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2815 Soma

From Wikipedia, the free encyclopedia
Binary Florian asteroid

2815 Soma
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date15 September 1982
Designations
(2815) Soma
Pronunciation/ˈsmə/[2]
Named after
Soma cube
(mechanical puzzle)[3]
1982 RL · 1955 MH
1970 AC · 1974 DL
1979 XB1
main-belt · Flora[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc61.77 yr (22,562 days)
Aphelion2.6107AU
Perihelion1.8552 AU
2.2329 AU
Eccentricity0.1692
3.34yr (1,219 days)
168.50°
0° 17m 43.44s / day
Inclination5.7042°
119.87°
237.53°
Knownsatellites1[4][5][6]
(Ds/Dp:0.25±0.02)
(orbital period: 17.915 h
)
Physical characteristics
Dimensions6.641±0.105 km[7]
7.067 km[8]
7.07 km(taken)[4]
7.158±0.088 km[9]
2.7327±0.0008h[a]
2.73325±0.00007 h[5]
0.2273[8]
0.3207±0.0411[9]
0.365±0.083[7]
S[4]
12.49±0.06(R)[a] · 12.53±0.02(R)[5] · 12.6[9] · 12.7[1] · 12.92±0.16[10] · 12.98±0.078[4][8]

2815 Soma, provisional designation1982 RL, is abinary Florianasteroid from the inner regions of theasteroid belt, approximately 7 kilometers in diameter. It was discovered on 15 September 1982, by American astronomerEdward Bowell at Lowell'sAnderson Mesa Station in Flagstaff, Arizona, in the United States .[11] It is named for the mechanical puzzleSoma cube.[3]

Orbit and classification

[edit]

Soma is a member of theFlora family, a large family ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,219 days). Its orbit has aneccentricity of 0.17 and aninclination of 6° with respect to theecliptic.[1] It was first identified as1955 MH atGoethe Link Observatory in 1955. The body'sobservation arc begins with1970 AC atCrimea-Nauchnij, 12 years prior to its official discovery at Anderson Mesa.[11]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer (WISE) with its subsequentNEOWISE mission,Soma measures 6.641 and 7.158 kilometers in diameter and its surface has analbedo of 0.365 and 0.3207, respectively.[7][9] TheCollaborative Asteroid Lightcurve Link adopts Peter Pravec's revised WISE-data, that is, an albedo of 0.2273 and a diameter of 7.067 kilometers with anabsolute magnitude of 12.98.[4][8]

Moon and lightcurve

[edit]

Primary

[edit]

In November 2009, a rotationallightcurve ofSoma was obtained from photometric observations by astronomersPetr Pravec,Donald Pray andPeter Kušnirák at Carbuncle Hill Observatory, Rhode Island, andOndřejov Observatory, in the Czech Republic, respectively. Lightcurve analysis gave arotation period of 2.7327 hours with a brightness variation of 0.08magnitude, indicating that the body has a nearly spheroidal shape (U=3-).[a] The body's spin rate is within the 2.2-to-20 hours range found for most asteroids, about half an hour longer than the so-calledfast rotators.

Secondary

[edit]

In March 2011, photometric observations revealed thatSoma is a synchronousbinary asteroid with aminor-planet moon orbiting it every 17.915 hours. The system has a secondary-to-primary mean-diameter ratio of 0.25, which means that satellite's diameter measures approximately 25% of that ofSoma (the primary), and translate into a diameter of 1.75 kilometers.[5] The observations also gave a refined rotation period forSoma of 2.73325 hours and an amplitude of 0.07 magnitude (U=n.a.). The system has an absolute magnitude of 12.53, and aphase slope parameter (G) of 0.27.[5]

Naming

[edit]

Thisminor planet was named for theSoma cube, following a proposal by Belgian astronomerJean Meeus(also see2213 Meeus). The Soma cube a dissection puzzle with seven pieces, invented by the Danish mathematicianPiet Hein and popularized by American writerMartin Gardner(also see2587 Gardner).[3] The approved naming citation was published by theMinor Planet Center on 10 September 1984 (M.P.C. 9080).[12]

Notes

[edit]
  1. ^abcPravec (2009) web:lightcurve plot of (2815) Soma with rotation period2.7327±0.0008 hours and a brightness amplitude of0.08 magnitude. Quality Code of 3-. Summary figures atCollaborative Asteroid Lightcurve Link anddata sheet from theOndrejov Asteroid Photometry Project

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2815 Soma (1982 RL)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Retrieved3 July 2017.
  2. ^"soma".Merriam-Webster.com Dictionary. Merriam-Webster.
  3. ^abcSchmadel, Lutz D. (2007). "(2815) Soma".Dictionary of Minor Planet Names – (2815) Soma.Springer Berlin Heidelberg. p. 231.doi:10.1007/978-3-540-29925-7_2816.ISBN 978-3-540-00238-3.
  4. ^abcdef"LCDB Data for (2815) Soma". Asteroid Lightcurve Database (LCDB). Retrieved23 March 2017.
  5. ^abcdePollock, J.; Pravec, P.; Kusnirak, P.; Hornoch, K.; Chiorny, V.; Gajdos, S.; et al. (April 2011)."(2815) Soma".Central Bureau Electronic Telegrams.2705 (2705): 1.Bibcode:2011CBET.2705....1P. Retrieved23 March 2017.
  6. ^Johnston, Robert (21 September 2014)."(2815) Soma".johnstonsarchive.net. Retrieved23 March 2017.
  7. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved23 March 2017.
  8. ^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. Retrieved23 March 2017.
  9. ^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.
  10. ^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. Retrieved23 March 2017.
  11. ^ab"2815 Soma (1982 RL)".Minor Planet Center. Retrieved23 March 2017.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved23 March 2017.

External links

[edit]
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