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5771 Somerville

From Wikipedia, the free encyclopedia
Main-belt asteroid

5771 Somerville
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date21 September 1987
Designations
(5771) Somerville
Named after
Mary Somerville[2]
(Scottishpolymath)
1987 ST1 · 1982 YY1
1989 BG1
main-belt · (outer)[3]
Lixiaohua[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc34.36 yr (12,549 days)
Aphelion3.8347AU
Perihelion2.4381 AU
3.1364 AU
Eccentricity0.2226
5.55yr (2,029 days)
135.29°
0° 10m 38.64s / day
Inclination8.2191°
288.45°
101.58°
Physical characteristics
Dimensions22.84 km(derived)[3]
24.90±6.97 km[5]
26.43±5.87 km[6]
28.306±0.264 km[7]
33.60±2.18 km[8]
9.20±0.05h[9][a]
0.017±0.002[8]
0.029±0.001[7]
0.03±0.03[6]
0.04±0.08[5]
0.0407(derived)[3]
C [3]
12.20[7] · 12.30[1][3][6] · 12.40[8] · 12.50[5] · 12.94±0.26[10]

5771 Somerville, provisional designation1987 ST1, is a carbonaceous Lixiaohuaasteroid from the outer regions of theasteroid belt, approximately 26 kilometers in diameter. It was discovered on 21 September 1987, by American astronomerEdward Bowell at theAnderson Mesa Station of theLowell Observatory in Flagstaff, Arizona.[11] The asteroid was named for Scottish polymathMary Somerville.[2]

Orbit and classification

[edit]

Somerville is a member of theLixiaohua family,[4] an outer-beltasteroid family with more than 700 known members, consisting ofC-type andX-type asteroids. The family's namesake is3556 Lixiaohua.[12]: 23 

The asteroid orbits the Sun in theouter main-belt at a distance of 2.4–3.8 AU once every 5 years and 7 months (2,029 days). Its orbit has aneccentricity of 0.22 and aninclination of 8° with respect to theecliptic.[1]Somerville was first identified as1982 YY1 atPurple Mountain Observatory in December 1982. The body'sobservation arc begins with its official discovery observation at Flagstaff.[11]

Physical characteristics

[edit]

Somerville is an assumedC-type asteroid.[3]

Rotation period

[edit]

In March 2012, a rotationallightcurve ofSomerville was obtained from photometric observations by American astronomerBrian Warner at his Palmer Divide Observatory (716) in Colorado. Lightcurve analysis gave arotation period of 9.20 hours with a brightness amplitude of 0.80magnitude (U=2+).[9][a]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Somerville measures between 24.90 and 33.60 kilometers in diameter and its surface has analbedo between 0.017 and 0.04.[5][6][7][8]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0407 and a diameter of 22.84 kilometers based on anabsolute magnitude of 12.3.[3]

Naming

[edit]

Thisminor planet was named afterMary Somerville (1780–1872; née Fairfax), a Scottishpolymath andscience writer who studied mathematics and astronomy. She is considered to be one of Europe's most distinguished women scientists of her time.[2] The official naming citation was published by theMinor Planet Center on 12 July (M.P.C. 25444).[13]

Notes

[edit]
  1. ^abLightcurve plot of (5771) Somerville, Palmer Divide Observatory,Brian D. Warner (2012), with a period of9.20±0.05 hours and an amplitude (mag) of0.80±0.03.

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 5771 Somerville (1987 ST1)" (2017-04-28 last obs.).Jet Propulsion Laboratory. Retrieved9 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(5771) Somerville".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 488.doi:10.1007/978-3-540-29925-7_5435.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (5771) Somerville". Asteroid Lightcurve Database (LCDB). Retrieved9 September 2017.
  4. ^ab"Asteroid 5771 Somerville – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  5. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  6. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved9 September 2017.
  7. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved9 September 2017.
  8. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  9. ^abWarner, Brian D. (July 2012)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2011 December – 2012 March".The Minor Planet Bulletin.39 (3):158–167.Bibcode:2012MPBu...39..158W.ISSN 1052-8091. Retrieved9 September 2017.
  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. Retrieved9 September 2017.
  11. ^ab"5771 Somerville (1987 ST1)".Minor Planet Center. Retrieved9 September 2017.
  12. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved9 September 2017.

External links

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