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1190 Pelagia

From Wikipedia, the free encyclopedia
Dark Nysian asteroid

1190 Pelagia
Discovery[1]
Discovered byG. Neujmin
Discovery siteSimeiz Obs.
Discovery date20 September 1930
Designations
(1190) Pelagia
Named after
Pelageya Shajn
(Soviet–Russian astronomer)[2]
1930 SL · 1928 DP
1938 YA · 1953 VB
1953 XP · A909 BC
main-belt · (inner)
Nysa[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc108.44 yr (39,609 days)
Aphelion2.7530AU
Perihelion2.1096 AU
2.4313 AU
Eccentricity0.1323
3.79yr (1,385 days)
284.95°
0° 15m 36s / day
Inclination3.1697°
26.477°
41.199°
Physical characteristics
Dimensions15.05±3.86 km[4]
17.30±0.27 km[5]
17.39 km(derived)[3]
17.923±0.185 km[6]
2.3661±0.0003h[7]
0.031±0.042[6]
0.0486(derived)[3]
0.054±0.018[4]
0.067±0.002[5]
X[8] · C[3]
12.40[5] · 12.60[4] · 12.7[1][3] · 12.78±0.23[8] · 13.13[6]

1190 Pelagia, provisional designation1930 SL, is a dark Nysianasteroid from the inner regions of theasteroid belt, approximately 17 kilometers in diameter. It was discovered on 20 September 1930, by Soviet–Georgian astronomerGrigory Neujmin at theSimeiz Observatory on the Crimean peninsula.[9] The asteroid was named after astronomerPelageya Shajn.[2]

Classification and orbit

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Pelagia is a member of theNysa family (405),[3] a prominent family of theinner main-belt, named after44 Nysa.

It orbits the Sun at a distance of 2.1–2.8 AU once every 3 years and 9 months (1,385 days). Its orbit has aneccentricity of 0.13 and aninclination of 3° with respect to theecliptic.[1] The asteroid'sobservation arc begins atHeidelberg Observatory in January 1909, when it was identified asA909 BC, more than 21 years prior to its official discovery observation at Simeiz.[9]

Physical characteristics

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The asteroid has been characterized as anX-type asteroid byPan-STARRS photometric survey.[8]

Lightcurve

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In December 2010, a rotationallightcurve ofPelagia was obtained from photometric observations by Japanese astronomer couple Hiromi and Hiroko Hamanowa. Lightcurve analysis gave a well-definedrotation period of 2.3661 hours with a brightness amplitude of 0.08magnitude (U=3).[7]

While not being afast rotator, the body has a notably short period for an asteroid of its size. Based on the lightcurve's low amplitude, it appears to have a ratherspheroidal shape.

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Pelagia measures between 15.05 and 17.923 kilometers in diameter and its surface has analbedo between 0.031 and 0.067.[4][5][6] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0486 and a diameter of 17.39 kilometers based on anabsolute magnitude of 12.7.[3]

Naming

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Thisminor planet was named in honor of Soviet–Russian astronomerPelageya Shajn (1894–1956). In 1928, she discovered the asteroid1112 Polonia and became the first femalediscoverer of minor planets (RI 895).[2] A second asteroid,1648 Shajna, was also named in her and her husbands memory (Grigory Shajn).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1190 Pelagia (1930 SL)" (2017-07-05 last obs.).Jet Propulsion Laboratory. Retrieved16 August 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1190) Pelagia".Dictionary of Minor Planet Names – (1190) Pelagia.Springer Berlin Heidelberg. p. 100.doi:10.1007/978-3-540-29925-7_1191.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1190) Pelagia". Asteroid Lightcurve Database (LCDB). Retrieved16 August 2017.
  4. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved16 August 2017.
  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. ^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. Retrieved16 August 2017.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1190) Pelagia".Geneva Observatory. Retrieved16 August 2017.
  8. ^abcVeres, 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. Retrieved16 August 2017.
  9. ^ab"1190 Pelagia (1930 SL)".Minor Planet Center. Retrieved16 August 2017.
  10. ^Schmadel, Lutz D. (2007). "(1648) Shajna".Dictionary of Minor Planet Names – (1648) Shajna. Springer Berlin Heidelberg. p. 131.doi:10.1007/978-3-540-29925-7_1649.ISBN 978-3-540-00238-3.

External links

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Minor planets
Asteroid
Distant minor planet
Comets
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