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1622 Chacornac

From Wikipedia, the free encyclopedia
Inner belt asteroid

1622 Chacornac
Discovery[1]
Discovered byA. Schmitt
Discovery siteUccle Obs.
Discovery date15 March 1952
Designations
(1622) Chacornac
Named after
Jean Chacornac
(astronomer)[2]
1952 EA · 1932 DD
1933 UX · 1939 KE
1942 EB1 · 1949 KF
1952 DP2 · 1953 TM1
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc85.94 yr (31,388 days)
Aphelion2.5989AU
Perihelion1.8705 AU
2.2347 AU
Eccentricity0.1630
3.34yr (1,220 days)
146.41°
0° 17m 42s / day
Inclination6.4607°
4.3644°
256.53°
Physical characteristics
Dimensions8.43±0.32 km[4]
9.85 km(calculated)[3]
10.27±0.65 km[5]
11.485±0.006h[6]
12.2044±0.0041 h[7]
12.206±0.002 h[8]
12.2190±0.0116 h[7]
0.224±0.030[5]
0.24(assumed)[3]
0.360±0.042[4]
S[3][9]
11.954±0.001(R)[7] · 12.040±0.001(R)[7] · 12.04±1.25[9] · 12.10[4] · 12.2[1][3][5]

1622 Chacornac (provisional designation1952 EA) is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 15 March 1952, by French astronomerAlfred Schmitt at theRoyal Observatory of Belgium in Uccle, and named after astronomerJean Chacornac.[2][10]

Orbit and classification

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TheS-type asteroid is a member of theFlora family, one of the largest groups of stony asteroids. It orbits the Sun in theinner main-belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,220 days). Its orbit has aneccentricity of 0.16 and aninclination of 6° with respect to theecliptic.[1] The firstprecovery was taken atLowell Observatory in 1930, extending Chacornac'sobservation arc by 22 years prior to its official discovery observation.[10]

Lightcurves

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Between 2009 and 2013, several rotationallightcurves for this asteroid were obtained from photometric observations at thePalomar Transient Factory and the Hunters Hill Observatory, as well as by astronomers Eric Barbotin andRaoul Behrend. Lightcurve analysis gave arotation period between 11.48 and 12.20 hours with a brightness variation between 0.21 and 0.25 inmagnitude (U=2/2/2).[6][7][8]

Diameter and albedo

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According to the survey carried out by the JapaneseAkari satellite, Chacornac measures 10.3 kilometers in diameter and its surface has analbedo of 0.224,[5] while observations by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission gave a diameter of 8.4 kilometers and a high albedo of 0.36.[4] TheCollaborative Asteroid Lightcurve Link agrees with the results obtained by AKARI and assumes an albedo of 0.24 – derived from8 Flora, the family's largest member and namesake – and calculates a diameter of 9.9 kilometers with anabsolute magnitude of 12.2.[3]

Naming

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Thisminor planet was named in memory of French astronomerJean Chacornac (1823–1873), an earlydiscoverer of minor planets himself, most notably25 Phocaea. He also discovered the parabolic cometC/1852 K1 (Chacornac) in 1852 and independently discovered20 Massalia. The lunar craterChacornac also bears his name.[2] The officialnaming citation was published by theMinor Planet Center on 1 August 1978 (M.P.C. 4418).[11]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1622 Chacornac (1952 EA)" (2016-11-19 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1622) Chacornac".Dictionary of Minor Planet Names – (1622) Chacornac.Springer Berlin Heidelberg. p. 129.doi:10.1007/978-3-540-29925-7_1623.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1622) Chacornac". Asteroid Lightcurve Database (LCDB). Retrieved1 August 2016.
  4. ^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. Retrieved1 August 2016.
  5. ^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)
  6. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1622) Chacornac".Geneva Observatory. Retrieved1 August 2016.
  7. ^abcdeWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved1 August 2016.
  8. ^abHiggins, David; Warner, Brian D. (October 2009)."Lightcurve Analysis at Hunters Hill Observatory and Collaborating Stations - Autumn 2009".The Minor Planet Bulletin.36 (4):159–160.Bibcode:2009MPBu...36..159H.ISSN 1052-8091. Retrieved1 August 2016.
  9. ^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. Retrieved1 August 2016.
  10. ^ab"1622 Chacornac (1952 EA)".Minor Planet Center. Retrieved1 August 2016.
  11. ^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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