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2927 Alamosa

From Wikipedia, the free encyclopedia
Main-belt asteroid

2927 Alamosa
Discovery[1]
Discovered byN. G. Thomas
Discovery siteAnderson Mesa Stn.
Discovery date5 October 1981
Designations
(2927) Alamosa
Named after
Alamosa, Colorado[2]
(discoverer's birthplace)
1981 TM · 1936 OA
1975 EN2
main-belt[3] · (middle)[4]
background[5]
Orbital characteristics[3]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc82.26yr (30,044 d)
Aphelion2.9605AU
Perihelion2.1020 AU
2.5312 AU
Eccentricity0.1696
4.03 yr (1,471 d)
162.56°
0° 14m 40.92s / day
Inclination17.022°
150.47°
189.56°
Physical characteristics
11.83 km(calculated)[4]
4.3832 h[6]
0.20(assumed)[4]
S[4][7][8][9]
12.1[1][3]

2927 Alamosa, provisional designation1981 TM, is a stony backgroundasteroid from the central region of theasteroid belt, approximately 12 kilometers (7.5 miles) in diameter. The asteroid was discovered on 5 October 1981, by American astronomerNorman Thomas at Lowell'sAnderson Mesa Station in Flagstaff, Arizona.[1] TheS-type asteroid has arotation period of 4.4 hours.[4] It was named after the U.S. town ofAlamosa in Colorado.[2]

Orbit and classification

[edit]

Alamosa is a non-family asteroid from the main belt'sbackground population. It orbits the Sun in thecentral asteroid belt at a distance of 2.1–3.0 AU once every 4.03 years (1,471 days;semi-major axis of 2.53 AU). Its orbit has aneccentricity of 0.17 and aninclination of 17° with respect to theecliptic.[3] It was first identified as1936 OA atHeidelberg Observatory in 1936, extending the asteroid'sobservation arc by 45 years prior to its official discovery observation at Anderson Mesa.[1]

Naming

[edit]

Thisminor planet was named after the U.S. town ofAlamosa, Colorado, located in the San Luis Valley on the upperRio Grande. The town is the birthplace of the discovering astronomer, Norman Thomas.[2] The official naming citation was published by theMinor Planet Center on 20 December 1983 (M.P.C. 8405).[10] Almosa is Spanish forcottonwood tree.

Physical characteristics

[edit]

Alamosa has been characterized as a commonS-type asteroid byPan-STARRS' survey,[4][7] theSmall Solar System Objects Spectroscopic Survey (S3OS2),[5][9] as well as in theSDSS-based taxonomy.[8] In the SMASS-like variant of the S3OS2 taxonomy,Alamosa is aK-type asteroid.[5][9]

In April and May 2012, a rotationallightcurve was obtained fromphotometric observations made at the Phillips Academy Observatory (I12). Lightcurve analysis gave a well-definedrotation period of4.3832±0.0002 hours with a brightness variation of 0.26 inmagnitude (U=3).[6] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 11.8 kilometers with anabsolute magnitude of 12.0.[4]

References

[edit]
  1. ^abcd"2927 Alamosa (1981 TM)".Minor Planet Center. Retrieved18 November 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(2927) Alamosa".Dictionary of Minor Planet Names – (2927) Alamosa.Springer Berlin Heidelberg. p. 241.doi:10.1007/978-3-540-29925-7_2928.ISBN 978-3-540-00238-3.
  3. ^abcd"JPL Small-Body Database Browser: 2927 Alamosa (1981 TM)" (2018-10-18 last obs.).Jet Propulsion Laboratory. Retrieved18 November 2018.
  4. ^abcdefg"LCDB Data for (2927) Alamosa". Asteroid Lightcurve Database (LCDB). Retrieved18 November 2018.
  5. ^abc"Asteroid 2927 Alamosa".Small Bodies Data Ferret. Retrieved18 November 2018.
  6. ^abOdden, Caroline; French, John; Briggs, John (October 2012)."Lightcurve Analysis for Four Asteroids".The Minor Planet Bulletin.39 (4):236–238.Bibcode:2012MPBu...39..236O.ISSN 1052-8091. Retrieved4 May 2016.
  7. ^abVeres, 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. Retrieved4 May 2016.
  8. ^abCarvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010)."SDSS-based taxonomic classification and orbital distribution of main belt asteroids".Astronomy and Astrophysics.510: 12.Bibcode:2010A&A...510A..43C.doi:10.1051/0004-6361/200913322. Retrieved30 October 2019.(PDS data set)
  9. ^abcLazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004)."S3OS2: the visible spectroscopic survey of 820 asteroids"(PDF).Icarus.172 (1):179–220.Bibcode:2004Icar..172..179L.doi:10.1016/j.icarus.2004.06.006. Retrieved18 November 2018.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved18 November 2018.

External links

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