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1206 Numerowia

From Wikipedia, the free encyclopedia
Main-belt asteroid

1206 Numerowia
Shape model ofNumerowia from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date18 October 1931
Designations
(1206) Numerowia
Named after
Boris Numerov
(Russian astronomer)[2]
1931 UH · 1974 QE
1974 TY1
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc85.63 yr (31,276 days)
Aphelion3.0180AU
Perihelion2.7123 AU
2.8651 AU
Eccentricity0.0533
4.85yr (1,771 days)
38.115°
0° 12m 11.52s / day
Inclination13.003°
324.44°
277.42°
Physical characteristics
Dimensions14.173±0.092 km[4]
14.534±0.264 km[5]
15.63±1.09 km[6]
27.90 km(calculated)[3]
4.7743±0.0013h[7]
4.77529±0.00001 h[8]
0.057(assumed)[3]
0.141±0.021[6]
0.159±0.026[5]
0.1680±0.0205[4]
C[3]
11.5[1][3] · 11.80[4][6]

1206 Numerowia (provisional designation1931 UH) is anasteroid from the outer region of theasteroid belt, approximately 15 kilometers in diameter. It was discovered by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany on 18 October 1931, and named after Russian astronomerBoris Numerov.[2][9]

Orbit and classification

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Numerowia orbits the Sun in theouter main-belt at a distance of 2.7–3.0 AU once every 4 years and 10 months (1,771 days). Its orbit has aneccentricity of 0.05 and aninclination of 13° with respect to theecliptic.[1] The asteroid'sobservation arc begins at Heidelberg four days after its official discovery observation.[9]

Physical characteristics

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Rotation period and poles

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In February 2006, a rotationallightcurve of Numerowia was obtained from photometric observations by astronomerLawrence Molnar and colleges at theCalvin–Rehoboth Observatory in New Mexico, United States. Lightcurve analysis gave a well-definedrotation period of 4.7743 hours with a high brightness variation of 0.63magnitude (U=3), indicating that the body has a non-spheroidal shape.[7]

A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database (LPD), gave a concurring period of 4.77529 hours (U=n.a.), as well as two spin axis of (64.0°, −50.0°) and (271.0°, −69.0°) inecliptic coordinates (λ, β).[8]

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, Numerowia measures between 14.173 and 15.63 kilometers in diameter and its surface has analbedo between 0.141 and 0.168.[4][5][6]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forC-type asteroid of 0.057 and consequently calculates a larger diameter of 27.90 kilometers using anabsolute magnitude of 11.5.[3]

Naming

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Thisminor planet was named after Russian astronomer and geophysicistBoris Numerov (1891–1941), founder and director of theInstitute for Theoretical Astronomy in Leningrad, who was executed for espionage by the Soviet Union in 1941. The accusation was based on the fact that a German had named the asteroid after him.[2] In 1957, his memory was rehabilitated.[10] The lunar craterNumerov was also named in his honour. The official naming citation was published byPaul Herget inThe Names of the Minor Planets in 1955 (H 112).[2]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1206 Numerowia (1931 UH)" (2017-06-04 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved5 August 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1206) Numerowia".Dictionary of Minor Planet Names – (1206) Numerowia.Springer Berlin Heidelberg. p. 101.doi:10.1007/978-3-540-29925-7_1207.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1206) Numerowia". Asteroid Lightcurve Database (LCDB). Retrieved5 August 2017.
  4. ^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.
  5. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved5 August 2017.
  6. ^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)
  7. ^abMolnar, Lawrence A.; Haegert, Melissa J.; Beaumont, Christopher N.; Block, Marjorie J.; Brom, Timothy H.; Butler, Andrew R.; et al. (January–March 2008)."Lightcurve Analysis of a Magnitude Limited Asteroid Sample".The Minor Planet Bulletin.35 (1):9–12.Bibcode:2008MPBu...35....9M.ISSN 1052-8091. Retrieved5 August 2017.
  8. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved5 August 2017.
  9. ^ab"1206 Numerowia (1931 UH)".Minor Planet Center. Retrieved5 August 2017.
  10. ^"Columbia University Computing History–A Chronology of Computing at Columbia University".Columbia University. 30 January 2017. Retrieved5 August 2017.

External links

[edit]
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