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6084 Bascom

From Wikipedia, the free encyclopedia
Phocaea asteroid from the inner regions of the asteroid belt

6084 Bascom
Discovery[1]
Discovered byC. S. Shoemaker
E. M. Shoemaker
Discovery sitePalomar Obs.
Discovery date12 February 1985
Designations
(6084) Bascom
Named after
Florence Bascom
(American geologist)[2]
1985 CT · 1978 EC6
1992 BM1
main-belt · Phocaea[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc67.22 yr (24,553 days)
Aphelion2.8582AU
Perihelion1.7697 AU
2.3139 AU
Eccentricity0.2352
3.52yr (1,286 days)
163.37°
0° 16m 48s / day
Inclination22.999°
147.24°
258.81°
Knownsatellites1(P: 43.5 h; 0.37 Ds/Dp)[5][a]
Physical characteristics
Dimensions6.17±1.15 km[6]
6.347±0.218 km[7][8]
6.388 km[9]
6.39 km(taken)[3]
2.74516±0.00002 h[10]
2.7454±0.0005h[5]
2.74542 h[3]
2.74544±0.00002 h[b]
0.2091[3][9]
0.220±0.030[7][8]
0.26±0.10[6]
S[3]
12.8±0.1(R)[5] · 12.80±0.03(R)[10] · 12.9[1] · 12.91±0.34[11] · 13.19[6] · 13.25[7] · 13.29±0.058[3][9]

6084 Bascom, provisional designation1985 CT, is abinary[a] Phocaeaasteroid from the inner regions of theasteroid belt, approximately 6.3 kilometers in diameter. It was discovered on 12 February 1985, by American astronomer coupleCarolyn andEugene Shoemaker atPalomar Observatory in California.[12] It is named after American geologistFlorence Bascom.[2] Itssatellite measures approximately 2.3 kilometers (0.37 Ds/Dp) and has an orbital period of 43.51 hours.[5]

Orbit and classification

[edit]

Bascom is a stonyS-type asteroid and member of thePhocaea family (701),[4] a group of asteroids with similar orbital characteristics. It orbits the Sun in theinner main-belt at a distance of 1.8–2.9 AU once every 3 years and 6 months (1,286 days). Its orbit has aneccentricity of 0.24 and aninclination of 23° with respect to theecliptic.[1] A firstprecovery was taken at Palomar in 1950, extending the body'sobservation arc by 30 years prior to its official discovery observation.[12]

Diameter

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Bascom measures 6.17 and 6.347 kilometers in diameter and its surface has analbedo of 0.22 and 0.26, respectively.[6][7][8] TheCollaborative Asteroid Lightcurve Link (CALL) adoptsPetr Pravec's revised WISE-data, that is, an albedo of 0.2091 and a diameter of 6.39 kilometers for anabsolute magnitude of 13.29.[3][9]

Moon and lightcurve

[edit]

Between 29 December 2005 and 2 February 2006, the first ever rotationallightcurve was obtained from photometric observations taken by astronomersDavid Higgins at Hunters Hill Observatory, Australia, by Petr Pravec,Peter Kušnirák, andLenka Šarounová atOndřejov Observatory, Czech Republic, and byŠtefan Gajdoš,Adrián Galád andJozef Világi atModra Observatory, Slovakia.[5][a]

The observations revealed, thatBascom is a synchronousbinary asteroid that has amoon orbiting its primary every 43.5 hours. Mutualasteroid occultation and eclipsing events with amagnitude between 0.12 and 0.18 suggest, that the satellite's diameter is37±2% of that ofBascom (a secondary-to-primary diameter ratio of 0.37), which translates into a mean-diameter of 2.3 kilometers for the minor-planet moon. The photometric observations had an average absolute magnitude of 12.8.[5][a]

SinceBascom's first observation in December 2005, astronomer Peter Pravec has obtained additional lightcurves. They gave a refinedrotation period for the primary of 2.74516 to 2.74544 hours with a brightness variation between 0.14 and 0.23 magnitude (U=3/3/3).[10][b] These observations also confirmed the presence of the satellite giving a concurringorbital period of 43.51 hours.[10] For an asteroid of its size,Bascom has a relatively fast spin rate, but still above those offast rotators. CALL adopts a rotation period of 2.74542 hours.[3]

Naming

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Thisminor planet was named in memory ofFlorence Bascom (1862–1945), the second woman to earn her Ph.D. in geology in the United States. She was also the first woman hired by theUnited States Geological Survey and the first woman elected to the Council of theGeological Society of America. Bascom founded the geology department atBryn Mawr College, Pennsylvania, where she taught the next generation of notable female geologists for 33 years. Expert inpetrography,mineralogy andcrystallography, her research focused ongeomorphology.[2] The approved naming citation was published by theMinor Planet Center on 11 April 1998 (M.P.C. 31610).[13]

Notes

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  1. ^abcdCentral Bureau for Astronomical Telegrams –CBET No. 389
    Photometric observations obtained between 29 December 2005 and 2 February 2006, reveal, that6084 Bascom is a binary system with an orbital period of 43.5 hours. The primary rotates with a period of 2.7454 hours. The lightcurve's amplitude is 0.22 magnitude. Mutual eclipse and occultation events between 0.12 and 0.18 magnitude, suggest a secondary-to-primary mean-diameter ratio of0.37±0.02. The system's mean absolute R magnitude is12.8±0.1.
    Reported by: David Higgins (Hunters Hill Obs., Canberra, Australia), Petr Pravec, Peter Kušnirák, and Lenka Šarounová (Ondřejov Obs., Czech Republic) and Štefan Gajdoš, Adrián Galád and Jozef Világi (Modra Obs., Slovakia)
  2. ^abPravec (2013) web: rotation period2.74544±0.00002 hours with a brightness amplitude of0.23 mag. Summary figures atCollaborative Asteroid Lightcurve Link andOndrejov Asteroid Photometry Project

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 6084 Bascom (1985 CT)" (2017-06-06 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 17 March 2017. Retrieved4 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(6084) Bascom".Dictionary of Minor Planet Names – (6084) Bascom.Springer Berlin Heidelberg. pp. 508–509.doi:10.1007/978-3-540-29925-7_5637.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (6084) Bascom". Asteroid Lightcurve Database (LCDB). Retrieved15 March 2017.
  4. ^ab"Asteroid 6084 Bascom – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  5. ^abcdefHiggins, D.; Pravec, P.; Kusnirak, P.; Sarounova, L.; Gajdos, S.; Galad, A.; et al. (February 2006)."(6084) Bascom".Central Bureau Electronic Telegrams.389 (389): 1.Bibcode:2006CBET..389....1H. Retrieved15 March 2017.
  6. ^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.
  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.S2CID 35447010.
  8. ^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. Retrieved15 March 2017.
  9. ^abcdPravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012)."Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026. Retrieved15 March 2017.
  10. ^abcdPravec, P.; Scheirich, P.; Vokrouhlický, D.; Harris, A. W.; Kusnirák, P.; Hornoch, K.; et al. (March 2012)."Binary asteroid population. 2. Anisotropic distribution of orbit poles of small, inner main-belt binaries".Icarus.218 (1):125–143.Bibcode:2012Icar..218..125P.doi:10.1016/j.icarus.2011.11.026. Retrieved15 March 2017.
  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. Retrieved15 March 2017.
  12. ^ab"6084 Bascom (1985 CT)".Minor Planet Center. Retrieved15 March 2017.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved15 March 2017.

External links

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