Astronomy:4034 Vishnu
Discovery [1] | |
---|---|
Discovered by | E. F. Helin |
Discovery site | Palomar Obs. |
Discovery date | 2 August 1986 |
Designations | |
(4034) Vishnu | |
Named after | Vishnu (Hindu deity)[2] |
1986 PA | |
Minor planet category | Apollo · NEO · PHA [1][2] |
Orbital characteristics [1] | |
Epoch 6 January 2010 (JD 2455202.5) | |
Uncertainty parameter 0 | |
Observation arc | 28.93 yr (10,565 days) |
|{{{apsis}}}|helion}} | 1.5299 AU |
|{{{apsis}}}|helion}} | 0.5891 AU |
1.0595 AU | |
Eccentricity | 0.4439 |
Orbital period | 1.09 yr (398 days) |
Mean anomaly | 62.851° |
Mean motion | 0° 54m 13.32s / day |
Inclination | 11.170° |
Longitude of ascending node | 158.01° |
296.60° | |
Earth MOID | 0.0194 AU · 7.6 LD |
Physical characteristics | |
Mean diameter | 0.42 km[3] |
Geometric albedo | 0.52[3] |
SMASS = O [1] | |
Absolute magnitude (H) | 18.4[1] |
4034 Vishnu (prov. designation: 1986 PA) is a rare-type asteroid classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 420 meters (1,400 feet) in diameter. It was discovered on 2 August 1986, by American astronomer Eleanor Helin at Palomar Observatory in California, United States. It is named after the Hindu deity Vishnu.[2]
Naming
This minor planet was named for the four-armed god of protection and preservation of good, Vishnu, one of the principal deities of Hinduism. The asteroid's name was proposed by Belgian amateur astronomer and professional meteorologist Jean Meeus.[2][4] The approved naming citation was published by the Minor Planet Center on 15 July 2011 (M.P.C. 75547).[5]
Classification and orbit
Vishnu orbits the Sun at a distance of 0.6–1.5 AU once every 1 years and 1 month (398 days). Its orbit has an eccentricity of 0.44 and an inclination of 11° with respect to the ecliptic.[1] As no precoveries were taken, and no prior identifications were made, the body's observation arc begins with its official discovery observation at Palomar in 1986.[2]
Vishnu is a potentially hazardous asteroid due to its sufficiently large size and low Earth minimum orbital intersection distance of 0.0194 AU (2,900,000 km), which corresponds to 7.6 lunar distances.[1]
Its highly eccentric orbit crosses the orbits of all inner planets except that of Mercury, which effectively makes it a Venus-crosser, Earth-crosser and Mars-crosser all at once. From 1800 to 2200, Vishnu has made and will make multiple approaches of Venus (71×), Earth (29×), and Mars (7×) within 30 gigameters. It has been observed by radar astronomy (Binzel) and the orbital solution includes non-gravitational forces.[1]
Physical parameters
In the SMASS taxonomy, Vishnu is a rare O-type asteroid, meaning it is similar to the asteroid 3628 Boznemcová, which is the best asteroid match to the spectra of L6 and LL6 ordinary chondrite meteorites. These L and LL chondrites have lower iron metal content, but higher iron oxide content in the silicates.[1]
In the early 2000s, Vishnu has been observed in the thermal-infrared by the Keck telescope on Mauna Kea, Hawaii. The asteroid measures approximately 420 meters in diameter and its surface has a high albedo of 0.520.[3] As of 2017, Vishnu's rotation period and shape remain unknown as no lightcurves have yet been obtained.[6]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 "JPL Small-Body Database Browser: 4034 Vishnu (1986 PA)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2004034.
- ↑ 2.0 2.1 2.2 2.3 2.4 "4034 Vishnu (1986 PA)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=4034.
- ↑ 3.0 3.1 3.2 Delbó, Marco; Harris, Alan W.; Binzel, Richard P.; Pravec, Petr; Davies, John K. (November 2003). "Keck observations of near-Earth asteroids in the thermal infrared". Icarus 166 (1): 116–130. doi:10.1016/j.icarus.2003.07.002. Bibcode: 2003Icar..166..116D. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2003Icar..166..116D. Retrieved 14 March 2017.
- ↑ Schmadel, Lutz D. (2007). "(2213) Meeus". Dictionary of Minor Planet Names – (2213) Meeus. Springer Berlin Heidelberg. p. 180. doi:10.1007/978-3-540-29925-7_2214. ISBN 978-3-540-00238-3.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html.
- ↑ "LCDB Data for (4034) Vishnu". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=4034%7CVishnu.
External links
- Asteroid Lightcurve Database (LCDB), query form (info )
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- 4034 Vishnu at NeoDyS-2, Near Earth Objects—Dynamic Site
- Ephemeris · Obs prediction · Orbital info · MOID · Proper elements · Obs info · Close · Physical info · NEOCC
- 4034 Vishnu at ESA–space situational awareness
- 4034 Vishnu at the JPL Small-Body Database
Original source: https://en.wikipedia.org/wiki/4034 Vishnu.
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