Astron (spacecraft)

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Astron
Astron.gif
Diagram of the Astron observatory
Mission type Astrophysics
OperatorSoviet space program
CNES
COSPAR ID 1983-020A OOjs UI icon edit-ltr-progressive.svg
SATCAT no. 13901
Mission duration8 years
Spacecraft properties
Bus 4MV [1]
Manufacturer NPO Lavochkin
Launch mass3,250 kg (7,170 lb) [2]
Start of mission
Launch date23 March 1983 12:45 (1983-03-23UTC12:45) UTC
Rocket Proton-K/D-1
Launch site Baikonur 200/39
End of mission
DisposalDecommissioned
Deactivated23 March 1991
Orbital parameters
Reference system High Earth
Semi-major axis 108,531 km (67,438 mi) [3]
Eccentricity 0.6575927 [4]
Perigee altitude 30,791 km (19,133 mi) [3]
Apogee altitude 173,530.2 km (107,826.7 mi) [3]
Inclination 48.4° [3]
Period 5,930.5 minutes [3]
Mean motion 0.24281115 rev/day [4]
Epoch 19 July 2017 07:25:15 UTC
Main telescope
Collecting area0.17 m2 (1.8 sq ft) [1]
Wavelengths X-ray: 2–25  keV [1]
Ultraviolet: 150–350 nm

Astron was a Soviet space telescope launched on 23 March 1983 at 12:45:06 UTC, using the Proton-K rocket. [5] Based on the 4MV spacecraft design and operational for six years, Astron was the largest ultraviolet space telescope of its time.

The project was headed by Alexandr Boyarchuk. [6] [7] [8] The spacecraft was designed and constructed by the Crimean Astrophysical Observatory and NPO Lavochkin. A group of scientists from these institutions was awarded the USSR State Prize for their work. [9]

The payload consisted of an 80 cm ultraviolet telescope, which was jointly designed by the USSR and France, and an X-ray spectroscope. [10] It could take UV spectra 150-350 nm. [11]

Placed into an orbit with an apogee of 185,000 kilometres (115,000 mi), Astron was capable of making observations outside the Earth's umbra and radiation belt.

Among the most important observations made by Astron were those of SN 1987A supernova from March 4 to March 12, 1987, [12] and of Halley's Comet in December 1985, the latter of which enabled a group of Soviet scientists to develop a model of the comet's coma. [11]

Operation of the observatory ended on 23 March 1991. [13]

See also

Related Research Articles

<span class="mw-page-title-main">Comet</span> Natural object in space that releases gas

A comet is an icy, small Solar System body that warms and begins to release gases when passing close to the Sun, a process called outgassing. This produces an extended, gravitationally unbound atmosphere or coma surrounding the nucleus, and sometimes a tail of gas and dust gas blown out from the coma. These phenomena are due to the effects of solar radiation and the outstreaming solar wind plasma acting upon the nucleus of the comet. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust, and small rocky particles. The coma may be up to 15 times Earth's diameter, while the tail may stretch beyond one astronomical unit. If sufficiently close and bright, a comet may be seen from Earth without the aid of a telescope and can subtend an arc of up to 30° across the sky. Comets have been observed and recorded since ancient times by many cultures and religions.

<span class="mw-page-title-main">SN 1987A</span> 1987 supernova event in the constellation Dorado

SN 1987A was a type II supernova in the Large Magellanic Cloud, a dwarf satellite galaxy of the Milky Way. It occurred approximately 51.4 kiloparsecs from Earth and was the closest observed supernova since Kepler's Supernova in 1604. Light and neutrinos from the explosion reached Earth on February 23, 1987 and was designated "SN 1987A" as the first supernova discovered that year. Its brightness peaked in May of that year, with an apparent magnitude of about 3.

<span class="mw-page-title-main">Halley's Comet</span> Short-period comet visible every 75–77 years

Halley's Comet is the only known short-period comet that is consistently visible to the naked eye from Earth, appearing every 72–80 years. It last appeared in the inner parts of the Solar System in 1986 and will next appear in mid-2061. Officially designated 1P/Halley, it is also commonly called Comet Halley, or sometimes simply Halley.

<span class="mw-page-title-main">Solar and Heliospheric Observatory</span> European space observatory

The Solar and Heliospheric Observatory (SOHO) is a European Space Agency (ESA) spacecraft built by a European industrial consortium led by Matra Marconi Space that was launched on a Lockheed Martin Atlas IIAS launch vehicle on 2 December 1995, to study the Sun. It has also discovered over 5,000 comets. It began normal operations in May 1996. It is a joint project between the European Space Agency (ESA) and NASA. SOHO was part of the International Solar Terrestrial Physics Program (ISTP). Originally planned as a two-year mission, SOHO continues to operate after almost 29 years in space; the mission has been extended until the end of 2025, subject to review and confirmation by ESA's Science Programme Committee.

<span class="mw-page-title-main">Rashid Sunyaev</span> Russian astronomer (born 1943)

Rashid Alievich Sunyaev is a German, Soviet, and Russian astrophysicist of Tatar descent. He got his MS degree from the Moscow Institute of Physics and Technology (MIPT) in 1966. He became a professor at MIPT in 1974. Sunyaev was the head of the High Energy Astrophysics Department of the Russian Academy of Sciences, and has been chief scientist of the Academy's Space Research Institute since 1992. He has also been a director of the Max Planck Institute for Astrophysics in Garching, Germany since 1996, and Maureen and John Hendricks Distinguished Visiting Professor in the School of Natural Sciences at the Institute for Advanced Study in Princeton since 2010. In February 2022, he signed an open letter from Russian scientists and science journalists condemning Russia's invasion of Ukraine.

<span class="mw-page-title-main">Coma (comet)</span> Cloud of gas or a trail around a comet or asteroid

The coma is the nebulous envelope around the nucleus of a comet, formed when the comet passes near the Sun in its highly elliptical orbit. As the comet warms, parts of it sublimate; this gives a comet a diffuse appearance when viewed through telescopes and distinguishes it from stars. The word coma comes from the Greek κόμη (kómē), which means "hair" and is the origin of the word comet itself.

<span class="mw-page-title-main">Orbiting Astronomical Observatory</span> Series of American space observatories

The Orbiting Astronomical Observatory (OAO) satellites were a series of four American space observatories launched by NASA between 1966 and 1972, managed by NASA Chief of Astronomy Nancy Grace Roman. These observatories, including the first successful space telescope, provided the first high-quality observations of many objects in ultraviolet light. Although two OAO missions were failures, the success of the other two increased awareness within the astronomical community of the benefits of space-based observations, and led to the instigation of the Hubble Space Telescope.

<span class="mw-page-title-main">International Ultraviolet Explorer</span> Astronomical observatory satellite

International Ultraviolet Explorer, was the first space observatory primarily designed to take ultraviolet (UV) electromagnetic spectrum. The satellite was a collaborative project between NASA, the United Kingdom's Science and Engineering Research Council and the European Space Agency (ESA), formerly European Space Research Organisation (ESRO). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on 26 January 1978, 17:36:00 UTC aboard a NASA Thor-Delta 2914 launch vehicle. The mission lifetime was initially set for 3 years, but in the end, it lasted 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.

Comet dust refers to cosmic dust that originates from a comet. Comet dust can provide clues to comets' origin. When the Earth passes through a comet dust trail, it can produce a meteor shower.

<span class="mw-page-title-main">Comet nucleus</span> Central part of a comet

The nucleus is the solid, central part of a comet, formerly termed a dirty snowball or an icy dirtball. A cometary nucleus is composed of rock, dust, and frozen gases. When heated by the Sun, the gases sublime and produce an atmosphere surrounding the nucleus known as the coma. The force exerted on the coma by the Sun's radiation pressure and solar wind cause an enormous tail to form, which points away from the Sun. A typical comet nucleus has an albedo of 0.04. This is blacker than coal, and may be caused by a covering of dust.

<span class="mw-page-title-main">Comet Bennett</span> Icy small Solar System body; passed closest to Earth in 1970

Comet Bennett, formally known as C/1969 Y1, was one of the two bright comets observed in the 1970s, along with Comet West and is considered a great comet. The name is also borne by an altogether different comet, C/1974 V2. Discovered by John Caister Bennett on December 28, 1969, while still almost two AUs from the Sun, it reached perihelion on March 20, passing closest to Earth on March 26, 1970, as it receded, peaking at magnitude 0. It was last observed on February 27, 1971.

<span class="mw-page-title-main">Granat</span> Soviet/Russian space telescope (1989–1998)

The International Astrophysical Observatory "GRANAT", was a Soviet space observatory developed in collaboration with France, Denmark and Bulgaria. It was launched on 1 December 1989 aboard a Proton rocket and placed in a highly eccentric four-day orbit, of which three were devoted to observations. It operated for almost nine years.

<span class="mw-page-title-main">Spektr-R</span> Russian satellite

Spektr-R was a Russian scientific satellite with a 10 m (33 ft) radio telescope on board. It was launched on 18 July 2011 on a Zenit-3F launcher from Baikonur Cosmodrome, and was designed to perform research on the structure and dynamics of radio sources within and beyond the Milky Way. Together with some of the largest ground-based radio telescopes, the Spektr-R formed interferometric baselines extending up to 350,000 km (220,000 mi).

<span class="mw-page-title-main">Gamma-ray astronomy</span> Observational astronomy performed with gamma rays

Gamma-ray astronomy is a subfield of astronomy where scientists observe and study celestial objects and phenomena in outer space which emit cosmic electromagnetic radiation in the form of gamma rays, i.e. photons with the highest energies at the very shortest wavelengths. Radiation below 100 keV is classified as X-rays and is the subject of X-ray astronomy.

<span class="mw-page-title-main">Comet tail</span> Dust or gases blown off a comet by solar wind in the inner solar system, leaving a visible trail

A comet tail and coma are visible features of a comet when they are illuminated by the Sun and may become visible from Earth when a comet passes through the inner Solar System. As a comet approaches the inner Solar System, solar radiation causes the volatile materials within the comet to vaporize and stream out of the nucleus, carrying dust away with them.

<span class="mw-page-title-main">Orbiting Astronomical Observatory 2</span> Space telescope launched on December 7, 1968

The Orbiting Astronomical Observatory 2 was the first successful space telescope, launched on December 7, 1968. An Atlas-Centaur rocket launched it into a nearly circular 750-kilometre (470 mi) altitude Earth orbit. Data was collected in ultraviolet on many sources including comets, planets, and galaxies. It had two major instrument sets facing in opposite directions; the Smithsonian Astrophysical Observatory (SAO) and the Wisconsin Experiment Package (WEP). One discovery was large halos of hydrogen gas around comets, and it also observed Nova Serpentis, which was a nova discovered in 1970.

Alexandr Boyarchuk was a Russian physicist and astronomer.

References

  1. 1 2 3 Gunter D. Krebs. "Astron 1". Gunter's Space Page. Retrieved 25 October 2024.
  2. Mark Wade. "Astron". Encyclopedia Astronautica. Retrieved 25 October 2024.
  3. 1 2 3 4 5 "ASTRON". N2YO.com. Retrieved 25 October 2024.
  4. 1 2 T. S. Kelso. "Astron (TLE)". CelesTrak.org. Retrieved 19 July 2017.
  5. Jonathan McDowell. "Launch Log". Jonathan's Space Page. Retrieved 23 August 2009.
  6. "Spektr-UF Project History" (in Russian). Archived from the original on 6 March 2005.
  7. "Alexander Boyarchuk" (in Russian). Archived from the original on 30 September 2007. Retrieved 23 August 2009.
  8. A. A. Boyarchuk (1994). Астрофизические исследdeaования на космической станции "Астрон"[Astrophysical research on the Astron space telescope] (in Russian). Moscow, Russia: Nauka.
  9. "Crimean Astrophysical Observatory" (in Russian). Archived from the original on 27 September 2007. Retrieved 23 August 2009.
  10. "The Astron Satellite". NASA / Goddard. 26 June 2003. Archived from the original on 26 August 2009. Retrieved 23 August 2009.
  11. 1 2 A. A. Boyarchuk; V. P. Grinin; A. M. Zvereva; P. P. Petrov; A. I. Sheikhet (1986). "A model for the coma of Comet Halley, based on the Astron ultraviolet spectrophotometry". Pis'ma v Astronomicheskii Zhurnal (in Russian). 12: 696–706. Bibcode:1986PAZh...12..696B.
  12. A. A. Boyarchuk; R. E. Gershberg; A. M. Zvereva; P. P. Petrov; A. B. Severnyj; et al. (1987). "Observations on Astron: Supernova 1987A in the Large Magellanic Cloud". Pis'ma v Astronomicheskii Zhurnal (in Russian). 13: 739–743. Bibcode:1987PAZh...13..739B.
  13. B. Harvey; O. Zakutnyaya (2011). Russian Space Probes: Scientific Discoveries and Future Missions. Springer Praxis. pp. 376–380. ISBN   978-1-441-98149-3.