IRAS

Last updated
Infrared Astronomical Satellite / Infrarood Astronomische Satelliet
IRAS in JPL simulator.jpg
Infrared Astronomical Satellite in space simulator at JPL
Mission typeInfrared space observatory
Operator
COSPAR ID 1983-004A OOjs UI icon edit-ltr-progressive.svg
SATCAT no. 13777
Website irsa.ipac.caltech.edu/Missions/iras.html
Mission durationFinal: 9 months, 26 days
Spacecraft properties
Manufacturer
Launch mass1,083 kg (2,388 lb)
Dimensions3.60 × 3.24 × 2.05 m (11.8 × 10.6 × 6.7 ft) [1]
Start of mission
Launch date25 January 1983, 21:17 (1983-01-25UTC21:17)  UTC [2]
Rocket Delta 3910
Launch site Vandenberg SLC-2W
Entered service9 February 1983 [3]
End of mission
DisposalDecommissioned
Deactivated21 November 1983 (1983-11-22) [2]
Orbital parameters
Reference system Geocentric
Regime Sun-synchronous
Semi-major axis 7,270.69 km (4,517.80 mi)
Eccentricity 0.001857
Perigee altitude 879.05 km (546.22 mi)
Apogee altitude 906.05 km (562.99 mi)
Inclination 98.95 deg
Period 102.8 min
Mean motion 14.00 rev/day
Epoch 19 November 2016, 04:15:30  UTC [4]
Main telescope
Type Ritchey–Chrétien [5]
Diameter57 cm (22 in) [5]
Focal length545 cm (215 in), f/9.56 [5]
Collecting area2,019 cm2 (312.9 sq in) [5]
WavelengthsLong-wavelength to far-infrared
 

The Infrared Astronomical Satellite (Dutch: Infrarood Astronomische Satelliet) (IRAS) was the first space telescope to perform a survey of the entire night sky at infrared wavelengths. [6] Launched on 25 January 1983, [2] its mission lasted ten months. [7] The telescope was a joint project of the United States (NASA), the Netherlands (NIVR), and the United Kingdom (SERC). Over 250,000 infrared sources were observed at 12, 25, 60, and 100 micrometer wavelengths. [7]

Contents

Support for the processing and analysis of data from IRAS was contributed from the Infrared Processing and Analysis Center at the California Institute of Technology. Currently, the Infrared Science Archive at IPAC holds the IRAS archive. [8] [9]

The success of IRAS led to interest in the 1985 Infrared Telescope (IRT) mission on the Space Shuttle, and the planned Shuttle Infrared Telescope Facility which eventually transformed into the Space Infrared Telescope Facility, SIRTF, which in turn was developed into the Spitzer Space Telescope, launched in 2003. [10] The success of early infrared space astronomy led to further missions, such as the Infrared Space Observatory (1990s) and the Hubble Space Telescope 's NICMOS instrument.

Mission

IRAS launch USAF-1369th audiovisual squadron-(MAC).jpg
Launch of IRAS in 1983
Comet IRAS-Araki-Alckock-1983.jpg
False color image of comet IRAS–Araki–Alcock by IRAS
IRAS all-sky infrared survey.jpg
Infrared all-sky survey by IRAS

IRAS was the first observatory to perform an all-sky survey at infrared wavelengths. It mapped 96% of the sky four times, at 12, 25, 60 and 100 micrometers, with resolutions ranging from 30 arcseconds at 12 micrometers to 2 arcminutes at 100 micrometers. It discovered about 350,000 sources, many of which are still awaiting identification. About 75,000 of those are believed to be starburst galaxies, still enduring their star-formation stage. Many other sources are normal stars with disks of dust around them, possibly the early stage of planetary system formation. New discoveries included a dust disk around Vega and the first images of the Milky Way 's core.

IRAS's life, like that of most infrared satellites that followed, was limited by its cooling system. To effectively work in the infrared domain, a telescope must be cooled to cryogenic temperatures. In IRAS's case, 73 kilograms (161 lb) of superfluid helium kept the telescope at a temperature of 2  K (−271  °C ; −456  °F ), keeping the satellite cool by evaporation. IRAS was the first use of superfluids in space. [11] The on-board supply of liquid helium was depleted after 10 months on 21 November 1983, causing the telescope temperature to rise, preventing further observations. The spacecraft continues to orbit the Earth.

IRAS was designed to catalog fixed sources, so it scanned the same region of sky several times. Jack Meadows led a team at Leicester University, including John K. Davies and Simon F. Green, which searched the rejected sources for moving objects. This led to the discovery of three asteroids, including 3200 Phaethon (an Apollo asteroid and the parent body of the Geminid meteor shower), six comets, and a huge dust trail associated with comet 10P/Tempel. The comets included 126P/IRAS, 161P/Hartley–IRAS, and comet IRAS–Araki–Alcock (C/1983 H1), which made a close approach to the Earth in 1983. Out of the six comets IRAS found, four were long period and two were short period comets. [7]

Discoveries

IRAS made its observations from Earth orbit in 1983 IRAS in orbit.jpg
IRAS made its observations from Earth orbit in 1983

Overall, over a quarter million discrete targets were observed during its operations, both inside and beyond the Solar System. [7] In addition, new objects were discovered including asteroids and comets. [7] The observatory made headlines briefly with the announcement on 10 December 1983 of the discovery of an "unknown object" at first described as "possibly as large as the giant planet Jupiter and possibly so close to Earth that it would be part of this solar system". [12] [13] Further analysis revealed that, of several unidentified objects, nine were distant galaxies and the tenth was "intergalactic cirrus". [14] None were found to be Solar System bodies. [14] [15]

During its mission, IRAS (and later the Spitzer Space Telescope) detected odd infrared signatures around several stars. This led to the systems being targeted by the Hubble Space Telescope's NICMOS instrument between 1999 and 2006, but nothing was detected. In 2014, using new image processing techniques on the Hubble data, researchers discovered planetary disks around these stars. [16]

IRAS discovered six comets, out of total of 22 discoveries and recoveries of all comets that year. [7] [17] This was a lot for this period, before the launch of SOHO in 1995, which would allow the discovery of many more comets in the next decade (it would detect 1000 comets in ten years). [18]

Asteroid discoveries

Minor planets discovered: 4 [19]
3200 Phaethon 11 October 1983 list
3728 IRAS 23 August 1983 list
(10714) 1983 QG31 August 1983 list
(100004) 1983 VA1 November 1983 list

Later surveys

Several infrared space telescopes have continued and greatly expanded the study of the infrared Universe, such as the Infrared Space Observatory launched in 1995, the Spitzer Space Telescope launched in 2003, and the Akari Space Telescope launched in 2006.

A next generation of infrared space telescopes began when NASA's Wide-field Infrared Survey Explorer launched on 14 December 2009 aboard a Delta II rocket from Vandenberg Air Force Base. Known as WISE, the telescope provided results hundreds of times more sensitive than IRAS at the shorter wavelengths; it also had an extended mission dubbed NEOWISE beginning in October 2010 after its coolant supply ran out.

A planned mission is NASA's Near-Earth Object Surveillance Mission (NEOSM), which is a successor to the NEOWISE mission.

2020 near-miss

On 29 January 2020, 23:39:35 UTC, [20] IRAS was expected to pass as closely as 12 meters [21] from the U.S. Air Force's Gravity Gradient Stabilization Experiment (GGSE-4) of 1967, another un-deorbited satellite left aloft; the 14.7-kilometer per second pass [22] had an estimated risk of collision of 5%. Further complications arose from the fact that GGSE-4 was outfitted with an 18 meter long stabilization boom that was in an unknown orientation and may have struck the satellite even if the spacecraft's main body did not. [23] Initial observations from amateur astronomers seemed to indicate that both satellites had survived the pass, with the California-based debris tracking organization LeoLabs later confirming that they had detected no new tracked debris following the incident. [24] [25]

See also

Related Research Articles

<span class="mw-page-title-main">Asteroid</span> Minor planets found within the inner Solar System

An asteroid is a minor planet—an object that is neither a true planet nor a comet—that orbits within the inner Solar System. They are rocky, metallic or icy bodies with no atmosphere. Sizes and shapes of asteroids vary significantly, ranging from 1-meter rocks to a dwarf planet almost 1000 km in diameter.

<span class="mw-page-title-main">Space telescope</span> Instrument in space to study astronomical objects

A space telescope or space observatory is a telescope in outer space used to observe astronomical objects. Suggested by Lyman Spitzer in 1946, the first operational telescopes were the American Orbiting Astronomical Observatory, OAO-2 launched in 1968, and the Soviet Orion 1 ultraviolet telescope aboard space station Salyut 1 in 1971. Space telescopes avoid the filtering and distortion (scintillation) of electromagnetic radiation which they observe, and avoid light pollution which ground-based observatories encounter. They are divided into two types: Satellites which map the entire sky, and satellites which focus on selected astronomical objects or parts of the sky and beyond. Space telescopes are distinct from Earth imaging satellites, which point toward Earth for satellite imaging, applied for weather analysis, espionage, and other types of information gathering.

Infrared astronomy is a sub-discipline of astronomy which specializes in the observation and analysis of astronomical objects using infrared (IR) radiation. The wavelength of infrared light ranges from 0.75 to 300 micrometers, and falls in between visible radiation, which ranges from 380 to 750 nanometers, and submillimeter waves.

<span class="mw-page-title-main">Far-infrared astronomy</span> Scientific study of celestial objects visible in wavelengths of 30-450 μm

Far-infrared astronomy is the branch of astronomy and astrophysics that deals with objects visible in far-infrared radiation.

<span class="mw-page-title-main">Spitzer Space Telescope</span> Infrared space telescope - 2003 to Jan 2020

The Spitzer Space Telescope, formerly the Space Infrared Telescope Facility (SIRTF), was an infrared space telescope launched in 2003. Operations ended on 30 January 2020. Spitzer was the third space telescope dedicated to infrared astronomy, following IRAS (1983) and ISO (1995–1998). It was the first spacecraft to use an Earth-trailing orbit, later used by the Kepler planet-finder.

<span class="mw-page-title-main">Infrared Space Observatory</span>

The Infrared Space Observatory (ISO) was a space telescope for infrared light designed and operated by the European Space Agency (ESA), in cooperation with ISAS and NASA. The ISO was designed to study infrared light at wavelengths of 2.5 to 240 micrometres and operated from 1995 to 1998.

<span class="mw-page-title-main">Great Observatories program</span> Series of NASA satellites

NASA's series of Great Observatories satellites are four large, powerful space-based astronomical telescopes launched between 1990 and 2003. They were built with different technology to examine specific wavelength/energy regions of the electromagnetic spectrum: gamma rays, X-rays, visible and ultraviolet light, and infrared light.

<span class="mw-page-title-main">Marc Buie</span> American astronomer

Marc William Buie is an American astronomer and prolific discoverer of minor planets who works at the Southwest Research Institute in Boulder, Colorado in the Space Science Department. Formerly he worked at the Lowell Observatory in Flagstaff, Arizona, and was the Sentinel Space Telescope Mission Scientist for the B612 Foundation, which is dedicated to protecting Earth from asteroid impact events.

<span class="mw-page-title-main">Near Infrared Camera and Multi-Object Spectrometer</span>

The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) is a scientific instrument for infrared astronomy, installed on the Hubble Space Telescope (HST), operating from 1997 to 1999, and from 2002 to 2008. Images produced by NICMOS contain data from the near-infrared part of the light spectrum.

<span class="mw-page-title-main">Infrared Processing and Analysis Center</span> NASA science center at Caltech in the US

The Infrared Processing and Analysis Center (IPAC) provides science operations, data management, data archives and community support for astronomy and planetary science missions. IPAC has a historical emphasis on infrared-submillimeter astronomy and exoplanet science. IPAC has supported NASA, NSF and privately funded projects and missions. It is located on the campus of the California Institute of Technology in Pasadena, California.

Luminous infrared galaxies or LIRGs are galaxies with luminosities, the measurement of brightness, above 1011 L. They are also referred to as submillimeter galaxies (SMGs) through their normal method of detection. LIRGs are more abundant than starburst galaxies, Seyfert galaxies and quasi-stellar objects at comparable luminosity. Infrared galaxies emit more energy in the infrared than at all other wavelengths combined. A LIRG's luminosity is 100 billion times that of the Sun.

<span class="mw-page-title-main">Wide-field Infrared Survey Explorer</span> NASA satellite of the Explorer program

Wide-field Infrared Survey Explorer is a NASA infrared astronomy space telescope in the Explorers Program. It was launched in December 2009, and placed in hibernation mode in February 2011, before being re-activated in 2013 and renamed the Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE). WISE discovered thousands of minor planets and numerous star clusters. Its observations also supported the discovery of the first Y-type brown dwarf and Earth trojan asteroid.

Frank James Low was a solid state physicist who became a leader in the new field of infrared astronomy, after inventing the gallium doped germanium bolometer in 1961. This detector extended the range of the observable spectrum to much longer wavelengths.

<span class="mw-page-title-main">Infrared telescope</span> Telescope that uses infrared light

An infrared telescope is a telescope that uses infrared light to detect celestial bodies. Infrared light is one of several types of radiation present in the electromagnetic spectrum.

<span class="mw-page-title-main">Wide Field Camera 3</span> Astronomical camera on the Hubble Space Telescope

The Wide Field Camera 3 (WFC3) is the Hubble Space Telescope's last and most technologically advanced instrument to take images in the visible spectrum. It was installed as a replacement for the Wide Field and Planetary Camera 2 during the first spacewalk of Space Shuttle mission STS-125 on May 14, 2009.

<span class="mw-page-title-main">3548 Eurybates</span> Asteroid satellite

3548 Eurybates is a carbonaceous Jupiter trojan from the Greek camp and the parent body of the Eurybates family, approximately 68 kilometers in diameter. It is a target to be visited by the Lucy mission in August 2027. Discovered during the second Palomar–Leiden Trojan survey in 1973, it was later named after Eurybates from Greek mythology. This C-type asteroid is among the 60 largest known Jupiter trojans and has a rotation period of 8.7 hours. Eurybates has one kilometer-sized satellite, named Queta, that was discovered in images taken by the Hubble Space Telescope in September 2018.

2906 Caltech, provisional designation 1983 AE2, is an asteroid from the outer region of the asteroid belt, approximately 56 kilometers in diameter. It was discovered on 13 January 1983 by American astronomer Carolyn Shoemaker at Palomar Observatory in the United States. It is named after the California Institute of Technology.

<span class="mw-page-title-main">NEO Surveyor</span> Space-based infrared telescope

NEO Surveyor, formerly called Near-Earth Object Camera (NEOCam), then NEO Surveillance Mission, is a planned space-based infrared telescope designed to survey the Solar System for potentially hazardous asteroids.

<span class="mw-page-title-main">Fred Gillett (astronomer)</span> American astronomer (1937–2001)

Frederick Carl Gillett was an American astronomer who was a pioneer of infrared astronomy. He was based successively at the University of California, San Diego, Kitt Peak National Observatory, and the International Gemini Observatory. His discoveries include the Vega phenomenon and the first unidentified infrared emission bands.

References

  1. Beichman 1988, p. II-1.
  2. 1 2 3 "Infrared Astronomical Satellite". NASA . Retrieved 19 November 2016.
  3. Neugebauer, G.; Habing, H. J.; van Duinen, R.; Aumann, H. H.; Baud, B.; et al. (March 1984). "The Infrared Astronomical Satellite (IRAS) mission" (PDF). Astrophysical Journal. 278: L1–L6. Bibcode:1984ApJ...278L...1N. doi:10.1086/184209. hdl: 1887/6453 .
  4. "IRAS - Orbit". Heavens-Above . 19 November 2016. Retrieved 19 November 2016.
  5. 1 2 3 4 Beichman 1988, p. II-8.
  6. Beichman 1988, p. I-1.
  7. 1 2 3 4 5 6 Schmadel, Lutz D. (2007). "(3728) Iras". Dictionary of Minor Planet Names . Springer Berlin Heidelberg. p.  315. doi:10.1007/978-3-540-29925-7_3725. ISBN   978-3-540-00238-3.
  8. "Infrared Astronomical Satellite". Infrared Processing and Analysis Center. Caltech. Archived from the original on 6 June 2016. Retrieved 19 November 2016.
  9. "Infrared Astronomical Satellite (IRAS)". NASA/IPAC Infrared Science Archive. Caltech. Retrieved 19 November 2016.
  10. "Early History". Spitzer Space Telescope. NASA. Archived from the original on 2 August 2020. Retrieved 30 November 2016.
  11. Rowan-Robinson, Michael (1993). Ripples in the Cosmos. W. H. Freeman and Company. p. 75. ISBN   0-7167-4503-8.
  12. O'Toole, Thomas (30 December 1983). "Mystery Heavenly Body Discovered". The Washington Post . p. A1. Archived from the original on 1 February 2010.
  13. "Mystery heavenly body found close to Earth". The Gazette . Washington Post. 30 December 1983. p. A-1. Retrieved 16 October 2012.
  14. 1 2 Chester, Thomas J. (5 May 1998). "No Tenth Planet Yet From IRAS". Caltech. Archived from the original on 2 February 2010.
  15. Plait, Phil (17 November 2010). "The Planet X Saga: Science". Bad Astronomy. Retrieved 5 March 2011.
  16. Harrington, J. D.; Villard, Ray (24 April 2014). "Astronomical Forensics Uncover Planetary Disks in NASA's Hubble Archive". NASA. NASA Release 14-114. Retrieved 30 November 2016.
  17. Marsden, B. G. (1986). "1986QJRAS..27..102M Page 102". Quarterly Journal of the Royal Astronomical Society. 27: 102. Bibcode:1986QJRAS..27..102M . Retrieved 2019-09-30.
  18. "NASA - History's Greatest Comet Hunter Discovers 1,000th Comet". www.nasa.gov. Retrieved 2019-09-30.
  19. "Minor Planet Discoverers". Minor Planet Center. 4 September 2016. Retrieved 11 November 2016.
  20. @LeoLabs_Space (29 January 2020). "Our latest data on the IRAS / GGSE 4 event" (Tweet) via Twitter.
  21. @LeoLabs_Space (29 January 2020). "Our latest update this morning for IRAS / GGSE 4" (Tweet) via Twitter.
  22. "2 satellites will narrowly avoid colliding at 32,800 MPH over Pittsburgh on Wednesday". Space.com . 28 January 2020.
  23. @LeoLabs_Space (29 January 2020). "Adjusted calculations for larger object size" (Tweet) via Twitter.
  24. @juliancd38 (29 January 2020). "Trails of both IRAS and GGSE4 continue unimpeded after intersection" (Tweet) via Twitter.
  25. @LeoLabs_Space (29 January 2020). "Latest data following the event shows no evidence of new debris" (Tweet) via Twitter.

Bibliography