 25 website.WEB,weblink 25th Anniversary Image: Westerlund 2, Space Telescope Science Institute, April 24, 2015, The European Space Agency created a dedicated 25th anniversary page on its website.WEB,weblink Celebrating 25 years of the NASA/ESA Hubble Space Telescope, European Space Agency, April 24, 2015, In April 2016, a special celebratory image of the Bubble Nebula was released for Hubble's 26th "birthday".WEB,weblink Hubble captures birthday bubble,, European Space Agency, April 21, 2016, December 15, 2016,

Equipment failures

Gyroscope rotation sensors

HST uses gyroscopes to detect and measure any rotations so it can stabilize itself in orbit and point accurately and steadily at astronomical targets. Three gyroscopes are normally required for operation; observations are still possible with two or one, but the area of sky that can be viewed would be somewhat restricted, and observations requiring very accurate pointing are more difficult.WEB,weblink HST Two-Gyro Handbook, Sembach, K. R., October 2004, Space Telescope Science Institute, Baltimore, etal, 1.0, In 2018, the plan is to drop into one-gyroscope mode if less than three working gyroscopes are operational. The gyroscopes are part of the Pointing Control System, which uses five types of sensors (magnetic sensors, optical sensors, and the gyroscopes) and two types of actuators (reaction wheels and magnetic torquers).WEB,weblink Hubble Space Telescope Pointing Control System, NASA, October 24, 2018, Hubble carries six gyroscopes in total.After the Columbia disaster in 2003, it was unclear whether another servicing mission would be possible, and gyroscope life became a concern again, so engineers developed new software for two-gyroscope and one-gyroscope modes to maximize the potential lifetime. The development was successful, and in 2005, it was decided to switch to two-gyroscope mode for regular telescope operations as a means of extending the lifetime of the mission. The switch to this mode was made in August 2005, leaving Hubble with two gyroscopes in use, two on backup, and two inoperable.WEB,weblink Hubble Space Telescope Begins 'Two-Gyro' Science Operations, NASA, Dolores, Beasley, Susan, Hendrix, Donna, Weaver, August 31, 2005, February 8, 2019, One more gyroscope failed in 2007.NEWS,weblink Hubble telescope loses another gyroscope, New Scientist, Jeff, Hecht, September 6, 2007, January 6, 2009, By the time of the final repair mission in May 2009, during which all six gyroscopes were replaced (with two new pairs and one refurbished pair), only three gyroscopes were still working. Engineers determined that the gyroscope failures were caused by corrosion of electric wires powering the motor that was initiated by oxygen-pressurized air used to deliver the thick suspending fluid.WEB,weblink Gyroscopes, ESA, June 9, 2012, The new gyroscope models were assembled using pressurized nitrogen and they should be much more reliable.NEWS,weblink Endeavour to go Nov. 14; Hubble slips deeper into '09, Spaceflight Now, William, Harwood, October 30, 2008, January 6, 2009, In the 2009 servicing mission all six gyroscopes were replaced, and after almost ten years only three gryoscopes failed, but only after exceeding the average expected run time for the design.WEB,weblink Update on the Hubble Space Telescope Safe Mode, NASA, Garner, Rob, October 8, 2018, October 15, 2018, Of the six gyroscopes replaced in 2009, three were of the old design susceptible for flex-lead failure, and three were of the new design with a longer expected lifetime. The first of the old-style gyroscopes failed in March 2014, and the second in April 2018. On October 5, 2018, the last of the old-style gyroscopes failed, and one of the new-style gyroscopes was powered-up from standby state. However, that reserve gyroscope did not immediately perform within operational limits, and so the observatory was placed into "safe" mode while scientists attempted to fix the problem.NEWS,weblink Hubble telescope hit by mechanical failure, BBC News, Paul, Rincon, October 8, 2018, October 10, 2018, NEWS,weblink NASA makes progress on fixing Hubble gyro, Space News, Jeff, Foust, October 22, 2018, NASA tweeted on October 22, 2018, that the "rotation rates produced by the backup gyro have reduced and are now within a normal range. Additional tests {{interp|are}} to be performed to ensure Hubble can return to science operations with this gyro."NEWS,weblink What fixed NASA's Hubble Space Telescope? Someone flipped a switch on and off, USA Today, Brett, Molina, October 24, 2018, February 8, 2019, The solution that restored the backup new-style gyroscope to operational range was widely reported as "turning it off and on again".NEWS,weblink No, NASA didn't fix the Hubble Telescope by just turning it off and on again, The Washington Post, Amy B., Wang, October 24, 2018, February 8, 2019, A "running restart" of the gyroscope was performed, but this had no effect, and the final resolution to the failure was more complex. The failure was attributed to an inconsistency in the fluid surrounding the float within the gyroscope (e.g., an air bubble). On October 18, 2018, the Hubble Operations Team directed the spacecraft into a series of maneuvers – moving the spacecraft in opposite directions – in order to mitigate the inconsistency. Only after the maneuvers, and a subsequent set of maneuvers on October 19, did the gyroscope truly operate within its normal range.WEB,weblink NASA's Hubble Space Telescope Returns to Science Operations, NASA, Felicia, Chou, October 27, 2018, February 8, 2019, File:Formalhaut b.jpg|thumb|left|Hubble views the FomalhautFomalhaut

Instruments and electronics

Past servicing missions have exchanged old instruments for new ones, avoiding failure and making new types of science possible. Without servicing missions, all of the instruments will eventually fail. In August 2004, the power system of the Space Telescope Imaging Spectrograph (STIS) failed, rendering the instrument inoperable. The electronics had originally been fully redundant, but the first set of electronics failed in May 2001.WEB,weblink Space Telescope Imaging Spectrograph, STScI, April 26, 2008, This power supply was fixed during Servicing Mission 4 in May 2009.Similarly, the Advanced Camera for Surveys (ACS) main camera primary electronics failed in June 2006, and the power supply for the backup electronics failed on January 27, 2007.WEB,weblink Engineers Investigate Issue on One of Hubble's Science Instruments, January 29, 2007, NASA, April 26, 2008, Only the instrument's Solar Blind Channel (SBC) was operable using the side-1 electronics. A new power supply for the wide angle channel was added during SM 4, but quick tests revealed this did not help the high resolution channel.WEB,weblink Advanced Camera for Surveys, STScI, May 21, 2009, The Wide Field Channel (WFC) was returned to service by STS-125 in May 2009 but the High Resolution Channel (HRC) remains offline.NEWS,weblink Part of camera in newly repaired instrument revived, Harwood, William, May 17, 2009, Spaceflight Now, May 17, 2009,weblink" title="">weblink May 20, 2009, On January 8, 2019, Hubble entered a partial safe mode following suspected hardware problems in its most advanced instrument, the Wide Field Camera 3 instrument. NASA later reported that the cause of the safe mode within the instrument was a detection of voltage levels out of a defined range. On January 15, 2019, NASA stated that the cause of the failure was a software problem. Engineering data within the telemetry circuits were not accurate. In addition, all other telemetry within those circuits also contained erroneous values indicating that this was a telemetry issue and not a power supply issue. After resetting the telemetry circuits and associated boards the instrument began functioning again. On January 17, 2019, the device was returned to normal operation and on the same day it completed its first science observations.WEB,weblink Hubble's Wide Field Camera 3 Recovered, Collecting Science Data, Gutro, Rob, January 17, 2019, NASA, NEWS,weblink Hubble's Wide Field Camera 3 resumes operations, Kornfeld, Laurel, January 17, 2019, Spaceflight Insider,


Orbital decay and controlled reentry

(File:Soft Capture Mechanism installed on Hubble (illustration).jpg|thumb|Illustration of the Soft Capture Mechanism (SCM) installed on Hubble)Hubble orbits the Earth in the extremely tenuous upper atmosphere, and over time its orbit decays due to drag. If not reboosted, it will re-enter the Earth's atmosphere within some decades, with the exact date depending on how active the Sun is and its impact on the upper atmosphere. If Hubble were to descend in a completely uncontrolled re-entry, parts of the main mirror and its support structure would probably survive, leaving the potential for damage or even human fatalities.NEWS,weblink Why Hubble is being dropped, BBC News, David, Whitehouse, January 17, 2004, January 10, 2007, In 2013, deputy project manager James Jeletic projected that Hubble could survive into the 2020s.WEB,weblink Four years after final service call, Hubble Space Telescope going strong, CBS News, William, Harwood, May 30, 2013, June 3, 2013, Based on solar activity and atmospheric drag, or lack thereof, a natural atmospheric reentry for Hubble will occur between 2028 and 2040.NEWS,weblink How Will the Hubble Space Telescope Die?,, Mike, Wall, April 24, 2015, May 16, 2017, In June 2016, NASA extended the service contract for Hubble until June 2021.PRESS RELEASE,weblink NASA Extends Hubble Space Telescope Science Operations Contract, NASA, Northon, Karen, June 23, 2016, June 26, 2016, NASA's original plan for safely de-orbiting Hubble was to retrieve it using a space shuttle. Hubble would then have most likely been displayed in the Smithsonian Institution. This is no longer possible since the space shuttle fleet has been retired, and would have been unlikely in any case due to the cost of the mission and risk to the crew. Instead, NASA considered adding an external propulsion module to allow controlled re-entry.NEWS,weblink Keith, Cowing, NASA Considering Deletion of Hubble Deorbit Module, July 22, 2005, January 10, 2007, SpaceRef, Ultimately, in 2009, as part of Servicing Mission 4, the last servicing mission by the Space Shuttle, NASA installed the Soft Capture Mechanism (SCM), to enable deorbit by either a crewed or robotic mission. The SCM, together with the Relative Navigation System (RNS), mounted on the Shuttle to collect data to "enable NASA to pursue numerous options for the safe de-orbit of Hubble", constitute the Soft Capture and Rendezvous System (SCRS).WEB,weblink Team Hubble: Servicing Missions,, October 24, 2018,

Possible commercial service missions

{{As of|2017}}, the Trump Administration is considering a proposal by the Sierra Nevada Corporation to use a manned version of its Dream Chaser spacecraft to service Hubble some time in the 2020s both as a continuation of its scientific capabilities and as insurance against any malfunctions in the to-be-launched James Webb Space Telescope.NEWS,weblink A New Spaceship Could Fly Astronauts to the Hubble Space Telescope for Repairs, Popular Mechanics, Jay, Bennett, February 14, 2017, February 15, 2017,


{{further|James Webb Space Telescope}}{| class="wikitable" style="text-align:center; float:right; margin:10px" Visible spectrum range !Color|Wavelengthviolet|380–450 nmblue|450–475 nmcyan|476–495 nmgreen|495–570 nmyellow|570–590 nmorange|590–620 nmred|620–750 nmThere is no direct replacement to Hubble as an ultraviolet and visible light space telescope, because near-term space telescopes do not duplicate Hubble's wavelength coverage (near-ultraviolet to near-infrared wavelengths), instead concentrating on the farther infrared bands. These bands are preferred for studying high redshift and low-temperature objects, objects generally older and farther away in the universe. These wavelengths are also difficult or impossible to study from the ground, justifying the expense of a space-based telescope. Large ground-based telescopes can image some of the same wavelengths as Hubble, sometimes challenge HST in terms of resolution by using adaptive optics (AO), have much larger light-gathering power, and can be upgraded more easily, but cannot yet match Hubble's excellent resolution over a wide field of view with the very dark background of space.Plans for a Hubble successor materialized as the Next Generation Space Telescope project, which culminated in plans for the James Webb Space Telescope (JWST), the formal successor of Hubble.WEB,weblink Last Dance with the Shuttle: What's in Store for the Final Hubble Servicing Mission, John, Matson, May 8, 2009, Scientific American, May 18, 2009, Very different from a scaled-up Hubble, it is designed to operate colder and farther away from the Earth at the L2 Lagrangian point, where thermal and optical interference from the Earth and Moon are lessened. It is not engineered to be fully serviceable (such as replaceable instruments), but the design includes a docking ring to enable visits from other spacecraft.WEB,weblink Brian, Berger, NASA Adds Docking Capability For Next Space Observatory,, May 23, 2007, June 4, 2012, A main scientific goal of JWST is to observe the most distant objects in the universe, beyond the reach of existing instruments. It is expected to detect stars in the early Universe approximately 280 million years older than stars HST now detects.PRESS RELEASE,weblink NASA's Hubble Finds Most Distant Galaxy Candidate Ever Seen in Universe, NASA, January 26, 2011, June 4, 2012, Visual representation. The telescope is an international collaboration between NASA, the European Space Agency, and the Canadian Space Agency since 1996,WEB,weblinkweblink" title="">weblink dead, August 21, 2003, ESA JWST Timeline,, June 30, 2003, June 4, 2012, and is planned for launch on an Ariane 5 rocket.WEB,weblink About Webb's Launch, NASA, November 4, 2006, Although JWST is primarily an infrared instrument, its coverage extends down to 600 nm wavelength light, or roughly orange in the visible spectrum. A typical human eye can see to about 750 nm wavelength light, so there is some overlap with the longest visible wavelength bands, including orange and red light.(File:JWST-HST-primary-mirrors.svg|left|thumb|Hubble and JWST mirrors (4.5 m2 and 25 m2 respectively))A complementary telescope, looking at even longer wavelengths than Hubble or JWST, was the European Space Agency's Herschel Space Observatory, launched on May 14, 2009. Like JWST, Herschel was not designed to be serviced after launch, and had a mirror substantially larger than Hubble's, but observed only in the far infrared and submillimeter. It needed helium coolant, of which it ran out on April 29, 2013.{| class=wikitable style="text-align:center; float:right; margin:10px"Selected space telescopes and instrumentsHTTP://HERSCHEL.JPL.NASA.GOV/RELATEDMISSIONS.SHTML >TITLE=JPL: HERSCHEL SPACE OBSERVATORY: RELATED MISSIONS ACCESSDATE=JUNE 4, 2012, ! Name !! Year || Wavelength || Aperture| 0.01 mSpitzer Space Telescope>Spitzer 2003 3–180 μm 0.85 m| 2.4 m| 2.4 mHerschel Space Observatory>Herschel 2009 55–672 μm 3.5 mJames Webb Space Telescope>JWST Planned 0.6–28.5 μm 6.5 mFurther concepts for advanced 21st-century space telescopes include the Advanced Technology Large-Aperture Space Telescope,"What Will Astronomy Be Like in 35 Years?". Astronomy. August 2008. a conceptualized {{convert|8|to|16.8|m|in |abbr=off|sp=us}} optical space telescope that if realized could be a more direct successor to HST, with the ability to observe and photograph astronomical objects in the visible, ultraviolet, and infrared wavelengths, with substantially better resolution than Hubble or the Spitzer Space telescope. This effort is being planned for the 2025–2035 time frame.Existing ground-based telescopes, and various proposed Extremely Large Telescopes, can exceed the HST in terms of sheer light-gathering power and diffraction limit due to larger mirrors, but other factors affect telescopes. In some cases, they may be able to match or beat Hubble in resolution by using adaptive optics (AO). However, AO on large ground-based reflectors will not make Hubble and other space telescopes obsolete. Most AO systems sharpen the view over a very narrow field—Lucky Cam, for example, produces crisp images just 10" to 20" wide, whereas Hubble's cameras produce crisp images across a 2½' (150") field. Furthermore, space telescopes can study the universe across the entire electromagnetic spectrum, most of which is blocked by Earth's atmosphere. Finally, the background sky is darker in space than on the ground, because air absorbs solar energy during the day and then releases it at night, producing a faint—but nevertheless discernible—airglow that washes out low-contrast astronomical objects.NEWS,weblink Sharpening the 200-Inch, Sky & Telescope, Richard, Tresch Fienberg, September 14, 2007, July 1, 2008,

See also




  • WEB,weblinkweblink" title="">weblink dead, May 27, 2008, Hubble Space Telescope Call for Proposals for Cycle 25, Space Telescope Science Institute, Louis-Gregory, Strolger, Susan, Rose, January 2017, harv, April 16, 2008,
  • WEB,weblink Hubble Space Telescope Primer for Cycle 25, Space Telescope Science Institute, Susan, Rose, January 2017, harv, September 7, 2019,
  • JOURNAL,weblink The Hubble Space Telescope Optical Systems Failure Report, NASA Sti/Recon Technical Report N, 91, 12437, NASA, Lew, Allen, Roger, Angel, John D., Mangus, George A., Rodney, Robert R., Shannon, Charles P., Spoelhof, 4, November 1990, 1990STIN...9112437., NASA TM-103443, harv, The definitive report on the error in the Hubble mirror.
  • BOOK,weblink The Hubble Space Telescope, Power to Explore: History of Marshall Space Flight Center 1960–1990, NASA, Andrew J., Dunar, Stephen P., Waring, 1999, 978-0-16-058992-8, harv, Covers the development of the telescope.
  • BOOK,weblink Exploring the Unknown: Selected Documents in the History of the U.S. Civil Space Program. Volume V: Exploring the Cosmos, NASA History Series, NASA, John M., Logsdon, Amy Paige, Snyder, Roger D., Launius, Stephen J., Garber, Regan Anne, Newport, 2001, 978-0-16-061774-4, NASA SP-2001-4407, harv, Contains many of the primary documents such as Spitzer's 1946 article, the Wood's Hole report on STScI autonomy, and the ESA memorandum of understanding. Also includes other NASA astronomy programs.
  • JOURNAL, History of the Space Telescope, Quarterly Journal of the Royal Astronomical Society, Lyman S., Spitzer, 20, 29–36, March 1979, 1979QJRAS..20...29S, harv, Covers the early history of precursors and proposals.
  • BOOK,weblink The Hubble Space Telescope Servicing Mission, From Engineering Science to Big Science, NASA History Series, NASA, Joseph N., Tatarewicz, Pamela E., Mack, 1998, 978-0-16-049640-0, NASA SP-1998-4219, harv, A detailed account of the first servicing mission.

Further reading

  • WEB,weblink Report of the HST-JWST Transition Panel, NASA, John N., Bahcall, Barry C., Barish, Jacqueline N., Hewitt, Christopher F., McKee, Martin, Rees, Charles, Townes, 4, August 2003,
  • NEWS,weblink What went wrong with the Hubble Space Telescope (and what managers can learn from it), Techworld, Rohan, Pearce, March 29, 2012, March 30, 2012,
  • BOOK, The Universe in a Mirror: The Saga of the Hubble Space Telescope and the Visionaries Who Built It, Princeton University Press, Robert F., Zimmerman, 2010, 978-0-691-14635-5,

External links

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