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1365 Henyey

From Wikipedia, the free encyclopedia
Main-belt asteroid

1365 Henyey
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date9 September 1928
Designations
(1365) Henyey
Named after
Louis Henyey
(American astronomer)[2]
1928 RK · 1932 WL
1941 ME · 1973 YG4
1984 BA · A907 GK
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc109.96 yr (40,164 days)
Aphelion2.5248AU
Perihelion1.9723 AU
2.2486 AU
Eccentricity0.1229
3.37yr (1,232 days)
238.80°
0° 17m 32.28s / day
Inclination5.0758°
258.55°
337.32°
Physical characteristics
Dimensions10.31±1.91 km[4]
10.958±0.369 km[5]
11.31 km(calculated)[3]
18.986±0.002h[6]
32.2±0.2 h[7]
0.24(assumed)[3]
0.26±0.13[4]
0.280±0.041[5]
S[3]
11.80[5] · 11.9[1][3] · 12.01±0.26[8] · 12.10[4]

1365 Henyey, provisional designation1928 RK, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 11 kilometers in diameter. It was discovered by German astronomerMax Wolf atHeidelberg Observatory in southern Germany on 9 September 1928, and named for American astronomerLouis Henyey.[2][9]

Orbit and classification

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Henyey is a member of theFlora family, a large population of stonyS-type asteroids in the inner main-belt. It orbits the Sun in theinner main-belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,232 days). Its orbit has aneccentricity of 0.12 and aninclination of 5° with respect to theecliptic.[1] It was first Identified asA907 GK at Heidelberg in 1907. The body'sobservation arc begins with its official discovery observation in 1928.[9]

Physical characteristics

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Rotation period

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In August 2012, a first rotationallightcurve ofHenyey was obtained from photometric observations by Daniel Klinglesmith at Etscorn Campus Observatory (719) in New Mexico. It gave arotation period of 18.986 hours with a brightness variation of 0.23magnitude (U=2).[6] In November 2016, a divergent period solution of 32.2 hours with a change in brightness of 0.32 magnitude was found by French amateur astronomerRené Roy (U=2).[7]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Henyey measures 10.31 and 10.96 kilometers in diameter and its surface has analbedo of 0.26 and 0.28. respectively.[4][5] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of the family – and calculates a diameter of 11.31 kilometers with anabsolute magnitude of 11.9.[3]

Naming

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Based on a suggestion by William Westbrooke, thisminor planet was named after American astronomerLouis Henyey (1910–1970), known for his contributions in the field ofstellar structure andstellar evolution. The lunar craterHenyey is also named in his honour.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1971 (M.P.C. 3143).[10]

Further reading

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References

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  1. ^abcd"JPL Small-Body Database Browser: 1365 Henyey (1928 RK)" (2017-03-21 last obs.).Jet Propulsion Laboratory. Retrieved25 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1365) Henyey".Dictionary of Minor Planet Names – (1365) Henyey.Springer Berlin Heidelberg. p. 111.doi:10.1007/978-3-540-29925-7_1366.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1365) Henyey". Asteroid Lightcurve Database (LCDB). Retrieved12 January 2017.
  4. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  5. ^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.S2CID 46350317. Retrieved12 January 2017.
  6. ^abKlinglesmith, Daniel A. III; Hanowell, Jesse; Risley, Ethan; Turk, Janek; Vargas, Angelica; Warren, Curtis Alan (April 2013)."Asteroid Synodic Periods from Etscorn Campus Observatory".The Minor Planet Bulletin.40 (2):65–67.Bibcode:2013MPBu...40...65K.ISSN 1052-8091. Retrieved12 January 2017.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1365) Henyey".Geneva Observatory. Retrieved12 January 2017.
  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:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved12 January 2017.
  9. ^ab"1365 Henyey (1928 RK)".Minor Planet Center. Retrieved12 January 2017.
  10. ^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.Bibcode:2009dmpn.book.....S.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
Other
Authority control databasesEdit this at Wikidata
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