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1929 Kollaa

From Wikipedia, the free encyclopedia
Planetoid

1929 Kollaa
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date20 January 1939
Designations
(1929) Kollaa
Named after
Kollaa River[2]
(river inKarelia)
1939 BS · 1939 CH
1943 GG · 1968 BH
1976 JF3
main-belt · Vestian[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc48.64 yr (17,766 days)
Aphelion2.5396AU
Perihelion2.1862 AU
2.3629 AU
Eccentricity0.0748
3.63yr (1,327 days)
226.60°
0° 16m 17.04s / day
Inclination7.7797°
65.429°
71.220°
Physical characteristics
Dimensions6.06 km(calculated)[3]
6.71±0.34 km[4]
7.772±0.147 km[5][6]
2.980±0.005 h[a]
2.9887±0.0004h[7]
0.3855±0.0958[5]
0.393±0.066[4][6]
0.4(assumed)[3]
SMASS = V[1] · V[3]
12.2[5] · 12.50[4] · 12.6[1] · 12.64±0.32[8] · 12.7[3]

1929 Kollaa, provisional designation1939 BS, is a stony Vestianasteroid from the inner regions of theasteroid belt, approximately 7 kilometers in diameter. It was discovered by Finnish astronomerYrjö Väisälä atTurku Observatory in Southwest Finland, on 20 January 1939.[9] The asteroid was named after theKollaa River in what is now Russia.[2]

Orbit and classification

[edit]

Kollaa is a member of theVesta family. Vestian asteroids have a composition akin to cumulateeucrite meteorites and are thought to have originated deep within4 Vesta's crust, possibly from theRheasilvia crater, a largeimpact crater on its southern hemisphere near the South pole, formed as a result of a subcatastrophic collision. The asteroid Vesta is the main-belt's second-most-massive body after1 Ceres.[10]

The asteroid orbits the Sun in theinner main-belt at a distance of 2.2–2.5 AU once every 3 years and 8 months (1,327 days). Its orbit has aneccentricity of 0.07 and aninclination of 8° with respect to theecliptic.[1] As noprecoveries were taken, the asteroid'sobservation arc begins with its discovery.[9]

Physical characteristics

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In theSMASS taxonomy,Kollaa is a brightV-type asteroid.[1]

Lightcurves

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It has a well-definedrotation period of 2.98 hours, derived from two rotationallightcurve analysis. In March 2004, photometric observations at the U.S.Magdalena Ridge Observatory in New Mexico rendered a period of 2.980 hours with a brightness variation of 0.20 inmagnitude (U=3).[a] In 2008 a second, concurring period was obtained by French amateur astronomerPierre Antonini at his privateObservatoire de Bédoin in France (132). It gave a period of 2.9887 hours and an amplitude 0.22 in magnitude (U=3).[7]

Diameter and albedo

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According to the surveys carried out by NASA'sWide-field Infrared Survey Explorer and its subsequentNEOWISE mission, the body measures 6.7 and 7.7 kilometers in diameter, respectively, and its surface has analbedo 0.39.[4][5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.40 and calculates a diameter of 6.4 kilometers with anabsolute magnitude of 12.7.[3]

Naming

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Thisminor planet is named after theKollaa River in Karelia, the focal point of violent battles during the FinnishWinter War (1939–40).[2] The official naming citation was published by theMinor Planet Center on 1 August 1980 (M.P.C. 5450).[11]

Notes

[edit]
  1. ^abRyan (2007) web: rotation period2.980±0.005 hours with a brightness amplitude of0.22 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1929) Kollaa from unpublished results byW. H. Ryan and E.V. Ryan, (2007).

References

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  1. ^abcdef"JPL Small-Body Database Browser: 1929 Kollaa (1939 BS)" (2016-09-14 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved10 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1929) Kollaa".Dictionary of Minor Planet Names – (1929) Kollaa.Springer Berlin Heidelberg. p. 155.doi:10.1007/978-3-540-29925-7_1930.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1929) Kollaa". Asteroid Lightcurve Database (LCDB). Retrieved24 July 2016.
  4. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8.S2CID 46350317. Retrieved24 July 2016.
  5. ^abcdMainzer, 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.S2CID 35447010. Retrieved24 July 2016.
  6. ^abMasiero, 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.S2CID 118745497. Retrieved8 December 2016.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1929) Kollaa".Geneva Observatory. Retrieved24 July 2016.
  8. ^Veres, 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.S2CID 53493339. Retrieved24 July 2016.
  9. ^ab"1929 Kollaa (1939 BS)".Minor Planet Center. Retrieved24 July 2016.
  10. ^Kelley, Michael S.; Vilas, Faith; Gaffey, Michael J.; Abell, Paul A. (September 2003)."Quantified mineralogical evidence for a common origin of 1929 Kollaa with 4 Vesta and the HED meteorites".Icarus.165 (1):215–218.Bibcode:2003Icar..165..215K.doi:10.1016/S0019-1035(03)00149-0. Retrieved18 January 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved24 July 2016.

External links

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