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1516 Henry

From Wikipedia, the free encyclopedia
Main-belt asteroid

1516 Henry
Discovery[1]
Discovered byA. Patry
Discovery siteNice Obs.
Discovery date28 January 1938
Designations
(1516) Henry
Named after
Paul and Prosper Henry (astronomers, opticians)[2]
1938 BG · 1938 DM
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc79.00 yr (28,854 days)
Aphelion3.1087AU
Perihelion2.1368 AU
2.6227 AU
Eccentricity0.1853
4.25yr (1,551 days)
216.91°
0° 13m 55.2s / day
Inclination8.7440°
125.84°
94.457°
Physical characteristics
Dimensions19.19±4.31 km[4]
19.92±1.7 km[5]
19.98 km(derived)[3]
26.163±0.138 km[6]
26.442±0.150 km[7]
27.70±8.84 km[8]
28.55±0.36 km[9]
10 h[10]
17.370±0.006h[11]
0.039±0.007[6]
0.0392±0.0045[7]
0.04±0.03[8]
0.042±0.001[9]
0.0536±0.011[5]
0.0701(derived)[3]
0.08±0.06[4]
S[3]
11.33±1.36[12] · 11.8[7][9] · 11.90[8] · 11.95[4] · 12.0[1][3] · 12.30[5]

1516 Henry (provisional designation1938 BG) is a stonyasteroid from the middle region of theasteroid belt, approximately 20 kilometers in diameter. It was discovered on 28 January 1938, by French astronomerAndré Patry atNice Observatory in southeastern France.[13] It is named for French astronomers and opticians,Paul and Prosper Henry.[2]

Orbit and classification

[edit]

TheS-type asteroid orbits the Sun in thecentral main-belt at a distance of 2.1–3.1 AU once every 4 years and 3 months (1,551 days). Its orbit has aneccentricity of 0.19 and aninclination of 9° with respect to theecliptic.[1] Noprecoveries were taken, and no prior identifications were made. Henry'sobservation arc starts at Nice in August 1939, or 19 months after its official discovery observation.[13]

Physical characteristics

[edit]

In May 2005, a rotationallightcurve of Henry was obtained by French amateur astronomerChristophe Demeautis. It gave arotation period of 17.370 hours with a brightness variation of 0.54magnitude (U=2).[11] In February 2010, photometric observations byDavid Polishook and others at the CalifornianPalomar Transient Factory gave a divergent period of 10 hours with an amplitude of only 0.04 (U=2).[10]

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, Henry measures between 19.19 and 28.55 kilometers in diameter, and its surface has analbedo between 0.039 and 0.070.[4][5][6][7][8][9] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0701 and a diameter of 19.98 kilometers with anabsolute magnitude of 12.0.[3]

Naming

[edit]

Thisminor planet is named for the two brothersPaul Henry and Prosper Henry (1848–1905 and 1849–1903, respectively), who each discovered seven asteroids. As opticians, they constructed the 76-cm refracting telescope atNice Observatory, among others. While mapping the ecliptic during theirCarte du Ciel survey, they made all their fourteen, low-numbered asteroid discoveries, starting with125 Liberatrix.

The Henry Brothers are also honored by the lunar craterHenry Frères. The Martian craterHenry was named in honour of Paul.[2] The officialnaming citation was published by theMinor Planet Center on 1 April 1978 (M.P.C. 4358).[14]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1516 Henry (1938 BG)" (2017-01-27 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 4 January 2017. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1516) Henry".Dictionary of Minor Planet Names – (1516) Henry.Springer Berlin Heidelberg. p. 120.doi:10.1007/978-3-540-29925-7_1517.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1516) Henry". Asteroid Lightcurve Database (LCDB). Retrieved3 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. ^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.
  6. ^abcMasiero, 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:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.S2CID 118745497. Retrieved3 January 2017.
  7. ^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.S2CID 35447010.
  8. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381. Retrieved3 January 2017.
  9. ^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)
  10. ^abPolishook, D.; Ofek, E. O.; Waszczak, A.; Kulkarni, S. R.; Gal-Yam, A.; Aharonson, O.; et al. (April 2012)."Asteroid rotation periods from the Palomar Transient Factory survey".Monthly Notices of the Royal Astronomical Society.421 (3):2094–2108.arXiv:1201.1930.Bibcode:2012MNRAS.421.2094P.doi:10.1111/j.1365-2966.2012.20462.x.S2CID 40538809.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1516) Henry".Geneva Observatory. Retrieved3 January 2017.
  12. ^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. Retrieved3 January 2017.
  13. ^ab"1516 Henry (1938 BG)".Minor Planet Center. Retrieved3 January 2017.
  14. ^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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