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5040 Rabinowitz

From Wikipedia, the free encyclopedia
Main-belt asteroid

5040 Rabinowitz
Discovery[1]
Discovered byT. Gehrels
Discovery sitePalomar Obs.
Discovery date15 September 1972
Designations
(5040) Rabinowitz
Named after
David Rabinowitz
(American astronomer)[2]
1972 RF · 1987 QE
main-belt · Phocaea[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc46.20 yr (16,874 days)
Aphelion2.9644AU
Perihelion1.8705 AU
2.4174 AU
Eccentricity0.2263
3.76yr (1,373 days)
7.0892°
0° 15m 43.92s / day
Inclination24.361°
175.69°
149.71°
Physical characteristics
Dimensions6.41 km(calculated)[3]
4.472±0.001h[5]
4.6901±0.0004 h[a]
4.691±0.001 h[6]
0.23(assumed)[3]
S[3]
12.73±0.13(R)[a] · 12.9[1] · 13.15±0.35[7] · 13.18[3]

5040 Rabinowitz, provisional designation1972 RF, is a stony Phocaeaasteroid from the inner regions of theasteroid belt, approximately 6 kilometers in diameter. It was discovered by Dutch–American astronomerTom Gehrels atPalomar Observatory on 15 September 1972.[8] Contrary to most of his discoveries, this asteroid is unrelated to thePalomar–Leiden survey and exclusively credited to Tom Gehrels.

Orbit and classification

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The stonyS-type asteroid is a member of thePhocaea family (701), a group of asteroids with similar orbital characteristics, named after its largest member,25 Phocaea.[4] It orbits the Sun in theinner main-belt at a distance of 1.9–3.0 AU once every 3 years and 9 months (1,373 days). Its orbit has aneccentricity of 0.23 and aninclination of 24° with respect to theecliptic.[1] A firstprecovery was taken at the discovering observatory in 1971, extending the body'sobservation arc by one year prior to its official discovery observation.[8]

Physical characteristics

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Rotation period

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In July 2013, a rotationallightcurve for this asteroid was obtained from photometric observations by Czech astronomerPetr Pravec at theOndřejov Observatory. The well-defined lightcurve gave arotation period of4.6901±0.0004 hours with a brightness variation of 0.33 inmagnitude (U=3).[a]

During the same opposition opportunity, two more lightcurves – obtained byRobert Stephens at the Center for Solar System Studies and by Maurice Clark at the Preston Gott Observatory – gave a similar period of4.691 and4.472 hours, with an amplitude of 0.35 and 0.31 in magnitude, respectively (U=3-/2+).[5][6]

Diameter and albedo

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TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.23, derived from the Phocaea family's namesake, and calculates a diameter of 6.4 kilometers with anabsolute magnitude of 13.18.[3]

Naming

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Thisminor planet was named after American astronomerDavid Rabinowitz (born 1960), adiscoverer of minor planets himself and researcher atYale University. The naming also honors his work for theSpacewatch program.[2] The official naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22505).[9]

Notes

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  1. ^abcPravec (2013):lightcurve plot of (5040) Rabinowitz with a rotation period4.6901±0.0004 hours with a brightness amplitude of0.33 mag and an abs. magnitude of 12.73. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) andPravec, P.; Wolf, M.; Sarounova, L. (2013)

References

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  1. ^abcd"JPL Small-Body Database Browser: 5040 Rabinowitz (1972 RF)" (2017-06-04 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(5040) Rabinowitz".Dictionary of Minor Planet Names – (5040) Rabinowitz.Springer Berlin Heidelberg. p. 434.doi:10.1007/978-3-540-29925-7_4907.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (5040) Rabinowitz". Asteroid Lightcurve Database (LCDB). Retrieved1 July 2016.
  4. ^ab"Asteroid 5040 Rabinowitz – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  5. ^abClark, Maurice (April 2014)."Asteroid Photometry from the Preston Gott Observatory".The Minor Planet Bulletin.41 (2):100–101.Bibcode:2014MPBu...41..100C.ISSN 1052-8091. Retrieved1 July 2016.
  6. ^abStephens, Robert D.; Coley, Daniel R. (October 2013)."A Plethora of Phocaea Asteroids".The Minor Planet Bulletin.40 (4):203–204.Bibcode:2013MPBu...40..203S.ISSN 1052-8091. Retrieved1 July 2016.
  7. ^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. Retrieved1 July 2016.
  8. ^ab"5040 Rabinowitz (1972 RF)".Minor Planet Center. Retrieved1 July 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved1 July 2016.

External links

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