Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

2014 Vasilevskis

From Wikipedia, the free encyclopedia
Asteroid

2014 Vasilevskis
Discovery[1]
Discovered byA. R. Klemola
Discovery siteLick Obs.
Discovery date2 May 1973
Designations
(2014) Vasilevskis
Named after
Stanislavs Vasilevskis
(astronomer; staff member)[2]
1973 JA
main-belt · Phocaea[3][4]
Orbital characteristics[5]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc44.00 yr (16,072 days)
Aphelion3.0908AU
Perihelion1.7134 AU
2.4021 AU
Eccentricity0.2867
3.72yr (1,360 days)
295.50°
0° 15m 52.92s / day
Inclination21.376°
204.09°
82.819°
Physical characteristics
9.044±0.043 km[6]
9.071±0.051 km[7]
11.84±0.81 km[8]
15.6±0.1h[9]
32.16±0.02 h[10]
36.25 h[11]
39±2 h[12]
0.23(assumed)[3]
0.265±0.038[8]
0.309±0.041[6]
0.4513±0.1032[7]
S[3]
11.7[7][8] · 12.3[5][3] · 12.76±1.16[13]

2014 Vasilevskis, provisional designation1973 JA, is a stony Phocaeanasteroid from the inner regions of theasteroid belt, approximately 10 kilometers (6.2 mi) in diameter. It was discovered on 2 May 1973, by American astronomer Arnold Klemola at the U.S.Lick Observatory on Mount Hamilton, California. It was named after Stanislavs Vasilevskis, staff member at the discovering observatory.[2][1]

Orbit and classification

[edit]

Vasilevskis is a member of thePhocaea family (701),[4] a group of asteroids with similar orbital characteristics, named after the family's namesake,25 Phocaea. It orbits the Sun in theinner main-belt at a distance of 1.7–3.1 AU once every 3 years and 9 months (1,360 days). Its orbit has aneccentricity of 0.29 and aninclination of 21° with respect to theecliptic.[5] Noprecoveries were taken prior to its discovery.[1]

Physical characteristics

[edit]

Vasilevskis has been characterized as a commonS-type asteroid.[3]

Rotation period

[edit]

In May 2014, a photometriclightcurve analysis by American astronomerRobert Stephens at the Center for Solar System Studies (U81), California, gave arotation period of32.16±0.02 hours with a brightness variation of 0.26 inmagnitude (U=3-).[10]

Alternative measurements also made in 2014, include an observation by astronomerRené Roy, which rendered a period of39±2 hours with an amplitude of 0.31 in magnitude (U=2),[12] and an analysis at the Burleith Observatory (I13), with a period of15.6±0.1 hours, or 49% of the first period (U=2-).[9]

Diameter and albedo

[edit]

According to the space-based surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the asteroid measures between 9.1 and 11.8 kilometers in diameter, and its surface has analbedo between 0.265 and 0.451.[8][7] TheCollaborative Asteroid Lightcurve Link assumes an albedo 0.23 – derived from 25 Phocaea, the family's largest member and namesake – and calculates a diameter of 9.6 kilometers with anabsolute magnitude of 12.3.[3]

Naming

[edit]

Thisminor planet was named after astronomer Stanislavs Vasilevskis (died 1988), long-time staff member at the discovering Lick Observatory from 1949 to 1974.[2]

A specialist forastrometric instrumentation, in particular the computational analysis of the position of astronomical objects fromphotographic plates, he has also performed broad astronomical surveys to obtain theparallax andproper motion of stars.[2] The officialnaming citation was published by theMinor Planet Center on 30 June 1977 (M.P.C. 4190).[14]

References

[edit]
  1. ^abc"2014 Vasilevskis (1973 JA)".Minor Planet Center. Retrieved29 March 2016.
  2. ^abcdSchmadel, Lutz D. (2007). "(2014) Vasilevskis".Dictionary of Minor Planet Names – (2014) Vasilevskis.Springer Berlin Heidelberg. p. 163.doi:10.1007/978-3-540-29925-7_2015.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2014) Vasilevskis". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^ab"Asteroid 2014 Vasilevskis".Small Bodies Data Ferret. Retrieved22 October 2019.
  5. ^abc"JPL Small-Body Database Browser: 2014 Vasilevskis (1973 JA)" (2017-05-03 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 7 September 2020. Retrieved10 June 2017.
  6. ^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. Retrieved8 December 2016.
  7. ^abcdMainzer, 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. Retrieved17 May 2016.
  8. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  9. ^abSchmidt, Richard E. (January 2015)."NIR Minor Planet Photometry from Burleith Observatory: 2014 February - June".The Minor Planet Bulletin.42 (1):1–3.Bibcode:2015MPBu...42....1S.ISSN 1052-8091. Retrieved17 May 2016.
  10. ^abStephens, Robert D. (October 2014)."Asteroids Observed from CS3: 2014 April-June".The Minor Planet Bulletin.41 (4):226–230.Bibcode:2014MPBu...41..226S.ISSN 1052-8091. Retrieved17 May 2016.
  11. ^Holliday, B. (December 1995)."Lightcurve Observations of Minor Planets 1508 Kemi and 2014 Vasilevskis".The Minor Planet Bulletin.22.: 43.Bibcode:1995MPBu...22...43H. Retrieved17 May 2016.
  12. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2014) Vasilevskis".Geneva Observatory. Retrieved17 May 2016.
  13. ^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. Retrieved17 May 2016.
  14. ^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.


Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=2014_Vasilevskis&oldid=1321112061"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp