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2648 Owa

From Wikipedia, the free encyclopedia
Background asteroid from the Flora region of the inner asteroid belt

2648 Owa
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date8 November 1980
Designations
(2648) Owa
Named after
"rock" inHopi[2]
1980 VJ · 1926 VD
1953 TJ
main-belt[1][3] · (inner)
Flora[4] · background[5][6]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc91.29yr (33,345 d)
Aphelion2.6438AU
Perihelion1.8565 AU
2.2502 AU
Eccentricity0.1749
3.38 yr (1,233 d)
12.319°
0° 17m 31.2s / day
Inclination4.7966°
279.91°
131.33°
Physical characteristics
5.40±0.25 km[7]
5.76±0.91 km[8]
5.933±0.160 km[9][10]
6.81 km(calculated)[4]
3.56±0.01 h[11]
3.563±0.002 h[a]
3.563 h[12]
3.5641±0.0001 h[b][c]
3.567±0.002 h[13]
0.24(assumed)[4]
0.38±0.17[8]
0.4174±0.0904[10]
0.459±0.029[7]
S(assumed)[4]
12.7[10] · 12.80[7]
12.88±0.32[14]
12.90[8] · 13.0[3][4]

2648 Owa, provisional designation1980 VJ, is a backgroundasteroid from the Flora region of the innerasteroid belt, approximately 6 kilometers (4 miles) in diameter. It was discovered on 8 November 1980, by American astronomerEdward Bowell at theAnderson Mesa Station near Flagstaff, Arizona, in the United States.[1] The presumablyS-type asteroid has arotation period of 3.56 hours.[4] It was named for the word "rock" in the Native AmericanHopi language.[2]

Orbit and classification

[edit]

Owa is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[5][6] Based on osculating Keplerianorbital elements, the asteroid has also been classified as a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[4]

It orbits the Sun in theinner main-belt at a distance of 1.9–2.6 AU once every 3 years and 5 months (1,233 days;semi-major axis of 2.25 AU). Its orbit has aneccentricity of 0.17 and aninclination of 5° with respect to theecliptic.[3] The asteroid was first observed as1926 VD atHeidelberg Observatory in November 1926. The body'sobservation arc begins atTurku Observatory in October 1953, more than 27 years prior to its official discovery observation at Anderson Mesa.[1]

Physical characteristics

[edit]

Owa is an assumed, stonyS-type asteroid.[4]

Rotation period

[edit]

In 2007, four rotationallightcurves ofOwa were obtained from photometric observations by James W. Brinsfield at Via Capote Observatory (G69),[11] by astronomers at theNational Undergraduate Research Observatory (NURO),[12] as well as byPetr Pravec andPierre Antonini (U=3-/3-/3/3).[13][b] In 2012, another lightcurve was obtained byDavid Higgins (U=3).[a] The consolidated result gave arotation period of 3.5641 hours with a brightness amplitude between 0.20 and 0.35magnitude (U=3).[4][c]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Owa measures between 5.40 and 5.933 kilometers in diameter and its surface has analbedo between 0.38 and 0.459.[7][8][9][10]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the parent body of the Flora family – and calculates a diameter of 6.81 kilometers based on anabsolute magnitude of 13.0.[4]

Naming

[edit]

Thisminor planet was named after theHopi word for "rock". The Hopi are a Native American tribe, who primarily live on theHopi Reservation in northern Arizona. The asteroid's name was suggested by German-American linguistEkkehart Malotki.[2] The official naming citation was published by theMinor Planet Center on 1 December 1982 (M.P.C. 7473).[15]

Notes

[edit]
  1. ^abHiggins (2012) web: rotation period3.563±0.002 hours with a brightness amplitude of0.35±0.02 mag. Quality code of 3. Summary figures at theLCDB
  2. ^abPravec (Oct 2007) web: rotation period3.5641±0.0001 hours with a brightness amplitude of0.23±0.02 mag. Quality Code is 3. Summary figures at theLCDB andPravec, P.; Wolf, M.; Sarounova, L. (2007)
  3. ^abLightcurveplot-A andplot-B of (2648) Owa fromOndrejov data obtained by the NEO Photometric Program and collaborating projects.

References

[edit]
  1. ^abcd"2648 Owa (1980 VJ)".Minor Planet Center. Retrieved6 April 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(2648) Owa".Dictionary of Minor Planet Names – (2648) Owa. Springer Berlin Heidelberg. pp. 216–217.doi:10.1007/978-3-540-29925-7_2649.ISBN 978-3-540-00238-3.
  3. ^abcd"JPL Small-Body Database Browser: 2648 Owa (1980 VJ)" (2018-02-25 last obs.).Jet Propulsion Laboratory. Retrieved6 April 2018.
  4. ^abcdefghij"LCDB Data for (2648) Owa". Asteroid Lightcurve Database (LCDB). Retrieved6 April 2018.
  5. ^ab"Asteroid 2648 Owa – Asteroid Dynamical Families V4.1".Small Bodies Data Ferret. Retrieved29 October 2019.
  6. ^ab"Asteroid 2648 Owa – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  7. ^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.
  8. ^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.
  9. ^abMasiero, 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. Retrieved6 April 2018.
  10. ^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.
  11. ^abBrinsfield, James W. (June 2008)."The Rotation Periods of 531 Zerlina, 1194 Aleta 1352 Wawel, 2005 Hencke, 2648 Owa, and 3509 Sanshui".The Minor Planet Bulletin.35 (2):86–87.Bibcode:2008MPBu...35...86B.ISSN 1052-8091. Retrieved6 April 2018.
  12. ^abJohnson, Thomas; Pech, Katherin; van Schilfgaarde, Ryan; Chase, Matt; Burns, M. Shane (October 2008)."Lightcurve Analysis of 102 Miriam, 1433 Geramtina, and 2648 Owa".The Minor Planet Bulletin.35 (4):151–152.Bibcode:2008MPBu...35..151J.ISSN 1052-8091. Retrieved6 April 2018.
  13. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2648) Owa". Geneva Observatory. Retrieved6 April 2018.
  14. ^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.
  15. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved6 April 2018.

External links

[edit]
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Distant minor planet
Comets
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