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1955 McMath

From Wikipedia, the free encyclopedia
Main-belt asteroid

1955 McMath
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date22 September 1963
Designations
(1955) McMath
Named after
Robert McMath
(astronomer, engineer)[2]
1963 SR · 1936 BA
1949 XN · 1951 EP2
1953 RN · 1963 TK
main-belt · Koronis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc67.17 yr (24,535 days)
Aphelion3.0388AU
Perihelion2.6703 AU
2.8545 AU
Eccentricity0.0645
4.82yr (1,762 days)
32.257°
0° 12m 15.84s / day
Inclination1.0053°
258.11°
154.10°
Physical characteristics
Dimensions9.759±0.248 km[4][5]
10.31 km(calculated)[3]
5.547±0.0315h[6]
5.57±0.00 h[7]
5.574±0.002 h[8]
5.5976±0.0315 h[6]
0.24(assumed)[3]
0.322±0.041[4][5]
S[3]
11.78±0.045(R)[8] · 11.9[4] · 11.97±0.15(R)[7] · 12.003±0.002(R)[6] · 12.1[1][3] · 12.42±0.53[9] · 12.498±0.003(S)[6]

1955 McMath, provisional designation1963 SR, is a stony Koronisasteroid from the outer region of theasteroid belt, approximately 10 kilometers in diameter.

It was discovered on 22 September 1963, by Indiana University'sIndiana Asteroid Program at itsGoethe Link Observatory near Brooklyn, Indiana, United States.[10] It was later named after solar astronomerRobert Raynolds McMath.[2]

Orbit and classification

[edit]

McMath is a stonyS-type asteroid and a member of theKoronis family, which is named after158 Koronis and consists of about 300 known bodies. It orbits the Sun in theouter main-belt at a distance of 2.7–3.0 AU once every 4 years and 10 months (1,762 days). Its orbit has aneccentricity of 0.06 and aninclination of 1° with respect to theecliptic.[1] The firstprecovery was taken atGoethe Link Observatory in 1949, extending the asteroid'sobservation arc by 15 years prior to its discovery. The first (unused) observation atUccle Observatory dates back to 1936.[10]

Physical characteristics

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Rotation period

[edit]

It has a well determinedrotation period of5.574±0.002 hours with a brightness amplitude of 0.30 inmagnitude (U=3).[8] Between 2011 and 2013, three additionallightcurves with concurring periods ofMcMath with an amplitude between 0.32 and 0.39 magnitude were obtained through photometric observations in the R- and S-band at the U.S.Palomar Transient Factory in California (U=2/3-/2).[7][6]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,McMath measures 9.8 kilometers in diameter and its surface has a highalbedo of 0.32,[4] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo forstony members of the Koronis family of 0.24, and calculates a diameter of 10.3 kilometers.[3]

Naming

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Thisminor planet was named after American solar astronomerRobert Raynolds McMath (1891–1962), who was also a bridge engineer and businessman. He was a co-donor and the director of theMcMath–Hulbert Observatory in Lake Angelus, Michigan, which was deeded to the University of Michigan. Under his advice, theNSF chose the site atKitt Peak National Observatory for theMcMath–Pierce Solar Telescope.

From the late 1950s, Robert McMath served as the first president ofAssociation of Universities for Research in Astronomy and thereafter as its chairman. The lunar craterMcMath is also named in his and his father's honour.[2] The approved naming citation was published by theMinor Planet Center on 1 March 1981 (M.P.C. 5848).[11]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1955 McMath (1963 SR)" (2017-02-15 last obs.).Jet Propulsion Laboratory. Retrieved2 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1955) McMath".Dictionary of Minor Planet Names – (1955) McMath.Springer Berlin Heidelberg. p. 157.doi:10.1007/978-3-540-29925-7_1956.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1955) McMath". Asteroid Lightcurve Database (LCDB). Retrieved21 April 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. Retrieved21 April 2016.
  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. Retrieved8 December 2016.
  6. ^abcdeWaszczak, 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. Retrieved18 May 2016.
  7. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (June 2014)."313 New Asteroid Rotation Periods from Palomar Transient Factory Observations".The Astrophysical Journal.788 (1): 21.arXiv:1405.1144.Bibcode:2014ApJ...788...17C.doi:10.1088/0004-637X/788/1/17. Retrieved18 May 2016.
  8. ^abcSlivan, Stephen M.; Binzel, Richard P.; Boroumand, Shaida C.; Pan, Margaret W.; Simpson, Christine M.; Tanabe, James T.; et al. (May 2008)."Rotation rates in the Koronis family, complete to H≈11.2".Icarus.195 (1):226–276.Bibcode:2008Icar..195..226S.doi:10.1016/j.icarus.2007.11.019. Retrieved21 April 2016.
  9. ^Veres, 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. Retrieved18 May 2016.
  10. ^ab"1955 McMath (1963 SR)".Minor Planet Center. Retrieved21 April 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved18 May 2016.

External links

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