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2031 BAM

From Wikipedia, the free encyclopedia
Asteroid

2031 BAM
Orbital diagram ofBAM
Discovery[1]
Discovered byL. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date8 October 1969
Designations
(2031) BAM
Named after
Baikal–Amur Mainline[2]
(Siberian railway line)
1969 TG2 · 1939 VB
1959 TW · 1972 NQ
main-belt · (inner)
Flora[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc77.39 yr (28,268 days)
Aphelion2.6203AU
Perihelion1.8477 AU
2.2340 AU
Eccentricity0.1729
3.34yr (1,220 days)
124.02°
0° 17m 42.72s / day
Inclination4.7524°
169.28°
213.58°
Physical characteristics
Dimensions7.14 km(calculated)[3]
8.14±0.36 km[5]
10.774±0.004h[6]
0.170±0.017[5]
0.24(assumed)[3]
S[3][7]
12.9[1][3] · 13.00[5] · 13.05±0.81[7]

2031 BAM, provisional designation1969 TG2, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter. It was discovered on 8 October 1969, by Soviet astronomerLyudmila Chernykh at theCrimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.[8] The asteroid was named for those who built theBaikal–Amur Mainline (BAM; БАМ), a Siberian railway line.[2]

Orbit and classification

[edit]

BAM is a member of theFlora family (402),[3][4] a giantasteroid family and the largest family of stony asteroids in the main belt.[9]: 23  It orbits the Sun in theinner asteroid belt at a distance of 1.8–2.6 AU once every 3 years and 4 months (1,220 days;semi-major axis of 2.23 AU). Its orbit has aneccentricity of 0.17 and aninclination of 5° with respect to theecliptic.[1]

The body'sobservation arc begins with its identification as1939 VB atUccle Observatory in November 1939, almost 30 years prior to its official discovery observation at Nauchnyj.[8]

Physical characteristics

[edit]

BAM has been characterized as a stonyS-type asteroid byPan-STARRS photometric survey.[7]

Rotation period

[edit]

In October 2016, a rotationallightcurve ofBAM was obtained from photometric observations by amateur astronomer Matthieu Conjat. Lightcurve analysis gave a well-definedrotation period of 10.774 hours with a brightness amplitude of 0.15magnitude (U=3).[6]

Diameter and albedo

[edit]

According to the survey carried out by the JapaneseAkari satellite,BAM measures 8.14 kilometers in diameter and its surface has analbedo of 0.170.[5] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo of 0.24 – derived from8 Flora, the parent body of the Flora family – and calculates a diameter of 7.14 kilometers based on anabsolute magnitude of 12.9.[3]

Naming

[edit]

Thisminor planet was named after those who constructed theBaikal–Amur Mainline (BAM; БАМ) through eastern Russia from 1974 to 1986. The rail line opened in 1989, and runs betweenUst-Kut (nearLake Baikal andKomsomolsk-on-Amur.[2][10] The officialnaming citation was published by theMinor Planet Center on 1 September 1978 (M.P.C. 4482).[11]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2031 BAM (1969 TG2)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved5 December 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2031) Bam".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 164.doi:10.1007/978-3-540-29925-7_2032.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (2031) BAM". Asteroid Lightcurve Database (LCDB). Retrieved5 December 2017.
  4. ^ab"Asteroid 2031 BAM – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^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)
  6. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2031) BAM". Geneva Observatory. Retrieved5 December 2017.
  7. ^abcVeres, 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. Retrieved5 December 2017.
  8. ^ab"2031 BAM (1969 TG2)".Minor Planet Center. Retrieved5 December 2017.
  9. ^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.
  10. ^"BAM". Mark Andrew Holmes' Personal Web Page. Retrieved5 December 2017.
  11. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.


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