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1823 Gliese

From Wikipedia, the free encyclopedia
Main-belt asteroid

1823 Gliese
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date4 September 1951
Designations
(1823) Gliese
Named after
Wilhelm Gliese
(German astronomer)[2]
1951 RD · 1944 MC
1948 VH · 1950 BL
1950 DR · 1950 EF
1954 NE · 1970 EU2
1971 SE1
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc68.36 yr (24,967 days)
Aphelion2.5268AU
Perihelion1.9244 AU
2.2256 AU
Eccentricity0.1353
3.32yr (1,213 days)
37.708°
0° 17m 48.48s / day
Inclination2.8919°
310.01°
296.68°
Physical characteristics
Dimensions8.19 km(calculated)[3]
8.439±0.324[4]
9.544±0.025 km[5]
4.4864±0.0006h[a]
4.488±0.003 h[6]
0.1349±0.0152[5]
0.189±0.046[4]
0.24(assumed)[3]
S[3][7]
12.55±0.49[7] · 12.6[1][3] · 12.9[5]

1823 Gliese, provisional designation1951 RD, is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter. It was discovered on 4 September 1951, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany.[8] The asteroid was named after German astronomerWilhelm Gliese.[2]

Orbit and classification

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TheS-type asteroid is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 1.9–2.5 AU once every 3 years and 4 months (1,213 days). Its orbit has aneccentricity of 0.14 and aninclination of 3° with respect to theecliptic.[1] The first unused observations date back to 1944 atJohannesburg Observatory, when it was identified as1944 MC. The first usedprecovery was taken at the discovering Heidelberg observatory in 1950, extending the asteroid'sobservation arc by one year prior to its official discovery.[8]

Physical characteristics

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Rotation period

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A rotationallightcurve of this asteroid was obtained from photometric observations made by Czech astronomerPetr Pravec at theOndřejov Observatory in August 2014. The lightcurve gave a well-definedrotation period of4.4864±0.0006 hours with a brightness variation of 0.27 inmagnitude (U=3).[a] One month later, in September 2014, a second lightcurve by American astronomerBrian Warner at his Palmer Divide Observatory, Colorado, gave a concurring period of4.488±0.003 hours with an amplitude of 0.23 in magnitude (U=3).[6]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer, the asteroid measures 8.4 and 9.5 kilometers in diameter and its surface has analbedo of 0.189 and 0.135, respectively,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of this asteroid's orbital family – and calculates a diameter of 8.2 kilometers with anabsolute magnitude of 12.6.[3]

Naming

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Thisminor planet was named after German astronomerWilhelm Gliese (1915–1993) at theAstronomisches Rechen-Institut. Gliese is widely known for having compiled about 1,000 stars located within 25 parsecs of Earth into theGliese Catalogue of Nearby Stars.[2] The officialnaming citation was published by theMinor Planet Center on 18 April 1977 (M.P.C. 4156).[9] Alarge number of Exoplanets derive their names form this star catalogue.

Notes

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  1. ^abPravec, P.; Wolf, M.; Sarounova, L. (2014)web publication. Summary figures listed at theLight Curve Data Base – (1823) Gliese

References

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  1. ^abcd"JPL Small-Body Database Browser: 1823 Gliese (1951 RD)" (2017-03-15 last obs.).Jet Propulsion Laboratory. Retrieved8 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1823) Gliese".Dictionary of Minor Planet Names – (1823) Gliese.Springer Berlin Heidelberg. p. 146.doi:10.1007/978-3-540-29925-7_1824.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1823) Gliese". Asteroid Lightcurve Database (LCDB). Retrieved16 May 2016.
  4. ^abcMasiero, 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. Retrieved8 December 2016.
  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. Retrieved16 May 2016.
  6. ^abWarner, Brian D. (January 2015)."Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2014 June-October".The Minor Planet Bulletin.42 (1):54–60.Bibcode:2015MPBu...42...54W.ISSN 1052-8091. Retrieved4 November 2015.
  7. ^abVeres, 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. Retrieved16 May 2016.
  8. ^ab"1823 Gliese (1951 RD)".Minor Planet Center. Retrieved16 May 2016.
  9. ^Schmadel, Lutz D. (2009). "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

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Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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