Astronomy:402 Chloë

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Short description: Main-belt asteroid
402 Chloë
000402-asteroid shape model (402) Chloë.png
Modelled shape of Chloë from its lightcurve
Discovery
Discovered byAuguste Charlois
Discovery date21 March 1895
Designations
(402) Chloë
Pronunciation/ˈkli/ KLOH-ee[1]
Named afterΧλόη Khloē
1895 BW
Minor planet categoryMain belt
AdjectivesChloëan (/klˈən/ kloh-EE-ən)
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc120.77 yr (44,113 d)
|{{{apsis}}}|helion}}2.84302 astronomical unit|AU (425.310 Gm)
|{{{apsis}}}|helion}}2.27556 AU (340.419 Gm)
2.55929 AU (382.864 Gm)
Eccentricity0.11086
Orbital period4.09 yr (1,495.5 d)
Mean anomaly263.333°
Mean motion0° 14m 26.617s / day
Inclination11.8254°
Longitude of ascending node129.415°
17.6154°
Physical characteristics
Dimensions54.21±2.5 km
Rotation period10.664 h (0.4443 d)
Geometric albedo0.1483±0.015
K
Absolute magnitude (H)9.02


402 Chloë (prov. designation: A895 FB or 1895 BW) is a large main-belt asteroid. It was discovered by French astronomer Auguste Charlois on 21 March 1895 from Nice.[2] This asteroid is orbiting the Sun at a distance of 2.56 astronomical unit|AU with a period of 4.09 years and an eccentricity of 0.11. The orbital plane is inclined at an angle of 11.8° to the plane of the ecliptic.[2]

This asteroid spans a girth of approximately 54 km.[2] It is classified as a K-type asteroid and is a Barbarian.[3] Analysis of the asteroid light curve, based on photometric data collected during 2009, show a rotation period of 10.664±0.001 h with a brightness variation of 0.30±0.01 in magnitude.[4]

References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. 2.0 2.1 2.2 2.3 "402 Chloe (1895 BW)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=402. 
  3. Gil-Hutton, R. et al. (September 2014), "Polarimetric survey of main-belt asteroids. IV. New results from the first epoch of the CASLEO survey", Astronomy & Astrophysics 569: 6, doi:10.1051/0004-6361/201424238, A122, Bibcode2014A&A...569A.122G. 
  4. Warner, Brian D. (July 2009), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 December - 2009 March", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers 36 (3): 109–116, Bibcode2009MPBu...36..109W. 

External links