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402 Chloë

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Main-belt asteroid For other uses, see Chloe (disambiguation).

402 Chloë
Modelled shape of Chloë from its lightcurve
Discovery
Discovered byAuguste Charlois
Discovery date21 March 1895
Designations
MPC designation(402) Chloë
Pronunciation/ˈkloʊi/ KLOH-ee
Named afterΧλόη Khloē
Alternative designations1895 BW
Minor planet categoryMain belt
AdjectivesChloëan (/kloʊˈiːən/ kloh-EE-ən)
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc120.77 yr (44,113 d)
Aphelion2.84302 AU (425.310 Gm)
Perihelion2.27556 AU (340.419 Gm)
Semi-major axis2.55929 AU (382.864 Gm)
Eccentricity0.11086
Orbital period (sidereal)4.09 yr (1,495.5 d)
Mean anomaly263.333°
Mean motion0° 14 26.617 / day
Inclination11.8254°
Longitude of ascending node129.415°
Argument of perihelion17.6154°
Physical characteristics
Dimensions54.21±2.5 km
Synodic rotation period10.664 h (0.4443 d)
Geometric albedo0.1483±0.015
Spectral typeK
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. This asteroid is orbiting the Sun at a distance of 2.56 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.

This asteroid spans a girth of approximately 54 km. It is classified as a K-type asteroid and is a Barbarian, which means it belongs to a class of asteroids of which 234 Barbara is the prototype. 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.

References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ "402 Chloe (1895 BW)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 10 May 2016.
  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, Bibcode:2014A&A...569A.122G, doi:10.1051/0004-6361/201424238, hdl:11336/8937, A122.
  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, Bibcode:2009MPBu...36..109W.

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