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20488 Pic-du-Midi

From Wikipedia, the free encyclopedia
Main-belt asteroid

20488 Pic-du-Midi
Discovery[1]
Discovered byPises Obs.
Discovery sitePises Obs.
Discovery date17 July 1999
Designations
(20488) Pic-du-Midi
Named after
Pic du Midi Observatory
(in the FrenchPyrenees)[2]
1999 OL · 1998 HD60
main-belt · (middle)[3]
background
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc19.28 yr (7,041 days)
Aphelion3.1496AU
Perihelion2.3196 AU
2.7346 AU
Eccentricity0.1518
4.52yr (1,652 days)
342.51°
0° 13m 4.8s / day
Inclination7.0346°
345.85°
354.85°
Physical characteristics
6.64 km(calculated)[3]
7.894±0.199 km[4][5]
2.812±0.0004 h[6]
0.057(assumed)[3]
0.059±0.013[4][5]
C(assumed)[3]
14.167±0.002(R)[6] · 14.2[1][4] · 14.62[3]

20488 Pic-du-Midi (provisional designation1999 OL) is a backgroundasteroid from the middle region of theasteroid belt, approximately 7 kilometers in diameter. It was discovered on 17 July 1999, by astronomers atPises Observatory in southern France.[7] The asteroid was named for thePic du Midi Observatory.[2]

Orbit and classification

[edit]

Pic-du-Midi is a non-family from the main belt'sbackground population. It orbits the Sun in thecentral main-belt at a distance of 2.3–3.1 AU once every 4 years and 6 months (1,652 days). Its orbit has aneccentricity of 0.15 and aninclination of 7° with respect to theecliptic.[1] The firstprecovery was taken bySpacewatch at Kitt Peak in 1997, extending the body'sobservation arc by more than 2 years prior to its official discovery observation at Pises.[7]

Physical characteristics

[edit]

Rotation period

[edit]

In September 2013, a photometriclightcurve of Pic-du-Midi was obtained at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 2.812 hours with a brightness variation of 0.14 inmagnitude (U=2).[6] For an asteroid of its size, Pic-du-Midi has a relatively fast spin rate, not significantly above the 2.2-hour threshold for the so-calledfast rotators.

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Pic-du-Midi measures 7.894 kilometers in diameter, and its surface has analbedo of 0.059,[4][5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo forcarbonaceous asteroids of 0.057 and calculates a diameter of 6.64 kilometers based on anabsolute magnitude of 12.62.[3]

Naming

[edit]

Thisminor planet was named after thePic du Midi Observatory located on thePyrenees mountains in southern France. Founded by theRamond Society in 1881, the observatory pioneered the study of thesolar corona andcosmic rays and was one of the first to use high-resolution techniques.[2] The approved naming citation was published by theMinor Planet Center on 9 March 2001 (M.P.C. 42368).[8]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 20488 Pic-du-Midi (1999 OL)" (2016-05-13 last obs.).Jet Propulsion Laboratory. Retrieved27 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(20488) Pic-du-Midi".Dictionary of Minor Planet Names – (20488) Pic-du-Midi.Springer Berlin Heidelberg. p. 862.doi:10.1007/978-3-540-29925-7_9624.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (20488) Pic-du-Midi". Asteroid Lightcurve Database (LCDB). Retrieved3 March 2017.
  4. ^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.
  5. ^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. Retrieved3 March 2017.
  6. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved3 March 2017.
  7. ^ab"20488 Pic-du-Midi (1999 OL)".Minor Planet Center. Retrieved3 March 2017.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 March 2017.

External links

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