Astronomy:17163 Vasifedoseev

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17163 Vasifedoseev
Discovery[1]
Discovered byLINEAR
Discovery siteLincoln Lab's ETS
Discovery date9 June 1999
Designations
(17163) Vasifedoseev
Named afterVasiliy Fedoseev
(2003 ISEF awardee)[2]
1999 LT19 · 1990 QY10
1994 LC4 · 1995 SY12
1998 FE39 · 1998 FN140
Minor planet categorymain-belt · Koronis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc26.62 yr (9,723 days)
|{{{apsis}}}|helion}}3.1357 AU
|{{{apsis}}}|helion}}2.6708 AU
2.9032 AU
Eccentricity0.0801
Orbital period4.95 yr (1,807 days)
Mean anomaly163.48°
Mean motion0° 11m 57.12s / day
Inclination1.3220°
Longitude of ascending node343.23°
2.8711°
Physical characteristics
Dimensions3.67 km (calculated)[3]
4.863±0.268 km[4][5]
Rotation period4.1124±0.0006 h[6]
Geometric albedo0.171±0.045[4][5]
0.24 (assumed)[3]
S[3][7]
Absolute magnitude (H)14.0[1] · 14.1[4] · 14.26±0.29[7] · 14.34[3] · 13.891±0.003 (R)[6]


17163 Vasifedoseev (provisional designation 1999 LT19) is a stony Koronian asteroid from the outer region of the asteroid belt, approximately 4 kilometers in diameter.

The asteroid was discovered on 9 June 1999, by the Lincoln Near-Earth Asteroid Research team at Lincoln Laboratory's ETS in Socorro, New Mexico, United States.[8] It was named for Vasiliy Fedoseev, an awardee of the ISEF contest in 2003.[2]

Orbit and classification

Vasifedoseev is a member of the Koronis family, a family of stony asteroids in the outer main-belt. It orbits the Sun at a distance of 2.7–3.1 AU once every 4 years and 11 months (1,807 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 ESO's La Silla Observatory in 1990, extending the asteroid's observation arc by 9 years prior to its discovery.[8]

Physical characteristics

Rotation period

A rotational lightcurve of Vasifedoseev was obtained from photometric observations by the wide-field survey at the Palomar Transient Factory in September 2010. Lightcurve analysis gave a rotation period of 4.1124 hours with a brightness variation of 0.23 magnitude ({{{1}}}).[6]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Vasifedoseev measures 4.9 kilometers in diameter and its surface has an albedo of 0.17,[4][5] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 and calculates a diameter of 3.7 kilometers with an absolute magnitude of 14.34.[3]

Naming

This minor planet was named after Russian Vasiliy G. Fedoseev (born 1986) an awardee of the Intel International Science and Engineering Fair (ISEF) in 2003. At the time, he attended the Lyceum of Information Technologies Moscow, Russia.[2] The official naming citation was published by the Minor Planet Center on 14 June 2004 (M.P.C. 52172).[9]

References

  1. 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 17163 Vasifedoseev (1999 LT19)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2017163. 
  2. 2.0 2.1 2.2 Schmadel, Lutz D. (2006). "(17163) Vasifedoseev [2.90, 0.08, 1.3]". Dictionary of Minor Planet Names – (17163) Vasifedoseev, Addendum to Fifth Edition: 2003–2005. Springer Berlin Heidelberg. p. 107. doi:10.1007/978-3-540-34361-5_1132. ISBN 978-3-540-34360-8. 
  3. 3.0 3.1 3.2 3.3 3.4 3.5 "LCDB Data for (17163) Vasifedoseev". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=17163%7CVasifedoseev. 
  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 17 May 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 3 December 2016. 
  6. 6.0 6.1 6.2 Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal 150 (3): 35. doi:10.1088/0004-6256/150/3/75. Bibcode2015AJ....150...75W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W. Retrieved 17 May 2016. 
  7. 7.0 7.1 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. doi:10.1016/j.icarus.2015.08.007. Bibcode2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 17 May 2016. 
  8. 8.0 8.1 "17163 Vasifedoseev (1999 LT19)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=17163. 
  9. "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. 

External links