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3350 Scobee

From Wikipedia, the free encyclopedia
Main-belt asteroid
3350 Scobee
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date8 August 1980
Designations
(3350) Scobee
Named after
Dick Scobee
(Challenger crew member)[2]
1980 PJ · 1973 SG2
1976 JU10
main-belt[1][3] · Flora[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc64.53 yr (23,568 days)
Aphelion2.7846AU
Perihelion1.8357 AU
2.3102 AU
Eccentricity0.2054
3.51yr (1,283 days)
200.70°
0° 16m 50.52s / day
Inclination3.4096°
353.72°
330.81°
Physical characteristics
Dimensions3.11±0.59 km[5]
3.26 km(calculated)[4]
7.401±0.210 km[6][7]
0.059±0.011[6][7]
0.22±0.08[5]
0.24(assumed)[4]
S[4]
14.3[6] · 14.6[1][4] · 14.81[5] · 15.10±0.25[8]

3350 Scobee, provisional designation1980 PJ, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 3 kilometers in diameter. It was discovered on 8 August 1980 by American astronomerEdward Bowell at Lowell'sAnderson Mesa Station near Flagstaff, Arizona.[3] It was named forDick Scobee, commander of the ill-fatedChallenger crew.

Orbit and classification

[edit]

Scobee is a member of theFlora family, one of the largest families ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 1.8–2.8 AU once every 3 years and 6 months (1,283 days). Its orbit has aneccentricity of 0.21 and aninclination of 3° with respect to theecliptic.[1] A firstprecovery was taken atPalomar Observatory in 1952, extending the body'sobservation arc by 28 years prior to its official discovery observation at Anderson Mesa.[3]

Physical parameters

[edit]

According to preliminary results of the space-based survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Scobee measured 7.401 kilometers in diameter and its surface had a dark, carbonaceousalbedo of 0.059.[6][7] TheCollaborative Asteroid Lightcurve Link, however, assumed an albedo of 0.24 – derived from8 Flora, the largest member and namesake of the family – and calculated a diameter of 3.26 kilometers based on anabsolute magnitude of 14.6.[4] More recent NEOWISE-observations, taken during the second year since the spacecraft was reactivated in late 2013, are in agreement, giving a diameter of 3.11 kilometers and an albedo of 0.22.[5]

Photometric observations gave a respective brightness variation of 0.16 and 0.17magnitude, which indicates that the body has a rather spheroidal shape. As of 2017, however, no rotationallightcurve of Scobee has been obtained and itsrotation period remains unknown.[4][5][9]

Naming

[edit]

Thisminor planet was named in memory of American astronaut and commander of the Challenger Space ShuttleDick Scobee (1939–1986), who died in theSpace Shuttle Challenger disaster on 28 January 1986.[2] The sequentially numbered minor planets3351 Smith,3352 McAuliffe,3353 Jarvis,3354 McNair,3355 Onizuka, and3356 Resnik were named for the other crew members of the ill-fatedSTS-51-L mission. The approved naming citation was published by theMinor Planet Center on 26 March 1986 (M.P.C. 10549).[10]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 3350 Scobee (1980 PJ)" (2017-03-26 last obs.).Jet Propulsion Laboratory. Retrieved3 July 2017.
  2. ^abSchmadel, Lutz D. (2007). "(3350) Scobee".Dictionary of Minor Planet Names – (3350) Scobee.Springer Berlin Heidelberg. p. 279.doi:10.1007/978-3-540-29925-7_3351.ISBN 978-3-540-00238-3.
  3. ^abc"3350 Scobee (1980 PJ)".Minor Planet Center. Retrieved18 March 2017.
  4. ^abcdefg"LCDB Data for (3350) Scobee". Asteroid Lightcurve Database (LCDB). Retrieved18 March 2017.
  5. ^abcdeNugent, 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. ^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.S2CID 35447010.
  7. ^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.S2CID 118745497. Retrieved18 March 2017.
  8. ^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. Retrieved18 March 2017.
  9. ^Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995)."Photoelectric Observations of 125 Asteroids".Abstracts of the Lunar and Planetary Science Conference.26: 1511.Bibcode:1995LPI....26.1511W. Retrieved18 March 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved18 March 2017.

External links

[edit]
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