9963 Sandage

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9963 Sandage
AnimatedOrbitOf9963Sandage.gif
Orbits of Sandage (blue), the inner planets (red) and Jupiter (outermost)
Discovery [1]
Discovered by E. F. Helin
Discovery site Palomar Obs.
Discovery date 9 January 1992
Designations
MPC designation (9963) Sandage
Named after
Allan Sandage
(astronomer)[2]
1992 AN · 1976 NH
1989 CK6
main-belt · Phocaea[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc 27.76 yr (10,139 days)
Aphelion 2.9985 AU
Perihelion 1.6832 AU
2.3409 AU
Eccentricity 0.2809
3.58 yr (1,308 days)
77.520°
0° 16m 30.72s / day
Inclination 23.462°
116.97°
241.15°
Physical characteristics
Dimensions 5.45 km (calculated)[3]
6.371±0.174 km[4][5]
4.6502±0.0008 h[6]
4.65053±0.00013 h[7]
0.158±0.025[4][5]
0.23 (assumed)[3]
S[3]
12.9[1] · 12.95±0.25[8] · 13.080±0.002 (R)[6] · 13.53[3] · 13.6[4]

9963 Sandage, provisional designation 1992 AN, is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter.

It was discovered by American astronomer Eleanor Helin at the U.S. Palomar Observatory in California on 9 January 1992., and later named after American astronomer Allan Sandage.[2][9]

Orbit and classification[edit]

Sandage is a stony S-type asteroid and a member of the Phocaea family, a group of asteroids with similar orbital characteristics. It orbits the Sun in the inner main-belt at a distance of 1.7–3.0 AU once every 3 years and 7 months (1,308 days). Its orbit has an eccentricity of 0.28 and an inclination of 23° with respect to the ecliptic.[1] First identified as 1976 NH at Crimea–Nauchnij in 1976, the body's observation arc begins at the German Karl Schwarzschild Observatory in 1989, or 3 years prior to its official discovery observation at Palomar.[9]

Physical characteristics[edit]

Rotation period[edit]

Two rotational lightcurves of Sandage were obtained from photometric observations at the Palomar Transient Factory and at Texas Tech's Preston Gott Observatory in November 2011 and June 2016, respectively. Lightcurve analysis gave a rotation period of 4.65 hours with a high brightness variation of 0.56 and 0.43 in magnitude, respectively (U=2/3-).[6][7]

Diameter and albedo[edit]

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Sandage measures 6.4 kilometers in diameter and its surface has an albedo of 0.16,[4] while the Collaborative 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 an absolute magnitude of 13.53.[3]

Naming[edit]

This minor planet was named after American astronomer Allan Sandage (1926–2010), a worldwide known expert on stellar astronomy and observational cosmology, who worked at Palomar and Mount Wilson Observatory.[2] Sandage determined the first reasonably accurate values for the Hubble constant and also discovered the first quasar. Naming citation was published on 2 September 2001 (M.P.C. 43381).[10]

References[edit]

  1. ^ a b c d "JPL Small-Body Database Browser: 9963 Sandage (1992 AN)" (2016-11-08 last obs.). Jet Propulsion Laboratory. Retrieved 4 December 2016. 
  2. ^ a b c Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (9963) Sandage. Springer Berlin Heidelberg. p. 715. ISBN 978-3-540-00238-3. Retrieved 1 August 2016. 
  3. ^ a b c d e f "LCDB Data for (9963) Sandage". Asteroid Lightcurve Database (LCDB). Retrieved 1 August 2016. 
  4. ^ a b c d Mainzer, 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:1109.6407Freely accessible. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 1 August 2016. 
  5. ^ a b Masiero, 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:1109.4096Freely accessible. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 4 December 2016. 
  6. ^ a b c Waszczak, 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:1504.04041Freely accessible. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 1 August 2016. 
  7. ^ a b Clark, 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. Retrieved 1 August 2016. 
  8. ^ 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:1506.00762Freely accessible. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 1 August 2016. 
  9. ^ a b "9963 Sandage (1992 AN)". Minor Planet Center. Retrieved 1 August 2016. 
  10. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 1 August 2016. 

External links[edit]