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4997 Ksana

From Wikipedia, the free encyclopedia
Asteroid

4997 Ksana
Discovery[1]
Discovered byL. G. Karachkina
Discovery siteCrimean Astrophysical Obs.
Discovery date6 October 1986
Designations
(4997) Ksana
Named after
Kseniya A. Nessler
(Russian chemist)[2]
1986 TM
main-belt · (outer)[3]
Pallas[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc30.57 yr (11,165 days)
Aphelion3.8162AU
Perihelion1.9285 AU
2.8723 AU
Eccentricity0.3286
4.87yr (1,778 days)
97.646°
0° 12m 9s / day
Inclination32.828°
10.897°
57.447°
Physical characteristics
Dimensions7.36±2.79 km[5]
9.860±0.160 km[6][7]
9.97±0.33 km[8]
10±1 km[9]
14.64 km(calculated)[3]
3.4342±0.0003h[10]
0.057(assumed)[3]
0.16±0.03[9]
0.271±0.206[5]
0.312±0.022[8]
0.3157±0.0548[7]
0.316±0.055[6]
SMASS =B[1] · B[3]
11.9[3][7][8] · 12.70[5][9] · 12.79±0.30[11] · 13.0[1]

4997 Ksana, provisional designation1986 TM, is a carbonaceous Palladianasteroid from the outer region of theasteroid belt, approximately 10 kilometers in diameter. It was discovered on 6 October 1986, by Russian astronomerLyudmila Karachkina atCrimean Astrophysical Observatory on the Crimean peninsula.[12] The asteroid was named for Russian chemistKseniya Nessler.[2]

Orbit and classification

[edit]

Ksana is a small member of thePallas family (801), a smallasteroid family of carbonaceous B-type asteroids.[4][13]: 23  It orbits the Sun in theouter main-belt at a distance of 1.9–3.8 AU once every 4 years and 10 months (1,778 days). Its orbit has aneccentricity of 0.33 and aninclination of 33° with respect to theecliptic.[1]As noprecoveries were taken, the asteroid'sobservation arc begins with its discovery observation in 1986.[12]

Physical characteristics

[edit]

On theSMASS taxonomic scheme,Ksana is aB-type asteroid, which are primitive, volatile-rich asteroids.[1] This also agrees with the overallspectral type of the Pallas family.[13]: 23 

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Ksana measures between 7.36 and10±1 kilometers in diameter and its surface has analbedo between 0.16 and 0.316.[5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a larger diameter of 14.64 kilometers with anabsolute magnitude of 12.9.[3]

Rotation period

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In February 2007, a rotationallightcurve ofKsana was obtained from photometric observations by Italian astronomer Federico Manzini at the SAS observatory in Novara, Italy. It gave it arotation period of3.4342±0.0003 hours with a brightness variation of 0.21 inmagnitude (U=2).[10]

Naming

[edit]

Thisminor planet was named by the discoverer for his friend, the Russian chemist Kseniya Andreevna Nessler, who has been an advocate against environmental pollution. The asteroid's name "Ksana" is a variation of Kseniya (Ксения), the equivalent to the romanizedXenia.[2] The official naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22505 and 22609).[14]

References

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  1. ^abcdef"JPL Small-Body Database Browser: 4997 Ksana (1986 TM)" (2017-05-01 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 17 September 2020. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4997) Ksana".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 430.doi:10.1007/978-3-540-29925-7_4870.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (4997) Ksana". Asteroid Lightcurve Database (LCDB). Retrieved30 October 2016.
  4. ^ab"Asteroid 4997 Ksana – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  5. ^abcdMasiero, 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. Retrieved30 October 2016.
  6. ^abcMasiero, 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.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved30 October 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.
  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. ^abcdAlí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013)."Physical properties of B-type asteroids from WISE data".Astronomy and Astrophysics.554: 16.arXiv:1303.5487.Bibcode:2013A&A...554A..71A.doi:10.1051/0004-6361/201220680. Retrieved30 October 2016.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (4997) Ksana".Geneva Observatory. Retrieved30 October 2016.
  11. ^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. Retrieved30 October 2016.
  12. ^ab"4997 Ksana (1986 TM)".Minor Planet Center. Retrieved30 October 2016.
  13. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 978-0-8165-3213-1.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved30 October 2016.

External links

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