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1005 Arago

From Wikipedia, the free encyclopedia
Asteroid

1005 Arago
Discovery[1]
Discovered byS. Belyavskyj
Discovery siteSimeiz Obs.
Discovery date5 September 1923
Designations
(1005) Arago
Named after
François Arago
(French mathematician)[2]
1923 OT
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc93.51 yr (34,156 days)
Aphelion3.5381AU
Perihelion2.7937 AU
3.1659 AU
Eccentricity0.1176
5.63yr (2,058 days)
206.34°
0° 10m 30s / day
Inclination19.060°
349.17°
60.660°
Physical characteristics
Dimensions48.57±14.27 km[4]
50.28±15.89 km[5]
52.74±0.89 km[6]
56.36±1.36 km[7]
57.69 km(derived)[3]
57.82±4.9 km[8]
61.132±0.345 km[9]
68.404±0.660 km[10]
8.7819±0.0001h[a]
8.784±0.001 h[11]
0.0498±0.0069[10]
0.0582(derived)[3]
0.0697±0.014[8]
0.070±0.008[6]
0.074±0.004[7]
0.08±0.04[4]
0.08±0.09[5]
P[10] · C[3]
9.7[7][8][10] · 9.9[1][3][4][6] · 9.98[5]

Arago (minor planet designation:1005 Arago), provisional designation1923 OT, is a darkasteroid from the outer regions of theasteroid belt, approximately 55 kilometers in diameter. It was discovered on 5 September 1923, by Russian astronomerSergey Belyavsky at theSimeiz Observatory on the Crimean peninsula.[12] The asteroid was named after French mathematicianFrançois Arago.[2]

Classification and orbit

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Arago orbits the Sun in theouter main-belt at a distance of 2.8–3.5 AU once every 5 years and 8 months (2,058 days). Its orbit has aneccentricity of 0.12 and aninclination of 19° with respect to theecliptic.[1] The asteroid'sobservation arc begins atUccle Observatory in 1935, twelve years after its official discovery observation at Simeiz.[12]

Physical characteristics

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Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer (WISE) with its subsequentNEOWISE mission,Arago measures between 48.57 and 68.404 kilometers (30.180 and 42.504 mi) in diameter and its surface has analbedo between 0.0498 and 0.08.[4][5][6][7][8][10] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0582 and a diameter of 57.69 kilometers (35.85 mi) based on anabsolute magnitude of 9.9.[3]

Lightcurve

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In October 2010, a rotationallightcurve ofArago was obtained from photometric observations that was later submitted to the CALL website. Lightcurve analysis gave arotation period of 8.7819 hours with a brightness amplitude of 0.22magnitude (U=n.a.).[a] In April 2016, another lightcurve was obtained by the group of Spanish amateur astronomers OBAS. It gave a concurring period of 8.784 hours with an amplitude of 0.22 magnitude (U=3).[11]

Spectral type

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Arago is characterized by WISE as a dark and reddishP-type asteroid. It is also a carbonaceousC-type asteroid as generically assumed by CALL.[3][10]

Naming

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Thisminor planet was named after French mathematicianFrançois Arago (1786–1853) director of theParis Observatory.[2] He is also honored by aninner ring of Neptune, the craterArago on the Moon and the craterArago on Mars. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 96).[13]

Notes

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  1. ^abCALL (2002): Submitted observations to the CALL website with a rotation period8.7819±0.0001 hours with a brightness amplitude of0.22 mag. Summary figures for (1005) Arago atCollaborative Asteroid Lightcurve Link (CALL)

References

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  1. ^abcd"JPL Small-Body Database Browser: 1005 Arago (1923 OT)" (2017-07-04 last obs.).Jet Propulsion Laboratory. Retrieved6 August 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1005) Arago".Dictionary of Minor Planet Names – (1005) Arago.Springer Berlin Heidelberg. p. 87.doi:10.1007/978-3-540-29925-7_1006.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1005) Arago". Asteroid Lightcurve Database (LCDB). Retrieved6 August 2017.
  4. ^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. Retrieved6 August 2017.
  5. ^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.
  6. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8.S2CID 46350317. Retrieved6 August 2017.
  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.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  9. ^Masiero, 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.S2CID 119293330. Retrieved6 August 2017.
  10. ^abcdefMainzer, 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.S2CID 35447010.
  11. ^abMansego, Enrique Arce; Rodriguez, Pedro Brines; de Haro, Juan Lozano; Chiner, Onofre Rodrigo; Silva, Alvaro Fornas; Porta, David Herrero; et al. (October 2016)."Eighteen Asteroids Lightcurves at Asteroides Observers (OBAS) - MPPD: 2016 March-May".The Minor Planet Bulletin.43 (4):332–336.Bibcode:2016MPBu...43..332M.ISSN 1052-8091. Retrieved6 August 2017.
  12. ^ab"1005 Arago (1923 OT)".Minor Planet Center. Retrieved6 August 2017.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved6 August 2017.

External links

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