Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

2873 Binzel

From Wikipedia, the free encyclopedia
Florian asteroid and binary system

2873 Binzel
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date28 March 1982
Designations
(2873) Binzel
Named after
Richard Binzel
(American astronomer)[2]
1982 FR · 1935 KH
1935 MH · 1938 GA
1959 RA1
main-belt · (inner)
Flora[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc81.27 yr (29,683 days)
Aphelion2.6074AU
Perihelion1.8954 AU
2.2514 AU
Eccentricity0.1581
3.38yr (1,234 days)
112.97°
0° 17m 30.48s / day
Inclination5.9003°
100.97°
168.33°
Knownsatellites1[5]
Physical characteristics
Dimensions6.426±0.471 km[6]
6.48 km(calculated)[3]
7.011±0.063 km[7]
11.560±0.0037h[8]
0.2307±0.0722[7]
0.24(assumed)[3]
0.272±0.060[6]
SMASS = Sq[1] · S[3]
12.660±0.002(R)[8] · 12.99[1][7] · 13.10±0.41[9] · 13.11[3]

2873 Binzel, provisional designation1982 FR, is a stony Florianasteroid andbinary system from the inner regions of theasteroid belt, approximately 6.5 kilometers in diameter. It was discovered on 28 March 1982, by American astronomerEdward Bowell at theAnderson Mesa Station in Flagstaff, Arizona.[10] The asteroid was named after astronomerRichard Binzel.[2] Its 1.6-kilometerminor-planet moon was discovered in 2019.[5]

Orbit and classification

[edit]

Binzel is a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[3][4][11]: 23  It orbits the Sun in theinner main belt at a distance of 1.9–2.6 AU once every 3 years and 5 months (1,234 days). Its orbit has aneccentricity of 0.16 and aninclination of 6° with respect to theecliptic.[1]

The body'sobservation arc begins with its identification as1935 KH at theJohannesburg Observatory in 1935, almost 47 years prior to its official discovery observation at Anderson Mesa.[10]

Physical characteristics

[edit]

In theSMASS classification,Binzel is a Sq-subtype, which transition from the common stonyS-type asteroids to the less commonQ-types.[1]

Rotation period

[edit]

In September 2010, a rotationallightcurve ofBinzel was obtained from photometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 11.560 hours with a brightness variation of 0.14magnitude (U=2).[8]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Binzel measures 6.426 and 7.011 kilometers in diameter and its surface has analbedo of 0.2307 and 0.272, respectively.[6][7]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of the Flora family – and calculates a diameter of 6.48 kilometers based on anabsolute magnitude of 13.11.[3]

Naming

[edit]

Thisminor planet was named after American astronomerRichard Binzel (born 1958) of the University of Texas at Austin. During the 1980s, Binzel has been a prolific photometrist, obtaining a large number of rotationallightcurves of main-belt asteroids. The official naming citation was prepared by Alan W. Harris and published by theMinor Planet Center on 8 November 1984 (M.P.C. 9215).[2][12]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 2873 Binzel (1982 FR)" (2016-08-29 last obs.).Jet Propulsion Laboratory. Retrieved30 August 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2873) Binzel".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 236.doi:10.1007/978-3-540-29925-7_2874.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (2873) Binzel". Asteroid Lightcurve Database (LCDB). Retrieved30 August 2017.
  4. ^ab"Asteroid 2873 Binzel – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abJohnston, Wm. Robert (27 May 2019)."Asteroids with Satellites Database – (2873) Binzel".Johnston's Archive. Retrieved4 June 2019.
  6. ^abcMasiero, 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. Retrieved30 August 2017.
  7. ^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.
  8. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved30 August 2017.
  9. ^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. Retrieved30 August 2017.
  10. ^ab"2873 Binzel (1982 FR)".Minor Planet Center. Retrieved30 August 2017.
  11. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved30 August 2017.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=2873_Binzel&oldid=1293144152"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp