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9260 Edwardolson

From Wikipedia, the free encyclopedia
Asteroid

9260 Edwardolson
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date8 October 1953
Designations
(9260) Edwardolson
Named after
Edward C. Olson
(astronomer)[2]
1953 TA1 · 1991 QH
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.48 yr (23,185 days)
Aphelion2.8164AU
Perihelion1.7638 AU
2.2901 AU
Eccentricity0.2298
3.47yr (1,266 days)
165.54°
0° 17m 3.84s / day
Inclination5.0979°
214.59°
148.34°
Knownsatellites1[a][4]
Physical characteristics
Dimensions4.05 km(taken)[3]
4.052 km[5]
4.115±0.362 km[6][7]
3.0852±0.0001h[8]
0.1643[5]
0.262±0.037[6][7]
S[3]
14.0[6] · 14.1[1] · 14.54±0.086[5][3]

9260 Edwardolson, provisional designation1953 TA1, is a Florianbinary[a]asteroid from the inner regions of theasteroid belt, approximately 4.1 kilometers in diameter. It was discovered on 8 October 1953, byIndiana University during itsIndiana Asteroid Program atGoethe Link Observatory in Brooklyn, Indiana, United States.[9] It was named for American astronomerEdward Olson.[2]

Classification and orbit

[edit]

Edwardolson is a member of theFlora family, one of the largest families ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 1.8–2.8 AU once every 3 years and 6 months (1,266 days). Its orbit has aneccentricity of 0.23 and aninclination of 5° with respect to theecliptic.[1] As noprecoveries were taken, the asteroid'sobservation arc begins with its official discovery observation in 1953.[9]

Diameter, albedo and rotation

[edit]

A rotationallightcurve ofEdwardolson was obtained from photometric observations in several locations including the SlovakianSkalnaté pleso Observatory. It rendered arotation period of3.0852±0.0001 hours with a low brightness variation of 0.11 inmagnitude, which suggests that the body has a nearly spheroidal shape (U=n/a).[8] According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the asteroid has analbedo of 0.26 and 0.16, and an respective absolute magnitude of 14.0 and 14.54. Both data sets converge to a diameter of 4.1 kilometers.[5][6][7]

Moon

[edit]

Aminor-planet moon orbitingEdwardolson was discovered in 2005, making it abinary system. The satellite has a fairly shortorbital period of 17 hours, 47 minutes, and 2 seconds (17.785±0.003 hours),[4] and an estimated mean-diameter ratio of0.27±0.03, which would give the satellite a diameter of approximately 1.0 to 1.3 kilometers.[a]

Naming

[edit]

Thisminor planet was named in honor of American astronomer Edward C. Olson (born 1930) of theUniversity of Illinois whose observations explained the distortion of the outer layers of mass-gaining stars, and how their rotation can come close to the stability limit during the involved mass-transfer process and the preserved angular momentum.[2] Olson was also an active member of theInternational Astronomical Union, affiliated with its DivisionG Stars and Stellar Physics.[10] The approved naming citation was published by theMinor Planet Center on 13 July 2004 (M.P.C. 52322).[11]

Notes

[edit]
  1. ^abcCentral Bureau for Astronomical Telegrams, No. 270, 2 November 2005, for (9260) Edwardolson
    A photometric observations between 6 and 30 October 2005, show that9260 Edwardolson is a binary system with an orbital period of17.785±0.003 hours. The primary rotates with a period of3.0852±0.0001 hours, and its lightcurve has a brightness variation of 0.11 magnitude, which is indicative of a nearly spheroidal shape. Mutual eclipse/occultation events, that are between 0.08 and 0.15 magnitude deep, indicate a secondary-to-primary mean-diameter ratio of0.27±0.03.
    Reported by M. Jakubik and M. Husarik, Skalnate Pleso Observatory; J. Vilagi, S. Gajdos, and A. Galad, Modra Observatory; P. Pravec and P. Kusnirak, Ondrejov Observatory; W. Cooney, J. Gross and D. Terrell via Sonoita Research Observatory (Sonoita, AZ); D. Pray, Greene, RI; and R. Stephens, Yucca Valley, CA
    Central Bureau for Astronomical Telegrams

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 9260 Edwardolson (1953 TA1)" (2017-03-31 last obs.).Jet Propulsion Laboratory. Retrieved5 July 2017.
  2. ^abcSchmadel, Lutz D. (2006). "(9260) Edwardolson [2.29, 0.23, 5.1]".Dictionary of Minor Planet Names – (9260) Edwardolson, Addendum to Fifth Edition: 2003–2005.Springer Berlin Heidelberg. p. 44.doi:10.1007/978-3-540-34361-5_334.ISBN 978-3-540-34361-5.
  3. ^abcd"LCDB Data for (9260) Edwardolson". Asteroid Lightcurve Database (LCDB). Retrieved24 July 2016.
  4. ^abJohnston, Robert."(9260) Edwardolson".johnstonsarchive.net. Retrieved1 January 2016.
  5. ^abcdPravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012)."Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026. Retrieved1 January 2016.
  6. ^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. Retrieved24 July 2016.
  7. ^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. Retrieved4 December 2016.
  8. ^abJakubik, M.; Husarik, M.; Vilagi, J.; Gajdos, S.; Galad, A.; Pravec, P.; et al. (November 2005)."(9260) Edwardolson".Central Bureau Electronic Telegrams.270 (270): 1.Bibcode:2005CBET..270....1J. Retrieved1 January 2016.
  9. ^ab"9260 Edwardolson (1953 TA1)".Minor Planet Center. Retrieved24 July 2016.
  10. ^"Edward C. Olson".IAU – International Astronomical Union. Retrieved1 January 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved24 July 2016.

External links

[edit]
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