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1835 Gajdariya

From Wikipedia, the free encyclopedia
Main-belt asteroid

1835 Gajdariya
Lightcurve-based 3D-model ofGajdariya
Discovery[1]
Discovered byT. Smirnova
Discovery siteCrimean Astrophysical Obs.
Discovery date30 July 1970
Designations
(1835) Gajdariya
Named after
Arkady Gaidar
(Russian writer)[2]
1970 OE · 1958 BH
1961 TJ · 1961 TQ1
1963 DB · 1971 UJ3
1973 EN
main-belt · Koronis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc59.28 yr (21,653 days)
Aphelion3.0842AU
Perihelion2.5811 AU
2.8326 AU
Eccentricity0.0888
4.77yr (1,741 days)
258.14°
0° 12m 24.12s / day
Inclination0.9857°
296.26°
80.748°
Physical characteristics
Dimensions12.40 km(calculated)[3]
12.704±0.035[4]
12.843±0.142 km[5]
13.30±1.04 km[6]
6.3276±0.0035h[7]
6.33768 h[8]
0.209±0.040[6][4]
0.24(assumed)[3]
0.2703±0.0433[5]
S[3]
11.5[5] · 11.7[1][3][6] · 11.70±0.28[9]

1835 Gajdariya, provisional designation1970 OE, is a stony Koronianasteroid from the outer region of theasteroid belt, approximately 12.5 kilometers in diameter.

It was discovered on 30 July 1970, by Russian astronomerTamara Smirnova atCrimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.[10] It was named after Russian writerArkady Gaidar.[2]

Characteristics

[edit]

TheS-type asteroid is a member of theKoronis family, which is named after158 Koronis and consists of about 300 known bodies with nearlyecliptical orbits. It orbits the Sun in theouter main-belt at a distance of 2.6–3.1 AU once every 4 years and 9 months (1,741 days). Its orbit has aneccentricity of 0.09 and aninclination of 1° with respect to the ecliptic.[1] Its spectra is that of anS-type asteroid with ageometric albedo of about 0.24. It has arotation period of 6.33 hours.[7][8]

Naming

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It was named in honor of Soviet–Russian writer and children's authorArkady Gaidar (1904–1941), who joined the partisans and became a machine gunner during theNazi invasion of the Soviet Union.[2] Gaidar was killed in combat in October 1941. The officialnaming citation was published by theMinor Planet Center on 1 June 1975 (M.P.C. 3825).[11]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1835 Gajdariya (1970 OE)" (2017-05-02 last obs.).Jet Propulsion Laboratory. Retrieved8 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1835) Gajdariya".Dictionary of Minor Planet Names – (1835) Gajdariya.Springer Berlin Heidelberg. p. 147.doi:10.1007/978-3-540-29925-7_1836.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (1835) Gajdariya". Asteroid Lightcurve Database (LCDB). Retrieved14 December 2016.
  4. ^abMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved14 December 2016.
  5. ^abcMainzer, 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.
  6. ^abcMasiero, 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. Retrieved14 December 2016.
  7. ^abMolnar, Lawrence A.; Haegert, Melissa, J.; Beaumont, Christopher N.; Block, Marjorie J.; Brom, Timothy H.; Butler, Andrew R.; et al. (March 2008)."Lightcurve Analysis of a Magnitude Limited Asteroid Sample".The Minor Planet Bulletin.35 (1):9–12.Bibcode:2008MPBu...35....9M.ISSN 1052-8091. Retrieved14 December 2016.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  8. ^abHanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013)."An anisotropic distribution of spin vectors in asteroid families".Astronomy and Astrophysics.559: 19.arXiv:1309.4296.Bibcode:2013A&A...559A.134H.doi:10.1051/0004-6361/201321993. Retrieved14 December 2016.
  9. ^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. Retrieved14 December 2016.
  10. ^"1835 Gajdariya (1970 OE)".Minor Planet Center. Retrieved14 December 2016.
  11. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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