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1760 Sandra

From Wikipedia, the free encyclopedia
Main-belt asteroid

1760 Sandra
Discovery[1]
Discovered byErnest Johnson
Discovery siteJohannesburg Obs.
Discovery date10 April 1950
Designations
(1760) Sandra
Named after
Sandra(discoverer's granddaughter)[2]
1950 GB · 1934 NP
1935 QH · 1950 HF
1950 JM · 1951 OK
1967 JC · 1968 OC
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc81.66 yr (29,826 days)
Aphelion3.5564AU
Perihelion2.7418 AU
3.1491 AU
Eccentricity0.1293
5.59yr (2,041 days)
6.2435°
0° 10m 35.04s / day
Inclination8.4403°
232.61°
332.93°
Physical characteristics
Dimensions33.989±0.214 km[4]
34.765±0.454 km[5]
35.89±3.5 km[6]
36.03 km(derived)[3]
36.64±1.03 km[7]
37.71±0.64 km[8]
6.5668±0.0004h[9]
0.034±0.002[7]
0.0345±0.008[6]
0.0385±0.0055[4]
0.054±0.011[8]
0.0542(derived)[3]
C[3]
10.90[8] · 11.0[1][3] · 11.23±0.27[10] · 11.5[4][6][7]

1760 Sandra, provisional designation1950 GB, is a carbonaceousasteroid from the outer regions of theasteroid belt, approximately 35 kilometers in diameter. It was discovered on 10 April 1950, by South African astronomerErnest Johnson atUnion Observatory in Johannesburg, and named after his granddaughter Sandra.[2][11]

Orbit and classification

[edit]

Sandra is a carbonaceousC-type asteroid that orbits the Sun in theouter main-belt at a distance of 2.7–3.6 AU once every 5 years and 7 months (2,041 days). Its orbit has aneccentricity of 0.13 and aninclination of 8° with respect to theecliptic.[1] It was first identified as1934 NP at the discovering observatory. The body'sobservation arc begins with its identification as1935 QH atHeidelberg in 1935, or 15 years prior to its official discovery observation at Johannesburg.[11]

Lightcurve

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In April 2006, a rotationallightcurve ofSandra was obtained from photometric observations by French amateur astronomerPierre Antonini. Lightcurve analysis gave a well-definedrotation period of 6.5668 hours with a brightness variation of 0.42magnitude (U=3).[9]

Diameter and albedo

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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,Sandra measures between 33.989 and 37.71 kilometers in diameter and its surface has analbedo between 0.034 and 0.054.[4][5][6][7][8] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0542 and a diameter of 36.03 kilometers with on anabsolute magnitude of 11.0.[3]

Naming

[edit]

Thisminor planet was named by the South African discoverErnest Johnson after his granddaughter Sandra.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3934).[12]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1760 Sandra (1950 GB)" (2017-04-28 last obs.).Jet Propulsion Laboratory. Retrieved1 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1760) Sandra".Dictionary of Minor Planet Names – (1760) Sandra.Springer Berlin Heidelberg. p. 140.doi:10.1007/978-3-540-29925-7_1761.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1760) Sandra". Asteroid Lightcurve Database (LCDB). Retrieved4 April 2017.
  4. ^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.
  5. ^abMasiero, 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. Retrieved4 April 2017.
  6. ^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.
  7. ^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)
  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. Retrieved4 April 2017.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1760) Sandra".Geneva Observatory. Retrieved4 April 2017.
  10. ^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. Retrieved4 April 2017.
  11. ^ab"1760 Sandra (1950 GB)".Minor Planet Center. Retrieved4 April 2017.
  12. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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