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9963 Sandage

From Wikipedia, the free encyclopedia
Asteroid

9963 Sandage
Orbits ofSandage (blue), theinner planets (red) andJupiter (outermost)
Discovery[1]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date9 January 1992
Designations
(9963) Sandage
Named after
Allan Sandage
(American astronomer)[2]
1992 AN · 1976 NH
1989 CK6
main-belt · Phocaea[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc28.13 yr (10,276 days)
Aphelion2.9982AU
Perihelion1.6833 AU
2.3408 AU
Eccentricity0.2809
3.58yr (1,308 days)
132.58°
0° 16m 30.72s / day
Inclination23.461°
116.97°
241.14°
Physical characteristics
Dimensions5.45 km(calculated)[3]
6.371±0.174 km[5][6]
4.6502±0.0008h[7]
4.65053±0.00013 h[8]
0.158±0.025[5][6]
0.23(assumed)[3]
S[3]
12.9[1] · 12.95±0.25[9] · 13.080±0.002(R)[7] · 13.53[3] · 13.6[5]

9963 Sandage, provisional designation1992 AN, is a stony Phocaeaasteroid from the inner regions of theasteroid belt, approximately 6 kilometers in diameter.

It was discovered by American astronomerEleanor Helin at thePalomar Observatory in California on 9 January 1992, and later named after American astronomerAllan Sandage.[2][10]

Orbit and classification

[edit]

Sandage is astony 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 1.7–3.0 AU once every 3 years and 7 months (1,308 days). Its orbit has aneccentricity of 0.28 and aninclination of 23° with respect to theecliptic.[1] First identified as1976 NH atCrimea–Nauchnij in 1976, the body'sobservation arc begins at the GermanKarl Schwarzschild Observatory in 1989, or 3 years prior to its official discovery observation at Palomar.[10]

Physical characteristics

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Rotation period

[edit]

Two rotationallightcurves ofSandage were obtained from photometric observations at thePalomar Transient Factory and atTexas Tech's Preston Gott Observatory in November 2011 and June 2016, respectively. Lightcurve analysis gave arotation period of 4.65 hours with a high brightness variation of 0.56 and 0.43 inmagnitude, respectively (U=2/3-).[7][8]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Sandage measures 6.4 kilometers in diameter and its surface has analbedo of 0.16,[5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.23 – derived from the family's largest member and namesake,25 Phocaea – and calculates a diameter of 5.5 kilometers with anabsolute magnitude of 13.53.[3]

Naming

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Thisminor planet was named after American astronomerAllan Sandage (1926–2010), a worldwide known expert onstellar astronomy andobservational cosmology, who worked at Palomar andMount Wilson Observatory.[2] Sandage determined the first reasonably accurate values for theHubble constant and also discovered the firstquasar. The official naming citation was published by theMinor Planet Center on 2 September 2001 (M.P.C. 43381).[11]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 9963 Sandage (1992 AN)" (2017-03-25 last obs.).Jet Propulsion Laboratory. Retrieved22 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(9963) Sandage".Dictionary of Minor Planet Names – (9963) Sandage.Springer Berlin Heidelberg. p. 715.doi:10.1007/978-3-540-29925-7_7773.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (9963) Sandage". Asteroid Lightcurve Database (LCDB). Retrieved1 August 2016.
  4. ^ab"Asteroid 9963 Sandage – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  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. Retrieved1 August 2016.
  6. ^abMasiero, 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. Retrieved4 December 2016.
  7. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved1 August 2016.
  8. ^abClark, Maurice (January 2016)."Asteroid Photometry from the Preston Gott Observatory".The Minor Planet Bulletin.43 (1):2–5.Bibcode:2016MPBu...43....2C.ISSN 1052-8091. Retrieved1 August 2016.
  9. ^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 August 2016.
  10. ^ab"9963 Sandage (1992 AN)".Minor Planet Center. Retrieved1 August 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved1 August 2016.

External links

[edit]
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