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1451 Granö

From Wikipedia, the free encyclopedia
Main-belt asteroid

1451 Granö
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date22 February 1938
Designations
(1451) Grano
Named after
Johannes Gabriel Granö
(University of Turku)[2]
1938 DT · 1976 WK
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc56.21 yr (20,532 days)
Aphelion2.4619AU
Perihelion1.9442 AU
2.2030 AU
Eccentricity0.1175
3.27yr (1,194 days)
60.928°
0° 18m 5.04s / day
Inclination5.1087°
175.29°
51.858°
Physical characteristics
Dimensions6.170±0.072[4]
6.329±0.037 km[5]
6.81 km(calculated)[3]
9.70±0.57 km[6]
5.109h(removed)[a]
138±0.05 h[7]
0.171±0.022[6]
0.20(assumed)[3]
0.4034±0.0919[5]
0.429±0.077[4]
S[3][8]
12.6[5][6] · 13.2[1][3] · 14.19±0.95[8]

1451 Granö, provisional designation1938 DT, is a stony Florianasteroid andslow rotator from the inner regions of theasteroid belt, approximately 6.5 kilometers in diameter. It was discovered on 22 February 1938, by Finnish astronomerYrjö Väisälä atTurku Observatory in Southwest Finland, and later named forJohannes Gabriel Granö, rector of theUniversity of Turku.[9]

Orbit and classification

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The asteroid is a member of theFlora family, a large group of stonyS-type 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 3 months (1,194 days). Its orbit has aneccentricity of 0.12 and aninclination of 5° with respect to theecliptic.[1] As noprecoveries were taken, and no previous identifications were made,Granö'sobservation arc begins with its official discovery observation in 1938.[9]

Physical characteristics

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Slow rotator

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A rotationallightcurve ofGranö was obtained from photometric observations made by amateur astronomerRobert Stephens at GMARS and Santana Observatories in March 2010. Analysis gave a longrotation period of 138 hours with a brightness variation of 0.65magnitude (U=2+).[7] This makesGranö aslow rotating asteroid. The result supersedes a previous period of 5.1 hours from May 2007 (U=2-).[a]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Granö measures between 6.17 and 9.70 kilometers in diameter, and its surface has analbedo between 0.171 and 0.429.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 6.81 kilometers using anabsolute magnitude of 13.2.[3]

Naming

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Thisminor planet was named afterJohannes Gabriel Granö (1882−1956), Finnish professor of geography and rector atUniversity of Turku from 1932 to 1934.[2] The officialnaming citation was published by theMinor Planet Center on 30 January 1964 (M.P.C. 2277).[10]

Notes

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  1. ^abGeneva Obs. Behrend (2007) web: rotation period5.109±0.004 hours with a brightness amplitude of0.06 mag. Summary figures for (1451) Grano atCollaborative Asteroid Lightcurve Link (CALL). Results are no longer published on website, see:Asteroids and comets rotation curves CdR – Observatoire de Genève, Raoul Behrend

References

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  1. ^abcd"JPL Small-Body Database Browser: 1451 Grano (1938 DT)" (2017-06-03 last obs.).Jet Propulsion Laboratory. Retrieved25 July 2017.
  2. ^abSchmadel, Lutz D. (2007). "(1451) Granö".Dictionary of Minor Planet Names – (1451) Granö.Springer Berlin Heidelberg. p. 116.doi:10.1007/978-3-540-29925-7_1452.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1451) Granö". Asteroid Lightcurve Database (LCDB). Retrieved16 December 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. Retrieved16 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.
  6. ^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)
  7. ^abStephens, Robert D. (October 2010)."Asteroids Observed from GMARS and Santana Observatories: 2010 April - June".The Minor Planet Bulletin.37 (4):159–161.Bibcode:2010MPBu...37..159S.ISSN 1052-8091. Retrieved16 December 2016.
  8. ^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 December 2016.
  9. ^ab"1451 Grano (1938 DT)".Minor Planet Center. Retrieved16 December 2016.
  10. ^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

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Minor planets
Asteroid
Distant minor planet
Comets
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