Astronomy:1622 Chacornac
| Discovery[1] | |
|---|---|
| Discovered by | A. Schmitt |
| Discovery site | Uccle Obs. |
| Discovery date | 15 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 | |
| Minor planet category | main-belt · Flora[3] |
| Orbital characteristics[1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 85.94 yr (31,388 days) |
| |{{{apsis}}}|helion}} | 2.5989 AU |
| |{{{apsis}}}|helion}} | 1.8705 AU |
| 2.2347 AU | |
| Eccentricity | 0.1630 |
| Orbital period | 3.34 yr (1,220 days) |
| Mean anomaly | 146.41° |
| Mean motion | 0° 17m 42s / day |
| Inclination | 6.4607° |
| Longitude of ascending node | 4.3644° |
| 256.53° | |
| Physical characteristics | |
| Dimensions | 8.43±0.32 km[4] 9.85 km (calculated)[3] 10.27±0.65 km[5] |
| Rotation period | 11.485±0.006 h[6] 12.2044±0.0041 h[7] 12.206±0.002 h[8] 12.2190±0.0116 h[7] |
| Geometric albedo | 0.224±0.030[5] 0.24 (assumed)[3] 0.360±0.042[4] |
| S[3][9] | |
| Absolute magnitude (H) | 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 designation 1952 EA, is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 15 March 1952, by French astronomer Alfred Schmitt at the Royal Observatory of Belgium in Uccle, and named after astronomer Jean Chacornac.[2][10]
Orbit and classification
The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids. It orbits the Sun in the inner main-belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,220 days). Its orbit has an eccentricity of 0.16 and an inclination of 6° with respect to the ecliptic.[1] The first precovery was taken at Lowell Observatory in 1930, extending Chacornac's observation arc by 22 years prior to its official discovery observation.[10]
Lightcurves
Between 2009 and 2013, several rotational lightcurves for this asteroid were obtained from photometric observations at the Palomar Transient Factory and the Hunters Hill Observatory, as well as by astronomers Eric Barbotin and Raoul Behrend. Lightcurve analysis gave a rotation period between 11.48 and 12.20 hours with a brightness variation between 0.21 and 0.25 in magnitude ({{{1}}}).[6][7][8]
Diameter and albedo
According to the survey carried out by the Japanese Akari satellite, Chacornac measures 10.3 kilometers in diameter and its surface has an albedo of 0.224,[5] while observations by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission gave a diameter of 8.4 kilometers and a high albedo of 0.36.[4] The Collaborative Asteroid Lightcurve Link agrees with the results obtained by AKARI and assumes an albedo of 0.24 – derived from 8 Flora, the family's largest member and namesake – and calculates a diameter of 9.9 kilometers with an absolute magnitude of 12.2.[3]
Naming
This minor planet was named in memory of French astronomer Jean Chacornac (1823–1873), an early discoverer of minor planets himself, most notably 25 Phocaea. He also discovered the parabolic comet C/1852 K1 (Chacornac) in 1852 and independently discovered 20 Massalia. The lunar crater Chacornac also bears his name.[2] The official naming citation was published by the Minor Planet Center on 1 August 1978 (M.P.C. 4418).[11]
References
- ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 1622 Chacornac (1952 EA)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001622. Retrieved 30 June 2017.
- ↑ 2.0 2.1 2.2 Schmadel, 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.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 "LCDB Data for (1622) Chacornac". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1622%7CChacornac. Retrieved 1 August 2016.
- ↑ 4.0 4.1 4.2 4.3 Masiero, 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. doi:10.1088/2041-8205/759/1/L8. Bibcode: 2012ApJ...759L...8M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M. Retrieved 1 August 2016.
- ↑ 5.0 5.1 5.2 5.3 Usui, 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. doi:10.1093/pasj/63.5.1117. Bibcode: 2011PASJ...63.1117U. (online, AcuA catalog p. 153)
- ↑ 6.0 6.1 Behrend, Raoul. "Asteroids and comets rotation curves – (1622) Chacornac". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#001622. Retrieved 1 August 2016.
- ↑ 7.0 7.1 7.2 7.3 7.4 Waszczak, 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. doi:10.1088/0004-6256/150/3/75. Bibcode: 2015AJ....150...75W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W. Retrieved 1 August 2016.
- ↑ 8.0 8.1 Higgins, 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. ISSN 1052-8091. Bibcode: 2009MPBu...36..159H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2009MPBu...36..159H. Retrieved 1 August 2016.
- ↑ 9.0 9.1 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. doi:10.1016/j.icarus.2015.08.007. Bibcode: 2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 1 August 2016.
- ↑ 10.0 10.1 "1622 Chacornac (1952 EA)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1622. Retrieved 1 August 2016.
- ↑ 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
- Asteroid Lightcurve Database (LCDB), query form (info )
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1622 Chacornac at AstDyS-2, Asteroids—Dynamic Site
- 1622 Chacornac at the JPL Small-Body Database
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