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1987 Kaplan

From Wikipedia, the free encyclopedia
Main-belt asteroid

1987 Kaplan
Lightcurve-based 3D-model ofKaplan
Discovery[1]
Discovered byP. F. Shajn
Discovery siteSimeiz Obs.
Discovery date11 September 1952
Designations
(1987) Kaplan
Named after
Samuil Kaplan[2]
(Soviet astrophysicist)
1952 RH
main-belt · (inner)
Phocaea[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc64.54 yr (23,573 days)
Aphelion2.9234AU
Perihelion1.8422 AU
2.3828 AU
Eccentricity0.2269
3.68yr (1,343 days)
238.97°
0° 16m 4.8s / day
Inclination23.645°
314.23°
38.176°
Physical characteristics
Dimensions11.70±2.27 km[5]
13.017±0.159 km[6]
13.52±0.39 km[7]
13.89 km(calculated)[3]
14.606±0.104 km[8]
9.453±0.002h[9][a]
9.45950±0.00005 h[10]
9.46±0.01 h[11][b]
9.49±0.02 h[12]
0.2094±0.0448[8]
0.23(assumed)[3]
0.262±0.053[6]
0.278±0.017[7]
0.28±0.12[5]
S(assumed)[3]
11.40[7] · 11.5[1][3][8] · 11.81[5] · 12.23±1.34[13]

1987 Kaplan, provisional designation1952 RH, is a stony Phocaeaasteroid from the inner regions of theasteroid belt, approximately 14 kilometers in diameter. It was discovered on 11 September 1952, by Soviet astronomerPelageya Shajn at theSimeiz Observatory on the Crimean peninsula.[14] The asteroid was named after Soviet astrophysicistSamuil Kaplan.[2]

Orbit and classification

[edit]

Kaplan is a member of thePhocaea family (701),[3][4] a largefamily of stony asteroids with nearly two thousand known members.[15]: 23 

It orbits the Sun in theinner main belt at a distance of 1.8–2.9 AU once every 3 years and 8 months (1,343 days). Its orbit has aneccentricity of 0.23 and aninclination of 24° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Simeiz in September 1952.[14]

Physical characteristics

[edit]

Kaplan is an assumedS-type asteroid, in agreement with the overallspectral type of thePhocaea family.[15]: 23 

Rotation period

[edit]

Between 2000 and 2011, three rotationallightcurves ofKaplan were obtained from photometric observations by astronomerBrian Warner at his Palmer Divide Observatory in Colorado, United States. Lightcurve analysis gave a well-definedrotation period between 9.453 and 9.49 hours with a brightness amplitude from 0.46 to 0.65magnitude (U=3/3/3).[9][11][12][b][a]

Poles

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In addition a modeled lightcurve, using photometric data from various sources, gave a concurring period of 9.45950 hours and determined two spin axis of (356.0°, −58.0°) and (233.0°, −89.0°) inecliptic coordinates.[10]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Kaplan measures between 11.70 and 14.606 kilometers in diameter and its surface has analbedo between 0.2094 and 0.28.[5][6][7][8]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.23 – derived from25 Phocaea, the family's parent body and namesake, and calculates a diameter of 13.89 kilometers based on anabsolute magnitude of 11.5.[3]

Naming

[edit]

Thisminor planet was named afterSamuil Kaplan (1921–1978), Soviet astronomer and astrophysicist at Lvov University Observatory (067), Ukraine, and at theRadiophysical Research Institute in Nizhny Novgorod (formerly known as Gorky), Russia. His research included a variety of astrophysical fields, such aswhite dwarfs,interstellar matter,radiative transfer,solar radiation,pulsars andgalactic nuclei.[2]

The official naming citation was published by theMinor Planet Center on 1 June 1980 (M.P.C. 5358).[16]

Notes

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  1. ^abLightcurve plot of (1987) Kaplan, Brian Warner at the Palmer Divide Observatory (2011). Rotation period9.453±0.002 hours with a brightness amplitude of0.65±0.02 mag. Quality code of 3. Summary figures at theLCDB.
  2. ^abLightcurve plot of (1987) Kaplan, Brian Warner at the Palmer Divide Observatory (2000). Rotation period9.46±0.01 hours with a brightness amplitude of0.47±0.01 mag. Quality code of 3. Summary figures at theLCDB.

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1987 Kaplan (1952 RH)" (2017-03-27 last obs.). Jet Propulsion Laboratory. Retrieved1 November 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1987) Kaplan".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 161.doi:10.1007/978-3-540-29925-7_1988.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1987) Kaplan". Asteroid Lightcurve Database (LCDB). Retrieved1 November 2017.
  4. ^ab"Asteroid 1987 Kaplan – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  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. Retrieved1 November 2017.
  7. ^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)
  8. ^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.
  9. ^abWarner, Brian D. (April 2012)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2011 September – December".The Minor Planet Bulletin.39 (2):69–80.Bibcode:2012MPBu...39...69W.ISSN 1052-8091. Retrieved1 November 2017.
  10. ^abHanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013)."An anisotropic distribution of spin vectors in asteroid families".Astronomy and Astrophysics.559: 19.arXiv:1309.4296.Bibcode:2013A&A...559A.134H.doi:10.1051/0004-6361/201321993. Retrieved1 November 2017.
  11. ^abWarner, Brian D. (January 2011)."Upon Further Review: V. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory".The Minor Planet Bulletin.38 (1):63–65.Bibcode:2011MPBu...38...63W.ISSN 1052-8091. Retrieved1 November 2017.
  12. ^abWarner, B. (September 2001)."Asteroid Photometry at the Palmer Divide Observatory".The Minor Planet Bulletin.28:40–41.Bibcode:2001MPBu...28...40W. Retrieved1 November 2017.
  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. Retrieved1 November 2017.
  14. ^ab"1987 Kaplan (1952 RH)".Minor Planet Center. Retrieved1 November 2017.
  15. ^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.
  16. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved1 November 2017.

External links

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