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2062 Aten

From Wikipedia, the free encyclopedia
Sub-kilometer asteroid

2062 Aten
Orbit ofAten atepoch September 2013
Discovery[1][2]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date7 January 1976
Designations
(2062) Aten
Pronunciation/ˈɑːtən/
Named after
Aten(Egyptian mythology)[3]
1976 AA
Aten · NEO[1][2]
Symbol
Orbital characteristics[1]
Epoch 31 December 2011 (JD 2455926.5)
Uncertainty parameter 0
Observation arc59.14 yr (21,601 days)
Earliestprecovery date17 December 1955
Aphelion1.1434AU
Perihelion0.7901 AU
0.9668 AU
Eccentricity0.1827
0.95yr (347 days)
172.27°
1° 2m 12.48s / day
Inclination18.934°
108.60°
148.04°
Earth MOID0.1131 AU · 44.1LD
Physical characteristics
Dimensions0.73±0.03 km[4]
0.80±0.03 km[5]
0.91 km[6]
1.1 km[7]
1.30 km[8]
40.77h[9]
0.20[8]
0.20±0.15[10]
0.26[7]
0.28[6]
0.39±0.05[4]
0.52±0.10[5]
S(Tholen)[1] · Sr(SMASS)[1]
B–V = 0.930[1]
U–B = 0.460[1]
16.80[1][5] · 17.01±1.40[11] · 17.12[9] · 17.20[12][6] · 17.30[4]

2062 Aten/ˈɑːtən/,[a] provisional designation1976 AA, is a stony sub-kilometerasteroid and namesake of theAten asteroids, a subgroup ofnear-Earth objects. The asteroid was named afterAten fromEgyptian mythology.

It was discovered on 7 January 1976, at thePalomar Observatory by American astronomerEleanor Helin,[2] who was the principal scientist for theNEAT project until her retirement in 2002. TheS-type asteroid measures approximately 900 meters in diameter, has a longer-than averagerotation period of 44.77 hours, and approaches the orbit Earth to 44.1lunar distances.

Orbit and classification

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Aten orbits the Sun at a distance of 0.8–1.1 AU once every 11 months (347 days). Its orbit has aneccentricity of 0.18 and aninclination of 19° with respect to theecliptic.[1] A firstprecovery was taken at the discovering observatory in December 1955, extending the body'sobservation arc by more than 20 years prior to its official discovery observation.[2]

Namesake of the Aten group

[edit]

Aten was the first asteroid found to have asemi-major orbital axis of less than oneastronomical unit and a period of less than one year.[3] A new category of asteroids was thus created, theAtens. As of 2017, the group consists of more than 1,200 numbered members. Other groups of near-Earth objects (NEOs) are theApollo andAmor asteroids, which are both significantly larger than the Atens, while theAtira asteroids form the smallest NEO-group by far.[13]

Close approaches

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The asteroid has an Earthminimum orbit intersection distance of 0.1131 AU (16,900,000 km) which corresponds to 44.1lunar distances.[1]

Physical characteristics

[edit]

In theTholen classification,Aten is a commonS-type asteroid. In theSMASS taxonomy it is classified as an Sr-type, a subtype which transitions to theR-type asteroids.[1]

Lightcurve

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In the 1990s, Italian astronomerStefano Mottola obtained a rotationallightcurve ofAten during the EUNEASO survey atLa Silla, which was a European near-Earth object search and follow-up observation program to determine additional physical parameters. Lightcurve analysis gave a longer-than averagerotation period of 40.77 hours with a brightness variation of 0.26magnitude (U=2).[9] No additional lightcurves have been obtained since.[12]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Aten measures between 700 and 830 meters in diameter and its surface has a highalbedo between 0.39 and 0.52.[4][5]

in 1994,Tom Gehrels published a diameter of 1.1 kilometers and an albedo of 0.26 in his bookHazards Due to Comets and Asteroids.[1][7] The Warm Spitzer NEO survey ("ExploreNEOs") gives a diameter of 1.3 kilometers with an albedo of 0.20.[8]

TheCollaborative Asteroid Lightcurve Link agrees with a revised thermal model for asteroid diameters and albedos, and adopts an albedo of 0.28 with a diameter of 0.91 kilometers based on anabsolute magnitude of 17.2.[6][12] However, theMinor Planet Center (MPC) classifiesAten as a larger (greater than 1 km) object.[2]

Naming

[edit]

Thisminor planet was named fromEgyptian mythology afterAten, the ancientEgyptian god of the solar disk, originally an aspect of the godRa.[3] The officialnaming citation was published by theMinor Planet Center on 1 August 1978 (M.P.C. 4420).[14]

Notes

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  1. ^Oxford English Dictionary

References

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  1. ^abcdefghijkl"JPL Small-Body Database Browser: 2062 Aten (1976 AA)" (2015-02-06 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 25 January 2020. Retrieved3 August 2017.
  2. ^abcde"2062 Aten (1976 AA)".Minor Planet Center. Retrieved3 August 2017.
  3. ^abcSchmadel, Lutz D. (2007). "(2062) Aten".Dictionary of Minor Planet Names – (2062) Aten.Springer Berlin Heidelberg. p. 167.doi:10.1007/978-3-540-29925-7_2063.ISBN 978-3-540-00238-3.
  4. ^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.
  5. ^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.S2CID 9341381.
  6. ^abcdHarris, Alan W. (February 1998). "A Thermal Model for Near-Earth Asteroids".Icarus.131 (2):291–301.Bibcode:1998Icar..131..291H.doi:10.1006/icar.1997.5865.
  7. ^abcTom Gehrels; Mildred Shapley Matthews; A. M. Schumann (1994).Hazards Due to Comets and Asteroids.University of Arizona Press. pp. 540–543.ISBN 978-0-8165-1505-9.
  8. ^abcHarris, A. W.; Mommert, M.; Hora, J. L.; Mueller, M.; Trilling, D. E.; Bhattacharya, B.; et al. (March 2011)."ExploreNEOs. II. The Accuracy of the Warm Spitzer Near-Earth Object Survey"(PDF).The Astronomical Journal.141 (3): 10.Bibcode:2011AJ....141...75H.doi:10.1088/0004-6256/141/3/75.S2CID 14208889.
  9. ^abcMottola, S.; de Angelis, G.; di Martino, M.; Erikson, A.; Harris, A. W.; Hahn, G.; et al. (March 1995). "The EUNEASO Photometric Follow-up Program".Abstracts of the Lunar and Planetary Science Conference.26: 1003.Bibcode:1995LPI....26.1003M.
  10. ^Thomas, C. A.; Trilling, D. E.; Emery, J. P.; Mueller, M.; Hora, J. L.; Benner, L. A. M.; et al. (September 2011)."ExploreNEOs. V. Average Albedo by Taxonomic Complex in the Near-Earth Asteroid Population".The Astronomical Journal.142 (3): 12.Bibcode:2011AJ....142...85T.doi:10.1088/0004-6256/142/3/85.
  11. ^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.S2CID 53493339.
  12. ^abc"LCDB Data for (2062) Aten". Asteroid Lightcurve Database (LCDB). Retrieved3 August 2017.
  13. ^"Discovery Statistics". CNEOS / JPL. Retrieved3 August 2017.
  14. ^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.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.


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