Astronomy:3409 Abramov

From HandWiki
Revision as of 05:53, 6 February 2024 by Steve Marsio (talk | contribs) (link)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
3409 Abramov
Discovery [1]
Discovered byN. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date9 September 1977
Designations
(3409) Abramov
Named afterFyodor 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 categorymain-belt · Koronis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.42 yr (31,930 days)
|{{{apsis}}}|helion}}3.0914 AU
|{{{apsis}}}|helion}}2.6174 AU
2.8544 AU
Eccentricity0.0830
Orbital period4.82 yr (1,761 days)
Mean anomaly92.335°
Mean motion0° 12m 15.84s / day
Inclination1.4019°
Longitude of ascending node211.41°
168.58°
Physical characteristics
Dimensions10.765±0.168 km[4][5]
10.80 km (calculated)[3]
11.402±1.938[lower-alpha 1]
Rotation period7.791±0.002 h[6]
9.0±0.4 h[7]
Geometric albedo0.236±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. 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. 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. 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. 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. 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. Bibcode2011ApJ...741...90M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M. Retrieved 27 April 2016. 
  5. 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. Bibcode2011ApJ...741...68M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 5 December 2016. 
  6. 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. Bibcode2008MPBu...35..105S. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2008MPBu...35..105S. Retrieved 13 January 2016. 
  7. 7.0 7.1 Behrend, Raoul. "Asteroids and comets rotation curves – (3409) Abramov". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#003409. 
  8. 8.0 8.1 "3409 Abramov (1977 RE6)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=3409. 
  9. "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. 

External links