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2537 Gilmore

From Wikipedia, the free encyclopedia
Main-belt asteroid

2537 Gilmore
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date4 September 1951
Designations
(2537) Gilmore
Named after
Alan C. Gilmore
Pamela M. Kilmartin
(New Zealand astronomers)[2]
1951 RL · 1977 QP2
main-belt · Eunomia[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc65.47 yr (23,912 days)
Aphelion3.1130AU
Perihelion2.1988 AU
2.6559 AU
Eccentricity0.1721
4.33yr (1,581 days)
81.217°
0° 13m 39.72s / day
Inclination12.937°
334.99°
18.786°
Physical characteristics
Dimensions6.68 km(calculated)[3]
7.221±0.118 km[4][5]
4.230±0.020h[6]
4.2302±0.0399 h[7]
0.21(assumed)[3]
0.309±0.055[4][5]
S[3]
12.6[4] · 12.650±0.120(R)[6] · 12.7[1] · 12.737±0.002(R)[7] · 13.19[3]

2537 Gilmore, provisional designation1951 RL, is a Eunomiaasteroid from the middle region of theasteroid belt, approximately 7 kilometers in diameter. It was discovered on 4 September 1951, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany.[8] It was named after New Zealand astronomer coupleAlan C. Gilmore andPamela M. Kilmartin

Orbit and classification

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Gilmore is a member of theEunomia family, a large group ofS-type asteroids and the most prominent family in the intermediate main-belt. It orbits the Sun in thecentral main-belt at a distance of 2.2–3.1 AU once every 4 years and 4 months (1,581 days). Its orbit has aneccentricity of 0.17 and aninclination of 13° with respect to theecliptic.[1] As noprecoveries were taken, the body'sobservation arc begins with its official discovery observation at Heidelberg in 1951.[8]

Physical characteristics

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Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Gilmore measures 7.2 kilometers in diameter and its surface has analbedo of 0.309,[4] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.21 and calculates a diameter of 6.7 kilometers with anabsolute magnitude of 13.19.[3]

Rotation period

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From January to February 2014, two rotationallightcurves ofGilmore were obtained from photometric observations at thePalomar Transient Factory, California. The lightcurves gave arotation period of4.230 and4.2302 hours with a brightness variation of 0.34 and 0.35 inmagnitude, respectively (U=2/2).[6][7]

Naming

[edit]

Thisminor planet was named in honor of New Zealand astronomer coupleAlan C. Gilmore and his wife, Pamela (néeKilmartin), two very productive observers of comets and minor planet in the Southern Hemisphere. They research at theMount John University Observatory since 1980, and are members of theRoyal Astronomical Society of New Zealand.[2]

The official naming citation was published by theMinor Planet Center on 24 July 1983 (M.P.C. 8064),[9] based on a proposal by Conrad Bardwell (see1615 Bardwell) andBrian G. Marsden. Pamela Gilmore is also honored by the minor planet3907 Kilmartin.[2]

References

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  1. ^abcd"JPL Small-Body Database Browser: 2537 Gilmore (1951 RL)" (2017-02-21 last obs.).Jet Propulsion Laboratory. Retrieved14 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2537) Gilmore".Dictionary of Minor Planet Names – (2537) Gilmore.Springer Berlin Heidelberg. p. 207.doi:10.1007/978-3-540-29925-7_2538.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2537) Gilmore". Asteroid Lightcurve Database (LCDB). Retrieved12 August 2016.
  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. ^abMasiero, 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. Retrieved6 December 2016.
  6. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27. Retrieved12 August 2016.
  7. ^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. Retrieved12 August 2016.
  8. ^ab"2537 Gilmore (1951 RL)".Minor Planet Center. Retrieved12 August 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved12 August 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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