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1390 Abastumani

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1390 Abastumani
Shape model ofAbastumani from itslightcurve
Discovery[1]
Discovered byP. Shajn
Discovery siteSimeiz Obs.
Discovery date3 October 1935
Designations
(1390) Abastumani
Named after
Abastumani
(Georgian town)[2]
1935 TA · 1926 GN
1929 UL · A907 GN
A916 VA
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc86.80 yr (31,705 days)
Aphelion3.5547AU
Perihelion3.3166 AU
3.4356 AU
Eccentricity0.0347
6.37yr (2,326 days)
290.65°
0° 9m 17.28s / day
Inclination19.932°
28.919°
332.76°
Physical characteristics
95.849±2.283 km[6]
98.30±2.03 km[7]
101.58±2.3 km(IRAS:12)[8]
107.827±6.977 km[9]
17.100±0.005 h[10]
0.0264±0.0121[9]
0.0298±0.001(IRAS:12)[8]
0.033±0.002[6][7]
9.40[1][7][8][9][11]

1390 Abastumani (prov. designation:1935 TA) is a very large and darkbackground asteroid from the outer region of theasteroid belt. It was discovered on 3 October 1935, by Russian astronomerPelageya Shajn at theSimeiz Observatory on the Crimean peninsula.[3] The primitiveP-type asteroid has arotation period of 17.1 hours and measures approximately 101 kilometers (63 miles) in diameter. It was named for the Georgian town ofAbastumani.[2]

Orbit and classification

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The dark and reddish asteroid is classified as a rareP-type asteroid in theTholen taxonomic scheme, of which only a few dozens bodies are currently known.[12] It orbits the Sun at a distance of 3.3–3.6 AU once every 6 years and 4 months (2,326 days). Its orbit has aneccentricity of 0.03 and aninclination of 20° with respect to theecliptic.[1] The first usedprecovery was taken atLowell Observatory in 1929, extending the asteroid'sobservation arc by 6 years prior to its discovery.[3]

Discovery

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Abastumani was discovered on 3 October 1935, by Soviet–Russian astronomerPelageya Shajn atSimeiz Observatory on the Crimean peninsula.[3] On the same night, the asteroid was independently discovered by South African astronomerCyril Jackson at Johannesburg Observatory.[2] It was one of the last large-sized bodies discovered in the outer belt(also see1269 Rollandia and1902 Shaposhnikov, discovered in 1930 and 1972, respectively).

Naming

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Thisminor planet is named after the spa town ofAbastumani located in theCaucasus Mountains ofGeorgia. It is now the place where the Abastuman Astronomical Observatory (119) is situated.[2] The officialnaming citation was published by theMinor Planet Center in November 1952 (M.P.C. 838).[13]

Physical characteristics

[edit]

In theTholen classification,Abastumani is a primitive, carbonaceousP-type asteroid, a commonspectral type in the outer main-belt and among theJupiter trojan population.[1]

Rotation period

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In April 2002, a rotationallightcurve ofAbastumani was obtained fromphotometric observation by astronomerJohn Gross at the U.S.Sonoran Skies Observatory (G94) in Benson, Arizona. It gave arotation period of17.100±0.005 hours with a brightness variation of 0.15 inmagnitude (U=2).[10]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the asteroid measures between 98.3 and 107.8 kilometers in diameter, and its surface has a very lowalbedo between 0.026 and 0.033.[7][8][9] TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, i.e. a diameter of 101.5 kilometers and an albedo of 0.0298.[11]

References

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  1. ^abcdefg"JPL Small-Body Database Browser: 1390 Abastumani (1935 TA)" (2016-08-15 last obs.).Jet Propulsion Laboratory. Retrieved1 December 2016.
  2. ^abcdSchmadel, Lutz D. (2007). "(1390) Abastumani".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 112.doi:10.1007/978-3-540-29925-7_1391.ISBN 978-3-540-00238-3.
  3. ^abcd"1390 Abastumani (1935 TA)".Minor Planet Center. Retrieved3 August 2016.
  4. ^"Asteroid 1390 Abastumani – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved16 March 2020.
  5. ^"Asteroid 1390 Abastumani".Small Bodies Data Ferret. Retrieved16 March 2020.
  6. ^abMasiero, 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. Retrieved1 December 2016.
  7. ^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)
  8. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  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. Retrieved3 August 2016.
  10. ^abGross, John (September 2003)."Sonoran Skies Observatory lightcurve results for asteroids 1054, 1390, 1813 1838, 2988, 3167, 4448, and 5262"(PDF).Minor Planet Bulletin.30 (3):44–46.Bibcode:2003MPBu...30...44G.ISSN 1052-8091. Retrieved16 March 2020.
  11. ^ab"LCDB Data for (1390) Abastumani". Asteroid Lightcurve Database (LCDB). Retrieved3 August 2016.
  12. ^"JPL Small-Body Database Search Engine: spec. type = P (Tholen)".JPL Solar System Dynamics. Retrieved3 January 2016.
  13. ^Schmadel, Lutz D. "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.

External links

[edit]
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