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2829 Bobhope

From Wikipedia, the free encyclopedia
Dark asteroid of the Meliboea family

2829 Bobhope
Shape model ofBobhope from itslightcurve
Discovery[1]
Discovered byE. L. Johnson
Discovery siteJohannesburg Obs.
Discovery date9 August 1948
Designations
(2829) Bobhope
Named after
Bob Hope
(American actor; comedian)[2]
1948 PK · 1942 JH
1952 DU2 · 1952 HR
1959 RV · 1972 YZ
main-belt · (outer)[3]
Meliboea[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc68.64 yr (25,070 days)
Aphelion3.6742AU
Perihelion2.5074 AU
3.0908 AU
Eccentricity0.1888
5.43yr (1,985 days)
272.56°
0° 10m 53.04s / day
Inclination14.301°
324.06°
339.21°
Physical characteristics
32.14±9.31 km[5]
36.29±12.47 km[6]
38.25±2.4 km[7]
40.89±0.87 km[8]
40.98±0.54 km[9]
41.361±0.224 km[10]
44.804±0.511 km[11]
5.013±0.003 h[12]
6.0888±0.0007 h[13]
0.05±0.03[6]
0.055±0.010[10][8]
0.06±0.05[5]
0.0668±0.0182[11]
0.080±0.003[9]
0.0916±0.013[7]
C[3]
10.3[7][9][11] · 10.70[5][8] · 10.8[1][3] · 10.95±0.48[14] · 11.12[6]

2829 Bobhope (prov. designation:1948 PK) is a darkasteroid of theMeliboea family, from the outer region of theasteroid belt. It was discovered on 9 August 1948, by South African astronomerErnest Leonard Johnson atUnion Observatory in Johannesburg.[15] The asteroid was later named after comedianBob Hope.[2] The asteroid has arotation period of 6.1 hours and measures approximately 37 kilometers (23 miles) in diameter.

Orbit and classification

[edit]

Bobhope is a member of theMeliboea family,[4] a smallerasteroid family of carbonaceous outer-belt asteroids with a few hundred members, named after137 Meliboea.[16]: 23  It orbits the Sun in theouter main-belt at a distance of 2.5–3.7 AU once every 5 years and 5 months (1,985 days). Its orbit has aneccentricity of 0.19 and aninclination of 14° with respect to theecliptic.[1] It was first observed as1942 JH at the discovering observatory in May 1942, yet the astrometric data from this observation remained unused to extend itsobservation arc prior to the official discovery date.[15]

Naming

[edit]

Thisminor planet was named for English-born, American comedianBob Hope (1903–2003), star of innumerable feature film, theater, TV and radio productions, and known for the horror comedyCat and the Canary (1939).[2] He hosted theAcademy Awards more than any other host, and received several Honorary and Special Oscars himself. Hope also received more than forty honorary doctorates.[2] Thenaming was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22496).[17]

Physical characteristics

[edit]

Bobhope has been characterized as a carbonaceousC-type asteroid,[3] which agrees with the overallspectral type of the Meliboea family.[16]: 23 

Rotation period

[edit]

A rotationallightcurve ofBobhope was obtained fromphotometric observations by astronomer Landy Carbo at Oakley Southern Sky Observatory (E09), Australia, and at the U.S.Oakley Observatory in September 2008. It gave it arotation period of5.013±0.003 hours with a brightness variation of0.46±0.08magnitude (U=2).[12] A previously published lightcurve by French amateur astronomerBernard Christophe gave a somewhat longer period of6.0888±0.0007 hours with an amplitude of 0.50 (U=2).[13]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Bobhope measures between 32.14 and 40.98 kilometers in diameter and its surface has analbedo between 0.05 and 0.0916.[5][6][7][8][9] More dated NEOWISE publications gave a larger diameter of 41.361 and 44.8 kilometers, respectively.[10][11] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0586 and a diameter of 38.0 kilometers with anabsolute magnitude of 10.8.[3]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2829 Bobhope (1948 PK)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Retrieved14 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(2829) Bobhope".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 232.doi:10.1007/978-3-540-29925-7_2830.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (2829) Bobhope". Asteroid Lightcurve Database (LCDB). Retrieved27 October 2016.
  4. ^ab"Asteroid 2829 Bobhope – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^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. Retrieved14 June 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. ^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.
  8. ^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. Retrieved27 October 2016.
  9. ^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)
  10. ^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. Retrieved27 October 2016.
  11. ^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.
  12. ^abCarbo, Landy; Kragh, Katherine; Krotz, Jonathan; Meiers, Andrew; Shaffer, Nelson; Torno, Steven; et al. (July 2009)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory and Oakley Observatory: 2008 September and October"(PDF).Minor Planet Bulletin.36 (3):91–94.Bibcode:2009MPBu...36...91C.ISSN 1052-8091. Archived fromthe original(PDF) on 26 November 2021. Retrieved18 March 2020.
  13. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2829) Bobhope".Geneva Observatory. Retrieved14 June 2017.
  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. Retrieved27 October 2016.
  15. ^ab"2829 Bobhope (1948 PK)".Minor Planet Center. Retrieved27 October 2016.
  16. ^abNesvorný, 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.
  17. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved27 October 2016.

External links

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