Astronomy:3409 Abramov
Discovery [1] | |
---|---|
Discovered by | N. Chernykh |
Discovery site | Crimean Astrophysical Obs. |
Discovery date | 9 September 1977 |
Designations | |
(3409) Abramov | |
Named after | Fyodor Abramov (Russian writer)[2] |
1977 RE6 · 1929 UP 1929 VD · 1948 TW1 1958 VU · 1972 TF5 1979 BS1 · 1980 GF1 1982 VY5 · 1985 GD1 | |
Minor planet category | main-belt · Koronis [3] |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 87.42 yr (31,930 days) |
|{{{apsis}}}|helion}} | 3.0914 AU |
|{{{apsis}}}|helion}} | 2.6174 AU |
2.8544 AU | |
Eccentricity | 0.0830 |
Orbital period | 4.82 yr (1,761 days) |
Mean anomaly | 92.335° |
Mean motion | 0° 12m 15.84s / day |
Inclination | 1.4019° |
Longitude of ascending node | 211.41° |
168.58° | |
Physical characteristics | |
Dimensions | 10.765±0.168 km[4][5] 10.80 km (calculated)[3] 11.402±1.938[lower-alpha 1] |
Rotation period | 7.791±0.002 h[6] 9.0±0.4 h[7] |
Geometric albedo | 0.236±0.044[lower-alpha 1] 0.24 (assumed)[3] 0.242±0.060[4][5] |
S [3] | |
Absolute magnitude (H) | 12.0[1][3][4][lower-alpha 1] |
3409 Abramov, provisional designation 1977 RE6, is a stony Koronian asteroid from the outer region of the asteroid belt, approximately 11 kilometers in diameter. It was discovered on 9 September 1977, by Soviet–Russian astronomer Nikolai Chernykh at Crimean Astrophysical Observatory in Nauchnyj on the Crimean peninsula.[8] The asteroid was named after Russian writer Fyodor Abramov.[2]
Orbit and classification
The S-type asteroid is a member of the Koronis family, a group consisting of about 200 known stony 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 10 months (1,761 days). Its orbit has an eccentricity of 0.08 and an inclination of 1° with respect to the ecliptic.[1] The first precovery was obtained at Lowell Observatory in 1929, extending the asteroid's observation arc by 48 years prior to its discovery.[8]
Physical characteristics
Lightcurves
In 2008, a photometric lightcurve analysis at the Universidad de Monterry Observatory, Mexico, gave a well-defined rotation period of 7.791±0.002 hours with a brightness amplitude of 0.50 in magnitude ({{{1}}}),[6] while an observation by astronomer René Roy rendered a tentative period of 9.0±0.4 hours ({{{1}}}).[7]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of the NASA's space-based Wide-field Infrared Survey Explorer, the asteroid has an albedo of 0.24 with a corresponding diameter of 10.8 kilometers.[4][5] The Collaborative Asteroid Lightcurve Link and others closely agree with these findings.[3][lower-alpha 1]
Naming
This minor planet was named in memory of Russian novelist and literary critic Fyodor Abramov (1920–1983), whose work focused on the difficult lives of the Russian peasant class.[2] The official naming citation was published by the Minor Planet Center on 1 September 1993 (M.P.C. 22498).[9]
Notes
- ↑ 1.0 1.1 1.2 1.3 Ryan (2015): mean diameter of 11.402±1.938 and an albedo of 0.236±0.044. Summary figures for (3409) Abramov at Collaborative Asteroid Lightcurve Link (CALL)
References
- ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 3409 Abramov (1977 RE6)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2003409.
- ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(3409) Abramov". Dictionary of Minor Planet Names – (3409) Abramov. Springer Berlin Heidelberg. p. 284. doi:10.1007/978-3-540-29925-7_3409. ISBN 978-3-540-00238-3.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 "LCDB Data for (3409) Abramov". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=3409%7CAbramov.
- ↑ 4.0 4.1 4.2 4.3 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. doi:10.1088/0004-637X/741/2/90. Bibcode: 2011ApJ...741...90M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M. Retrieved 27 April 2016.
- ↑ 5.0 5.1 5.2 Masiero, 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. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 5 December 2016.
- ↑ 6.0 6.1 Sada, Pedro V. (September 2008). "CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory". The Minor Planet Bulletin 35 (3): 105–107. ISSN 1052-8091. Bibcode: 2008MPBu...35..105S. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2008MPBu...35..105S. Retrieved 13 January 2016.
- ↑ 7.0 7.1 Behrend, Raoul. "Asteroids and comets rotation curves – (3409) Abramov". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#003409.
- ↑ 8.0 8.1 "3409 Abramov (1977 RE6)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=3409.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html.
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
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 3409 Abramov at AstDyS-2, Asteroids—Dynamic Site
- 3409 Abramov at the JPL Small-Body Database
Original source: https://en.wikipedia.org/wiki/3409 Abramov.
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