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1982 Cline

From Wikipedia, the free encyclopedia
Main-belt asteroid

1982 Cline
Discovery[1]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date4 November 1975
Designations
(1982) Cline
Named after
Edwin Cline(inventor)[2]
1975 VA · 1936 OO
1957 LN · 1961 XC
1961 XK · 1973 AS
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc59.91 yr (21,882 days)
Aphelion2.8858AU
Perihelion1.7351 AU
2.3104 AU
Eccentricity0.2490
3.51yr (1,283 days)
18.924°
0° 16m 50.16s / day
Inclination6.8421°
42.366°
279.57°
Physical characteristics
Dimensions6.03±0.17 km[4]
7.21±0.50 km[5]
8.100±0.030 km[1][6]
8.18 km(calculated)[3]
8.401±0.064 km[7]
5.78±0.01h[8]
0.194±0.028[1][6]
0.20(assumed)[3]
0.2364±0.0443[7]
0.340±0.050[5]
0.369±0.063[4]
S[3][9]
12.5[5][7] · 12.56±0.39[9] · 12.8[3][4] · 12.9[1]

1982 Cline, provisional designation1975 VA, is a stonyasteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter. It was discovered on 4 November 1975, by American astronomerEleanor Helin atPalomar Observatory in California, and named after Edwin Lee Cline, inventor and friend of the discoverer.[2][10]

Classification and orbit

[edit]

Cline is a stonyS-type asteroid that orbits the Sun in theinner main-belt at a distance of 1.7–2.9 AU once every 3 years and 6 months (1,283 days). Its orbit has aneccentricity of 0.25 and aninclination of 7° with respect to theecliptic.[1] As a main-belt asteroid with aperihelion of less than 1.74 AU, it is not far from being aMars-crosser (1.67 AU).[1] The firstprecovery was taken atJohannesburg Observatory (Hartbeespoort,076) in 1957, extending the asteroid'sobservation arc by 18 years prior to its discovery.[10]

Physical characteristics

[edit]

The body's first and only rotationallightcurve ofCline was obtained by American astronomer James W. Birnsfield at the Via Capote Observatory (G69), California, in November 2011. It gave a well-definedrotation period of5.78±0.01 hours with a brightness variation of 0.36 inmagnitude (U=3).[8]

According to the survey carried out by the JapaneseAkari satellite and the latest data from theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Cline measures 7.2 and 8.1 kilometers in diameter and its surface has analbedo of 0.194 of 0.34, respectively.[5][6] Previous results by WISE/NEOWISE also gave a diameter of 6.03 and 8.4 kilometers.[4][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 8.18 kilometers with anabsolute magnitude of 12.8.[3]

Naming

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Thisminor planet was named in memory of Edwin Lee Cline, a friend of the discoverer and a known inventor in the automotive field who "looked to space as the new frontier".[2] The officialnaming citation was published by theMinor Planet Center on 18 April 1977 (M.P.C. 4158).[11]

References

[edit]
  1. ^abcdefg"JPL Small-Body Database Browser: 1982 Cline (1975 VA)" (2017-05-04 last obs.).Jet Propulsion Laboratory. Retrieved1 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1982) Cline".Dictionary of Minor Planet Names – (1982) Cline.Springer Berlin Heidelberg. p. 160.doi:10.1007/978-3-540-29925-7_1983.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1982) Cline". Asteroid Lightcurve Database (LCDB). Retrieved25 October 2016.
  4. ^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. Retrieved25 October 2016.
  5. ^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)
  6. ^abcMasiero, 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. Retrieved14 September 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. ^abBrinsfield, James W. (April 2011)."Asteroid Lightcurve Analysis at the Via Capote Observatory: 4th Quarter 2010".The Minor Planet Bulletin.38 (2):73–74.Bibcode:2011MPBu...38...73B.ISSN 1052-8091. Retrieved25 October 2016.
  9. ^abVeres, 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. Retrieved25 October 2016.
  10. ^ab"1982 Cline (1975 VA)".Minor Planet Center. Retrieved25 October 2016.
  11. ^Schmadel, Lutz D. "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.

External links

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