Hubble Space Telescope 
The Hubble Space Telescope as seen from the departing Space Shuttle Atlantis, flying Servicing Mission 4 (STS-125), the fifth and final human spaceflight to visit the observatory. |
| General information |
| NSSDC ID | 1990-037B |
| Organization | NASA / ESA / STScI |
| Launch date | April 24, 1990, 8:33:51 am EDT[1] |
| Launch vehicle | Space Shuttle Discovery (STS-31) |
| Mission length | 20 years, 9 months, and 26 days elapsed |
| Deorbited | due ~2013–2021[2][3] |
| Mass | 11,110 kg (24,500 lb) |
| Type of orbit | Near-circular low Earth orbit |
| Orbit height | 559 km (347 mi) |
| Orbit period | 96–97 minutes (14-15 periods per day) |
| Orbit velocity | 7,500 m/s (25,000 ft/s) |
| Acceleration due to gravity | 8.169 m/s2 (26.80 ft/s2) |
| Location | Low Earth orbit |
| Telescope style | Ritchey-Chrétien reflector |
| Wavelength | Optical, ultraviolet, near-infrared |
| Diameter | 2.4 m (7 ft 10 in) |
| Collecting area | 4.5 m2 (48 sq ft)[4] |
| Focal length | 57.6 m (189 ft) |
| Instruments |
| NICMOS | infrared camera/spectrometer |
| ACS | optical survey camera
(partially failed) |
| WFC3 | wide field optical camera |
| COS | ultraviolet spectrograph |
| STIS | optical spectrometer/camera |
| FGS | three fine guidance sensors |
| Website | hubble.nasa.gov
hubblesite.org
www.spacetelescope.org |
The
Hubble Space Telescope (
HST) is a
space telescope that was carried into
orbit by a
space shuttle in 1990. Although not the first space telescope, Hubble 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 HST was built by the United States space agency
NASA, with contributions from the
European Space Agency, and is operated by the
Space Telescope Science Institute. It is named after the
astronomer Edwin Hubble. The HST is one of NASA's
Great Observatories, along with the
Compton Gamma Ray Observatory, the
Chandra X-ray Observatory, and the
Spitzer Space Telescope.
[5]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. When finally launched in 1990, scientists found that the main mirror had been ground incorrectly, severely compromising the telescope's capabilities. However, after a servicing mission in 1993, the telescope was restored to its intended quality. Hubble's orbit outside the distortion of
Earth's atmosphere allows it to take extremely sharp images with almost no
background light. Hubble's
Ultra Deep Field image, for instance, is the most detailed
visible-light image ever made of the universe's most distant objects. Many Hubble observations have led to breakthroughs in
astrophysics, such as accurately
determining the rate of expansion of the universe.
Hubble is the only telescope designed to be serviced in space by astronauts. Four servicing missions were performed from 1993 to 2002, but the fifth was canceled on safety grounds following the
Space Shuttle Columbia disaster. However, after
spirited public discussion, NASA administrator
Mike Griffin approved
one final servicing mission, completed in 2009. The telescope is now expected to function until at least 2014, when its scientific successor, the
James Webb Space Telescope (JWST), is due to be launched.
Contents- 1 Conception, design and aims
- 1.1 Proposals and precursors
- 1.2 Quest for funding
- 1.3 Construction and engineering
- 1.4 Optical Telescope Assembly (OTA)
- 1.5 Spacecraft systems
- 1.6 Initial instruments
- 1.7 Ground support
- 1.8 Challenger disaster, delays, and eventual launch
- 2 Flawed mirror
- 2.1 Origin of the problem
- 2.2 Design of a solution
- 3 Servicing missions and new instruments
- 3.1 Servicing Mission 1
- 3.2 Servicing Mission 2
- 3.3 Servicing Mission 3A
- 3.4 Servicing Mission 3B
- 3.5 Servicing Mission 4
- 4 Scientific results
- 4.1 Key Projects
- 4.2 Important discoveries
- 4.3 Impact on astronomy
- 5 Usage
- 5.1 Amateur observations
- 5.2 20th birthday
- 6 Hubble data
- 6.1 Transmission to Earth
- 6.2 Archives
- 6.3 Pipeline reduction
- 6.4 Data analysis
- 7 Outreach activities
- 8 Future
- 8.1 Equipment failure
- 8.2 Orbital decay
- 8.3 Debate over final servicing mission
- 8.4 Planned successors
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Conception, design and aims
Proposals and precursors
In 1923,
Hermann Oberth—considered along with
Robert H. Goddard and
Konstantin Tsiolkovsky fathers of modern rocketry—published
Die Rakete zu den Planetenräumen ("The Rocket into Planetary Space"), which mentioned how a telescope could be propelled into Earth orbit by a rocket.
[6]The history of the Hubble Space Telescope can be traced back as far as 1946, when the
astronomer Lyman Spitzer wrote the paper "Astronomical advantages of an extraterrestrial observatory".
[7] In it, he discussed the two main advantages that a space-based observatory would have over ground-based telescopes. First, the
angular resolution (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 and is 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 2.5 m 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 a space telescope to be developed. In 1962 a report by the
United States 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 the scientific objectives for a large space telescope.
[8]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,
[9] and NASA launched the
Orbiting Solar Observatory to obtain UV, X-ray, and gamma-ray spectra in 1962.
[10] An orbiting solar telescope was launched in 1962 by the United Kingdom as part of the
Ariel space program, and in 1966
National Aeronautics and Space Administration (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.
[11]The OSO and OAO missions demonstrated the important role space-based observations could play in astronomy, and 1968 saw the development by NASA of firm plans for a space-based
reflecting telescope with a mirror 3 m 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.
[12]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
US 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 instigated by
Gerald Ford led to Congress cutting all funding for the telescope project.
[13]In response to this, 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.
[14]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 costs
[15] and to allow a more compact and effective configuration for the telescope hardware. A proposed precursor 1.5 m 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.
[16] Congress eventually approved funding of
US$36,000,000 for 1978, and the design of the LST began in earnest, aiming for a launch date of 1983.
[14] In 1983 the telescope was named
[17] after
Edwin Hubble, who made one of the greatest scientific breakthroughs of the 20th century when he discovered that the
universe is
expanding.
[18]Construction and engineering
Polishing of Hubble's primary mirror begins at
Perkin-Elmer corporation,
Danbury,
Connecticut, March 1979. The engineer pictured is Dr. Martin Yellin, an optical engineer working for Perkin-Elmer on the project.
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 the
Goddard Space Flight Center was given overall control of the scientific instruments and ground-control center for the mission.
[19] 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.
[20]Optical Telescope Assembly (OTA)
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 10
nanometres, or about 1/65 of the wavelength of red light.
[21] 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 °C) temperatures by heaters. This limits Hubble's performance as an infrared telescope.
[22]Perkin-Elmer intended to use custom-built and extremely sophisticated
computer-controlled polishing machines to grind the mirror to the required shape.
[20] 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.
[23] (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.
[24]) The Kodak mirror is now on permanent display at the
Smithsonian Institution.
[25][26] An Itek mirror built as part of the effort is now used in the 2.4 m telescope at the
Magdalena Ridge Observatory.
[27]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 inch-thick top and bottom plates sandwiching a
honeycomb lattice. Perkin-Elmer simulated
microgravity by supporting the mirror on both sides with 138 rods that exerted varying amounts of force. 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.
[28] The mirror was completed by the end of 1981; it was washed using 2,400 gallons (9,100 L) of hot,
deionized water and then received a reflective coating of
aluminium 65 nm-thick and a protective coating of
magnesium fluoride 25 nm-thick.
[22][29]
Construction of Hubble. The optical metering truss and secondary baffle are visible.
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 first March and then September 1986. By this time the total project budget had risen to US$1.175 billion.
[30]Spacecraft systems
The spacecraft in which the telescope and instruments were to be housed was another major engineering challenge. It would have to adequately withstand frequent passages from direct sunlight into the darkness of Earth's
shadow, which would generate 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.
[31] 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; the telescope's instruments would be covered in ice. To reduce that risk, a nitrogen gas purge was performed prior to launching the telescope into space.
[32]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.
[33]Initial instruments
When 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. 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.
[34]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.
[35] 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 the
Martin Marietta corporation built the FOS.
[34]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.
[36]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.
[37]Ground support
Hubble's low orbit means many targets are visible for somewhat less than half of elapsed time, since they are blocked from view by the
Earth for one-half of each orbit.
The
Space Telescope Science Institute (
STSI) is responsible for the scientific operation of the telescope and 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 33 US universities and 7 international affiliates that make up the AURA consortium. STScI was established in 1981
[38] 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.
[39][40] The
Space Telescope European Coordinating Facility (ST-ECF), established at
Garching bei München near
Munich in 1984, provides similar support for European astronomers.
One rather complex task that falls to STScI is scheduling observations for the telescope.
[41] Hubble is situated in a low-Earth orbit so that it can be reached by the space shuttle for 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°, which is specified to keep sunlight from illuminating any part of the OTA. Earth and Moon avoidance is to keep bright light out of the FGSs and to keep 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 degrees 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
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.
Because Hubble orbits in the upper atmosphere, 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 4,000 km. 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.
[42]Engineering support for HST is provided by NASA and contractor personnel at the Goddard Space Flight Center in
Greenbelt, Maryland, 48 km 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.
[43]Challenger disaster, delays, and eventual launch
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 $6 million per month) pushed the overall costs of the project even higher. On the other hand, engineers used this time to perform extensive tests, swap out a possibly failure-prone battery, and make other improvements.
[44] Furthermore, the ground software needed to control Hubble was not ready in 1986, and in fact was barely ready by the 1990 launch.
[45]
Shuttle mission
STS-31 lifts off, carrying Hubble into orbit.
Eventually, following the resumption of shuttle flights in 1988, the launch of the telescope was scheduled for 1990. On April 24, 1990, shuttle mission
STS-31 saw
Discovery launch the telescope successfully into its planned orbit.
[46]From its original total cost estimate of about US$400 million, the telescope had by now cost over $2.5 billion to construct. Hubble's cumulative costs up to this day are estimated to be several times higher still, with US expenditure estimated at between $4.5 and $6 billion, and Europe's financial contribution at €593 million (1999 estimate).
[47]Flawed mirror
Within weeks of the launch of the telescope, the returned images showed that there was a serious problem with the optical system. Although the first images appeared to be sharper than ground-based images, the telescope 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.
[48] The detailed performance is shown in graphs from STScI illustrating the mis-
figured PSFs compared to post-correction and ground-based PSFs.
[49]Analysis of the flawed images showed that the cause of the problem was that the primary mirror had been ground to the wrong shape. Although it was probably the most precisely figured mirror ever made, with variations from the prescribed curve of only 10 nanometers,
[21] it was too flat at the edges by about 2200 nanometers (2.2
microns).
[50] 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.
[51]
Hubble is deployed from
Discovery.
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 was largely unaffected. 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.
[51] 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, the Hubble was pictured with the
Titanic, the
Hindenburg, and the
Edsel).
[52] 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. The error was well characterized and stable, enabling astronomers to optimize the results obtained using sophisticated
image processing techniques such as
deconvolution.
[53]Origin of the problem
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.
The correctly ground backup mirror built by Eastman Kodak for the Hubble space telescope (the mirror was never coated with a reflective surface, hence its inner support structure can be seen). It now resides in the
National Air and Space Museum in Washington, DC.
[54]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 the main
null corrector, a device used to measure the exact shape of the mirror, had been incorrectly assembled—one lens was wrongly spaced by 1.3 mm.
[55] During the polishing of the mirror, Perkin-Elmer had analyzed its surface with two other null correctors, both of which correctly indicated that the mirror was suffering from
spherical aberration. The company ignored these test results, as it believed that the two null correctors were less accurate than the primary device that was reporting that the mirror was perfectly figured.
[56]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.
[57]Design of a solution
COSTAR on display at the National Air and Space Museum
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 and Itek had each ground back-up mirrors for Hubble, it would have been impossible to replace the mirror in orbit, and too expensive and time-consuming to bring the telescope temporarily 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.
[58][59]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 −1.01390±0.0002, instead of the intended −1.00230.
[60][61] 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.
[62]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 eight separate
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.
[63]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.
[64] 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.
[63] By 2002 all of the original instruments requiring COSTAR had been replaced by instruments with their own corrective optics.
[65] 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.
Servicing missions and new instruments
Servicing Mission 1
Astronauts Musgrave and Hoffman installing corrective optics during SM1
Improvement in Hubble images after SM1
Hubble on the payload bay just prior to release during SM3B
The telescope had always been designed so that it could be regularly serviced, but after the problems with the mirror came to light, the first servicing mission assumed a much greater importance, as the astronauts would have to carry out extensive work on the telescope to install the corrective optics. The seven astronauts selected for the mission were trained intensively in the use of the hundred or more specialized tools that would be needed.
[66] The
Space Shuttle Endeavour mission
STS-61 took place in December 1993, and involved installation of several instruments and other
equipment over a total of 10 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 its internal optical correction system. In addition, the
solar arrays and their drive electronics were replaced, as well as four of the
gyroscopes used in the telescope pointing system, two electrical control units and other electrical components, and two magnetometers. The onboard computers were upgraded, and finally, the telescope's orbit was boosted, to compensate for the orbital decay from 3 years of
drag in the tenuous upper atmosphere.
[50]On January 13, 1994, NASA declared the mission a complete success and showed the first of many much sharper images.
[67] At the time, the mission had been one of the most complex ever undertaken, involving five lengthy periods of
extra-vehicular activity, and its resounding success was an enormous boon for NASA, as well as for the astronomers who now had a fully capable space telescope.
Servicing Mission 2
Servicing Mission 2, flown by
Discovery (
STS-82) 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, repaired thermal insulation and again boosted Hubble's orbit.
[68] 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.
[69]Servicing Mission 3A
Servicing Mission 3A flown by
Discovery (
STS-103), took place in December 1999, and was a split-off from Servicing Mission 3 after three of the six onboard gyroscopes had failed. (A fourth failed a few weeks before the mission, rendering the telescope incapable of performing science 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.
[70] Although the new computer is hardly a powerhouse (a 25 MHz
radiation hardened Intel 486 with two megabytes of RAM), it is still 20 times faster, with six times more memory, than the
DF-224 it replaced. The new computer increases throughput by moving some computing tasks from the ground to the spacecraft, and saves money by allowing the use of modern programming languages.
[71]Servicing Mission 3B
Servicing Mission 3B flown by
Columbia (
STS-109) in March 2002 saw the installation of a new instrument, with the FOC (the last original instrument) being replaced by the
Advanced Camera for Surveys (ACS). This meant that COSTAR was no longer required, since all new instruments had correction for the main mirror aberration built in.
[65]The mission also saw the revival of NICMOS, which had run out of
coolant in 1999. A new cooling system was installed that reduced the instrument's temperature enough for it to be usable again. Although not as cold as its original design called for, the temperature is more stable, in many ways a better tradeoff.
[69] ACS in particular enhanced Hubble's capabilities; it and the revived NICMOS together imaged the
Hubble Ultra Deep Field.
The mission replaced the solar arrays for the second time. The new arrays were derived from those built for the
Iridium comsat system and were only two-thirds the size of the old arrays, resulting in less drag against the tenuous reaches of the upper atmosphere while providing 30 percent more power. The additional power allowed all instruments on board the HST to be run simultaneously, and reduced a vibration problem that occurred when the old, less rigid arrays entered and left direct sunlight. Hubble's Power Distribution Unit was also replaced in order to correct a problem with sticky relays, a procedure that required the complete electrical power down of the spacecraft for the first time since it was launched.
[72]Servicing Mission 4
Astronauts work on Hubble during SM4
Hubble floats free from
Atlantis after SM4.
Servicing Mission 4 (SM4), which took place in May 2009, was the last scheduled shuttle mission (
STS-125) for the Hubble Space Telescope.
[73] The mission was first planned for October 14, 2008.
[74] However on September 27, 2008, the Science Instrument Command and Data Handling (SI C&DH) unit on HST failed. All science data pass through this unit before they can be transmitted to Earth. Although it had a backup unit, if the backup were to fail, the HST's useful life would be over.
[75] Therefore on September 29, 2008, NASA announced that the launch of SM4 would be postponed until 2009 so the SI C&DH unit could be replaced as well.
[76] SM4, with a replacement SI C&DH unit,
[77] was launched aboard
Space Shuttle Atlantis on May 11, 2009.
[78]On SM4, astronauts, over the course of five spacewalks, installed two new instruments,
Wide Field Camera 3 (WFC3), and the
Cosmic Origins Spectrograph (COS). WFC3 will increase Hubble's observational capabilities in the ultraviolet and visible spectral ranges by up to 35 times due to its higher sensitivity and wider field of view. The telephone-booth sized COS assembly replaced the Corrective Optics Space Telescope Axial Replacement (COSTAR) that was installed in 1993 to correct Hubble's spherical aberration problems. (COSTAR was no longer needed after the replacement of the
FOC in 2002, the last original instrument without the necessary correction built in.
[65]) The COS will do observations in the ultraviolet parts of the spectrum, complementing the measurements done by the repaired STIS system.
The mission repaired two instruments that had failed, the
Advanced Camera for Surveys (ACS) and the
Space Telescope Imaging Spectrograph (STIS). The astronauts also performed other component replacements, including all three Rate Sensor Units (each containing two gas-bearing gyroscopes); one of three Fine Guidance Sensor (FGS) units used to help keep pointing accuracy and increase platform stability; the SI C&DH unit; all six of the 125-pound (57 kg) nickel-hydrogen batteries used to provide all Hubble's electrical power to support operations during the night portion of its orbit; and three New Outer Blanket Layer (NOBL) thermal insulation protective blankets. The batteries had never been replaced and were more than 13 years over their original design life.
[79]Atlantis released the Hubble Space Telescope on May 19, 2009 back into space after all repairs were successfully made. After testing and calibration, Hubble resumed routine operation in September 2009.
[80] These efforts are expected to keep the telescope fully functioning at least into 2014, and perhaps longer.
[81]Hubble was originally designed to be returned to earth on board a shuttle. With the
retirement of the shuttle fleet, projected for 2011, this will no longer be possible. NASA engineers developed the Soft Capture and Rendezvous System (SCRS), a ring-like device that was attached to Hubble’s aft bulkhead during SM4, which will enable the future
rendezvous, capture, and safe disposal of Hubble by either a
crewed or
robotic mission.
[82] The next mission will be to deorbit Hubble at the end of its service life.
Scientific results
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;
[83] (2) a medium deep survey using the Wide Field Camera to take data whenever one of the other instruments was being used
[84] 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.
[85]Important discoveries
Hubble has helped to resolve some long-standing problems in astronomy, as well as turning up results that have required new
theories to explain them. 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.
[86]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[87] used the telescope 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. This acceleration was later measured more accurately by other ground-based and space-based telescopes, confirming Hubble's finding. The cause of this acceleration remains poorly understood;
[88] the most common cause attributed is
dark energy.
[89]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 work in the 1980s identified a number of good black hole candidates, it fell to work conducted with Hubble to show that black holes are probably common to the centers of all galaxies.
[90][91][92] 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.
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.
Other major discoveries made using Hubble data include proto-planetary disks (
proplyds) in the
Orion Nebula;
[93] evidence for the presence of
extrasolar planets around sun-like stars;
[94] and the optical counterparts of the still-mysterious
gamma ray bursts.
[95] HST has also been used to study objects in the outer reaches of the Solar System, including the dwarf planets
Pluto[96] and
Eris.
[97]A unique legacy of Hubble are the
Hubble Deep Field and
Hubble Ultra Deep Field images, which utilized 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 non-standard object
SCP 06F6 was discovered by the Hubble Space Telescope (HST) in February 2006.
[98][99]Impact on astronomy
Many objective measures show the positive impact of Hubble data on astronomy. Over 9,000 papers based on Hubble data have been published in peer-reviewed journals,
[100] 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.
[101]Although the HST has clearly had a significant impact on astronomical research, the financial cost of this impact has been large. A study on the relative impacts on astronomy of different sizes of telescopes found that while papers based on HST data generate 15 times as many citations as a 4 m ground-based telescope such as the
William Herschel Telescope, the HST costs about 100 times as much to build and maintain.
[102]Making the decision between investing in ground-based versus space-based telescopes in the future 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 10
8 times brighter than the faintest targets observed by Hubble.
[103][104] 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.
Usage
To consummate Hubble Telescope's 20th Birthday, NASA, along with ESA and Space Telescope Institute, released a findings from Hubble.
Anyone can apply for time on the telescope; there are no restrictions on nationality or academic affiliation.
[105] Competition for time on the telescope is intense, and the ratio of time requested to time available (the oversubscription ratio) typically ranges between 6 and 9.
[106]Calls for proposals are issued roughly annually, with time allocated for a cycle lasting approximately 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.
[107]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.
[108] Other uses of DD time have included the observations that led to the production of the Hubble Deep Field and Hubble Ultra Deep Field, and in the first four cycles of telescope time, observations carried out by amateur astronomers.
Amateur observations
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.
[109]Proposals for amateur time were stringently
peer reviewed by a committee of leading 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. In total, 13 amateur astronomers were awarded time on the telescope, with observations being carried out between 1990 and 1997. One such study was
Transition Comets — UV Search for OH Emissions in Asteroids. The very first proposal, A Hubble Space Telescope Study of Post Eclipse Brightening and Albedo Changes on Io, was published in Icarus,
[110] a journal devoted to solar system studies. After that time, however, budget reductions at STScI made the support of work by amateur astronomers untenable, and no further amateur programs have been carried out.
[111]20th birthday
The Hubble Telescope celebrated its 20th birthday on April 22, 2010. To consummate the celebration, NASA, ESA, and Space Telescope Institute (STScI) released an image from the
Carina Nebula.
[112]Hubble data
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. Approximately twice daily, the Hubble Space Telescope radios data to a satellite in the
geosynchronous Tracking and Data Relay Satellite System (TDRSS).
[113] The TDRSS 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.
[113] From there they are sent to the Goddard Space Flight Center and finally to the Space Telescope Science Institute for archiving.
[114]These data are then transmitted to the
Space Telescope Operations Control Center (STOCC) located in
Greenbelt, Maryland.
[113]Archives
All Hubble data is eventually made available via the
archives at STScI,
[115] CADC
[116] and
ESO.
[117] Data is usually proprietary—available only to the
principal investigator (PI) and astronomers designated by the PI—for one year after being taken. The PI can apply to the director of the STScI to extend or reduce the proprietary period in some circumstances.
[118]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.
[119] The
Hubble Heritage Project processes and releases to the public a small selection of the most striking images in
JPEG and
TIFF formats.
[120]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 are 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.
[121]Data analysis
Data analysis of a spectrum reveals the chemistry of hidden clouds
Hubble data can be analysed using many different packages. STScI maintains the custom-made STSDAS (Space Telescope Science Data Analysis System) 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.
[122]Outreach activities
The "Twenty Years at the Frontier of Science" exhibition at the Istituto Veneto di Scienze.
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.
[123] 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. The
Hubble Heritage Project was established to produce high-quality images for public consumption 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.
[124]In addition, STScI maintains several comprehensive websites for the general public containing Hubble images and information about the observatory.
[125][126][127][128] The outreach efforts are coordinated by the Office for Public Outreach, which was established in 2000 to ensure that US taxpayers saw the benefits of their investment in the space telescope program.
Since 1999, the leading Hubble outreach activities group in Europe has been the
Hubble European Space Agency Information Centre (HEIC).
[129] This office was established at the
Space Telescope - European Coordinating Facility (ST-ECF) in Munich, Germany. HEIC's mission statement is to fulfill the Hubble Space Telescope outreach and education tasks for the
European Space Agency (ESA). The work is centered on the production of news and photo releases that highlight interesting Hubble science results and images. These are often European in origin, and so not only increase the awareness of ESA’s Hubble share (15%), but the contribution of European scientists to the observatory. The group also produces video releases and other innovative educational material.
The Hubble Space Telescope has won two Space Achievement Awards from the
Space Foundation for its outreach activities, in 2001 and 2010.
[130]There is a replica of the Hubble Telescope on the courthouse lawn in
Marshfield, Missouri, the hometown of namesake Edwin P. Hubble.
Hubblecast
The
Hubblecast is a vodcast series made by the ESA's Hubble team to bring world-class science news to everyone about Hubble's latest discoveries. Hosted by "Dr. J"
(Joe Liske) who is a research scientist at
ESO. The episodes are available in several formats and resolutions for different platforms.
Future
Equipment failure
Past servicing missions have exchanged old instruments for new ones, both avoiding failure and making possible new types of science. 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.
[131] This power supply was fixed during servicing mission 4 in May 2009. Similarly, the main camera (the
ACS) primary electronics failed in June 2006, and the power supply for the backup electronics failed on January 27, 2007.
[132] 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.
[133] As of late May 2009, tests of both repaired instruments are still ongoing.
HST uses
gyroscopes to stabilize itself in orbit and point accurately and steadily at astronomical targets. Normally, three gyroscopes are required for operation; observations are still possible with two, but the area of sky that can be viewed would be somewhat restricted, and observations requiring very accurate pointing are more difficult.
[134] There are further contingency plans for science with just one gyro,
[135] but if all gyros fail, continued scientific observations will not be possible. 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.
[136] One more gyro failed in 2007.
[137] By the time of the final repair mission, during which all six gyros were replaced (with two new pairs and one refurbished pair), only three gyros were still working. Engineers are confident that they have identified the root causes of the gyro failures, and the new models should be much more reliable.
[138]In addition to predicted gyroscope failure, Hubble eventually required a change of
nickel hydrogen batteries. A robotic servicing mission including this would be tricky, as it requires many operations, and a failure in any might result in irreparable damage to Hubble. Alternatively, the observatory was designed so that during shuttle servicing missions it would receive power from a connection to the space shuttle, and this capability could have been utilized by adding an external power source (an additional battery) rather than changing the internal ones.
[139] In the end, however, the batteries were simply replaced during service mission 4.
Orbital decay
Hubble orbits the Earth in the extremely tenuous upper
atmosphere, and over time its orbit
decays due to
drag. If it is not re-boosted by a shuttle or other means, it will re-enter the Earth's atmosphere sometime between 2019 and 2032, with the exact date depending on how active the Sun is and its impact on the upper atmosphere. The state of Hubble's gyros also affects the re-entry date, as a controllable telescope can be oriented to minimize atmospheric drag. Not all of the telescope would burn up on re-entry. Parts of the main mirror and its support structure would probably survive, leaving the potential for damage or even human fatalities (estimated at up to a 1 in 700 chance of human fatality for a completely uncontrolled re-entry).
[140] With the success of
STS-125, the natural re-entry date range has been extended further as the mission replaced its gyroscopes, even though Hubble was not re-boosted to a higher orbit.
NASA's original plan for safely de-orbiting Hubble was to
retrieve it using a space shuttle. The Hubble telescope would then have most likely been displayed in the
Smithsonian Institution. This is no longer considered practical because of the costs of a shuttle flight, the mandate to retire the space shuttles by 2010, and the risk to a shuttle's crew. Instead NASA looked at adding an external propulsion module to allow controlled re-entry.
[141] The final decision was not to attach a de-orbit module on
STS-125, but to add a grapple fixture so a robotic mission could more easily attach such a module later.
[142]Debate over final servicing mission
Columbia was originally scheduled to visit Hubble again in February 2005. The tasks of this servicing mission would have included replacing a fine guidance sensor and two broken gyroscopes, placing protective "blankets" on top of torn insulation, replacing the
Wide Field and Planetary Camera 2 with a new
Wide Field Camera 3 and installing the
Cosmic Origins Spectrograph (COS). However, then-NASA Administrator
Sean O'Keefe decided that, in order to prevent a repeat of the
Columbia accident, all future shuttles must be able to reach the 'safe-haven' of the
International Space Station (ISS) should an in-flight problem develop that would preclude the shuttle from landing safely. The shuttle is incapable of reaching both the Hubble Space Telescope and the International Space Station during the same mission, and so future manned service missions were canceled.
[143]This decision was assailed by numerous astronomers, who felt that Hubble was valuable enough to merit the human risk. HST's successor, the
James Webb Space Telescope (JWST), will not be ready until well after the 2010 scheduled retirement of the space shuttle. While Hubble can image in the
ultraviolet and
visible wavelengths, JWST is limited to the
infrared. The break in space-observing capabilities between the decommissioning of Hubble and the commissioning of a successor is of major concern to many astronomers, given the great scientific impact of HST taken as a whole.
[144] The consideration that the JWST will not be located in
low Earth orbit, and therefore cannot be easily repaired in the event of an early failure, only makes these concerns more acute. Nor can JWST's instruments be easily upgraded. On the other hand, many astronomers felt strongly that the servicing of Hubble should
not take place if the costs of the servicing come from the JWST budget.
In January 2004, O'Keefe said he would review his decision to cancel the final shuttle servicing mission to HST due to public outcry and requests from Congress for NASA to look for a way to save it. On 13 July 2004 an official panel from the
National Academy of Sciences made the recommendation 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". In August 2004, O'Keefe requested the 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".
[145] In late 2004, several Congressional members, led by Sen. Barbara Mikulski (D-MD), held public hearings and carried on a fight with much public support (including thousands of letters from school children across the country) to get the Bush Administration and NASA to reconsider the decision to drop plans for a Hubble rescue mission.
[146]The arrival in April 2005 of the new NASA Administrator,
Michael D. Griffin, changed the status of the proposed shuttle rescue mission. At the time, Griffin stated he would reconsider the possibility of a manned servicing mission. Soon after his appointment, he authorized Goddard Space Flight Center to proceed with preparations for a manned Hubble maintenance flight, saying he would make the final decision on this flight after the next two shuttle missions. In October 2006 Griffin gave the final go-ahead for the mission. The 11-day
STS-125 mission by
Atlantis was scheduled for launch in October 2008.
[147][148] However, the main data-handling unit failed in late September 2008, halting all reporting of scientific data. This unit has a backup, and on October 25, 2008 Hubble was successfully rebooted and was reported to be functioning normally.
[149] However, since a failure in the backup unit would now leave the HST helpless, the service mission was postponed to allow astronauts to repair this problem. This mission got underway on May 11, 2009
[150] and completed all the long planned replacements as well as additional repairs, including replacing the main data-handling unit.
Planned successors
Several space telescopes are claimed to be successors to Hubble, and some ground based astronomy lays claim to higher optical achievements. None of the near-term space-based telescopes will duplicate Hubble's wavelength coverage (near ultra-violet to near infrared wavelength), instead concentrating on the farther
infrared bands. These bands are preferred for studying high Z and low temperature objects, but cannot be studied from the ground, and cannot be retrofitted to the Hubble since it lacks the requisite cooled optics. None of the space-based successors are designed to be serviced on orbit. In contrast, ground based astronomy includes roughly the same wavelengths as Hubble, is catching up in terms of resolution (via adaptive optics), has much larger light gathering power, and is easily upgraded. However, it cannot yet match the Hubble's excellent resolution over a wide field of view, and the very dark background of space.
JWST plans to detect stars in the
early Universe approximately 280 million years older than stars HST now detects.
The
James Webb Space Telescope (JWST) is a planned
infrared space observatory, and lays claim to being a planned successor of Hubble.
[151] The main scientific goal is to observe the most distant objects in the universe, beyond the reach of existing instruments. JWST will be able to detect stars in the
early Universe approximately 280 million years older than stars HST now detects.
[152][153]JWST is a NASA-led international collaboration between
NASA, the
European Space Agency and the
Canadian Space Agency. Formerly called the Next Generation Space Telescope (NGST), it was renamed after NASA's second administrator,
James E. Webb, in 2002. The telescope's launch is planned for no earlier than June 2014. It will be launched on an
Ariane 5 rocket.
[154]Another similar effort is the European Space Agency's
Herschel Space Observatory, launched on May 14, 2009. Like JWST, Herschel has a mirror substantially larger than Hubble's, but observes only in the
far-infrared.
Much further out is the
Advanced Technology Large-Aperture Space Telescope (AT-LAST)
[155] is a proposed 8 to 16-meter (320 to 640-inch) optical space
telescope that if approved, built, and launched (using the planned
Ares V rocket slated for
Project Constellation flights to the
Moon), would be a true replacement and successor for the Hubble Space Telescope (HST); with the ability to observe and photograph astronomical objects in the
optical,
ultraviolet, and
Infrared wavelengths, but with substantially better resolution than Hubble.
| Selected space telescopes & instruments[156] |
| Name | Year | Wavelength | Aperture |
| GALEX | 2003 | 0.135-0.280 μm | 0.5 m |
| Spitzer | 2003 | 3-180 μm | 0.85 m |
| Hubble STIS | 1997 | 0.115-1.03 μm | 2.4 m |
| Hubble WFC3 | 2009 | 0.2-1.7 μm | 2.4 m |
| Herschel | 2009 | 60-672 μm | 3.5 m |
| JWST | Planned | 0.6-10 μm | 6.5 m |
Existing ground based telescopes, and various proposed
Extremely Large Telescopes, certainly exceed the HST in terms of sheer light gathering power, due to their much larger mirrors. In some cases, they may also 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 are super sharp across a 2½' (150") field. Furthermore, space telescopes can study the heavens 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 faint, low-contrast astronomical objects.
[157]
