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6181 Bobweber

From Wikipedia, the free encyclopedia
Main-belt asteroid
6181 Bobweber
Discovery[1]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date6 September 1986
Designations
(6181) Bobweber
Named after
Robert Weber
(astronomer)[2]
1986 RW · 1979 YU8
1990 WL2
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc62.59 yr (22,860 days)
Aphelion3.0105AU
Perihelion1.8500 AU
2.4302 AU
Eccentricity0.2388
3.79yr (1,384 days)
30.628°
0° 15m 36.72s / day
Inclination7.5690°
303.65°
93.589°
Physical characteristics
Dimensions4.458±0.056 km[4]
4.488±0.046 km[5]
5.66 km(calculated)[3]
2.7576±0.0001h[6]
2.75796±0.00003 h[a]
0.20(assumed)[3]
0.4210±0.0447[5]
0.425±0.038[4]
S[3]
13.3[5] · 13.6[1][3]

6181 Bobweber, provisional designation1986 RW, is a stonyasteroid from the inner regions of theasteroid belt, approximately 5 kilometers in diameter. It was discovered on 6 September 1986, by American astronomerEleanor Helin at the U.S.Palomar Observatory in California, and named after astronomerRobert Weber.[2]

Orbit and classification

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TheS-type asteroid orbits the Sun in theinner main-belt at a distance of 1.9–3.0 AU once every 3 years and 9 months (1,384 days). Its orbit has aneccentricity of 0.24 and aninclination of 8° with respect to theecliptic.[1] The firstprecovery was taken at the discovering observatory in 1954, which extended the asteroid'sobservation arc by 32 years prior to its discovery observation.[2]

Physical characteristics

[edit]

Rotation period

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A rotationallightcurve ofBobweber was obtained from photometric observations by Czech astronomerPetr Pravec atOndřejov Observatory in December 2009. It gave a well-definedrotation period of2.75796±0.00003 hours with a brightness variation of 0.12 inmagnitude (U=3).[a] In January 2014, astronomer Julian Oey at the Australian Blue Mountains Observatory (Q68) obtained a nearly identical period of2.7576±0.0001 hours with an amplitude of 0.15 magnitude (U=3-).[6]

Diameter and albedo

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According to the surveys carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Bobweber measures 4.5 kilometers in diameter and its surface has a highalbedo of 0.42 and 0.43, respectively,[4][5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 5.7 kilometers.[3]

Naming

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Thisminor planet was named in memory ofRobert Weber (1926–2008), physicist anddiscoverer of minor planets atMIT Lincoln Laboratory, developer of theDeep Space Satellite Tracking Network. He also co-developed and was credited with the first discoveries made by theLincoln Near-Earth Asteroid Research (LINEAR) atLincoln Laboratory's Experimental Test Site at White Sands Missile Range in Socorro, New Mexico. The approved naming citation was published by theMinor Planet Center on 21 March 2008 (M.P.C. 62353).[2][7]

Notes

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  1. ^abPravec (2009):lightcurve plot of (6181) Bobweber, with a rotation period2.75796±0.00003 hours and a brightness amplitude of0.12 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) andPravec, P.; Wolf, M.; Sarounova, L. (2009)

References

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  1. ^abcd"JPL Small-Body Database Browser: 6181 Bobweber (1986 RW)" (2016-10-28 last obs.).Jet Propulsion Laboratory. Retrieved4 July 2017.
  2. ^abcd"6181 Bobweber (1986 RW)".Minor Planet Center. Retrieved26 September 2016.
  3. ^abcdef"LCDB Data for (6181) Bobweber". Asteroid Lightcurve Database (LCDB). Retrieved26 September 2016.
  4. ^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.
  5. ^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.
  6. ^abOey, Julian (January 2016). "Lightcurve Analysis of Asteroids from Blue Mountains Observatory in 2014".The Minor Planet Bulletin.43 (1):45–51.Bibcode:2016MPBu...43...45O.ISSN 1052-8091.
  7. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved26 September 2016.

External links

[edit]
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