1835 Gajdariya, provisional designation 1970 OE, is a stony Koronian asteroid from the outer region of the asteroid belt, approximately 12.5 kilometers in diameter.
.png) Lightcurve-based 3D-model of Gajdariya | |
| Discovery[1] | |
|---|---|
| Discovered by | T. Smirnova |
| Discovery site | Crimean Astrophysical Obs. |
| Discovery date | 30 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 arc | 59.28 yr (21,653 days) |
| Aphelion | 3.0842 AU |
| Perihelion | 2.5811 AU |
| 2.8326 AU | |
| Eccentricity | 0.0888 |
| 4.77 yr (1,741 days) | |
| 258.14° | |
| 0° 12m 24.12s / day | |
| Inclination | 0.9857° |
| 296.26° | |
| 80.748° | |
| Physical characteristics | |
| Dimensions | 12.40 km (calculated)[3] 12.704±0.035[4] 12.843±0.142 km[5] 13.30±1.04 km[6] |
| 6.3276±0.0035 h[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] | |
It was discovered on 30 July 1970, by Russian astronomer Tamara Smirnova at Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.[10] It was named after Russian writer Arkady Gaidar.[2]
Characteristics
editThe S-type asteroid is a member of the Koronis family, which is named after 158 Koronis and consists of about 300 known bodies with nearly ecliptical orbits. It orbits the Sun in the outer main-belt at a distance of 2.6–3.1 AU once every 4 years and 9 months (1,741 days). Its orbit has an eccentricity of 0.09 and an inclination of 1° with respect to the ecliptic.[1] Its spectra is that of an S-type asteroid with a geometric albedo of about 0.24. It has a rotation period of 6.33 hours.[7][8]
Naming
editIt was named in honor of Soviet–Russian writer and children's author Arkady Gaidar (1904–1941), who joined the partisans and became a machine gunner during the Nazi invasion of the Soviet Union.[2] Gaidar was killed in combat in October 1941. The official naming citation was published by the Minor Planet Center on 1 June 1975 (M.P.C. 3825).[11]
References
edit- ^ a b c d "JPL Small-Body Database Browser: 1835 Gajdariya (1970 OE)" (2017-05-02 last obs.). Jet Propulsion Laboratory. Retrieved 8 June 2017.
- ^ a b c Schmadel, 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.
- ^ a b c d e "LCDB Data for (1835) Gajdariya". Asteroid Lightcurve Database (LCDB). Retrieved 14 December 2016.
- ^ a b Masiero, 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. Retrieved 14 December 2016.
- ^ a b c Mainzer, 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.
- ^ a b c Masiero, 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. Retrieved 14 December 2016.
- ^ a b Molnar, 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. Retrieved 14 December 2016.
{{cite journal}}: CS1 maint: multiple names: authors list (link) - ^ a b Hanus, 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. Retrieved 14 December 2016.
- ^ 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. Retrieved 14 December 2016.
- ^ "1835 Gajdariya (1970 OE)". Minor Planet Center. Retrieved 14 December 2016.
- ^ 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
edit- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1835 Gajdariya at AstDyS-2, Asteroids—Dynamic Site
- 1835 Gajdariya at the JPL Small-Body Database
