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1992 Galvarino

From Wikipedia, the free encyclopedia
Main-belt asteroid

1992 Galvarino
Discovery[1]
Discovered byC. Torres
S. Cofré
Discovery siteCerro El Roble Stn.
Discovery date18 July 1968
Designations
(1992) Galvarino
Named after
Galvarino(Mapuche warrior)[2]
1968 OD
main-belt · Eos[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc48.69 yr (17,783 days)
Aphelion3.1367AU
Perihelion2.8468 AU
2.9917 AU
Eccentricity0.0485
5.17yr (1,890 days)
197.49°
0° 11m 25.8s / day
Inclination10.570°
182.59°
98.241°
Physical characteristics
Dimensions9.597±0.105 km[4][5]
10.24 km(calculated)[3]
7.004h[6]
0.14(assumed)[3]
0.145±0.018[4][5]
M[4] · L[7] · S[3]
12.7[1][3] · 12.8[4] · 12.91±0.22[7]

1992 Galvarino, provisional designation1968 OD, is an Eoanasteroid from the outer region of theasteroid belt, approximately 10 kilometers in diameter.

It was discovered on 18 July 1968, by Chilean astronomersCarlos Torres andS. Cofre at theCerro El Roble Station of Chile'sNational Astronomical Observatory, and named after the indigenous warriorGalvarino.[2][8]

Classification and orbit

[edit]

Galvarino is a stonyS-type asteroid and a member of theEos family, an orbital group of more than 4,000 asteroids, which are well known for mostly being of stony composition with a relatively highalbedo. It is also classified as aM- andL-type asteroids byWISE andPanSTARRS, respectively.[4][7]

It orbits the Sun in theouter main-belt at a distance of 2.8–3.1 AU once every 5 years and 2 months (1,890 days). Its orbit has aneccentricity of 0.05 and aninclination of 11° with respect to theecliptic.[1] Itsobservation arc begins with its official discovery observation in 1968, as noprecoveries and no previous identifications were made.[8]

Physical characteristics

[edit]

As of 2016, a single rotationallightcurve ofGalvarino has been obtained. The photometric observations were made in the 1990s, giving a well-definedrotation period of 7.004 hours with a brightness variation of 0.6magnitude (U=3).[6]

According to the surveys carried out by NASA's WISE satellite with its subsequentNEOWISE mission, the asteroid measures 9.6 kilometers in diameter and its surface has analbedo of 0.145,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.14 and calculates a diameter of 10.2 kilometers with anabsolute magnitude of 12.7.[3]

Naming

[edit]

Thisminor planet was named after the indigenous warriorGalvarino, the heroic figure during theArauco War, a long-running conflict between colonial Spaniards and theMapuche people of the 16th century in what is now Chile.

He was condemned by the Spanish soldiers to have his hands cut off and then to be freed as a living lesson to other Indians. Since his request for death was not granted, he promised revenge. He continued to fight the conquerors until recaptured and condemned to the gallows.[2] The approved naming citation was published by theMinor Planet Center on 1 June 1980 (M.P.C. 5358).[9]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1992 Galvarino (1968 OD)" (2017-03-26 last obs.).Jet Propulsion Laboratory. Retrieved1 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1992) Galvarino".Dictionary of Minor Planet Names – (1992) Galvarino.Springer Berlin Heidelberg. p. 161.doi:10.1007/978-3-540-29925-7_1993.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1992) Galvarino". Asteroid Lightcurve Database (LCDB). Retrieved8 December 2016.
  4. ^abcdefMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  5. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved8 December 2016.
  6. ^abBirlan, M.; Barucci, M. A.; Angeli, C. A.; Doressoundiram, A.; De Sanctis, M. C. (June 1996)."Rotational properties of asteroids: CCD observations of nine small asteroids".Planetary and Space Science.44 (6):555–558.Bibcode:1996P&SS...44..555B.doi:10.1016/0032-0633(96)00019-0. Retrieved8 December 2016.
  7. ^abcVeres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved8 December 2016.
  8. ^ab"1992 Galvarino (1968 OD)".Minor Planet Center. Retrieved8 December 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved8 December 2016.

External links

[edit]
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