Jump to content

402 Chloë

From Wikipedia, the free encyclopedia
(Redirected from (402) Chloë)

402 Chloë
Modelled shape of Chloë from its lightcurve
Discovery
Discovered byAuguste Charlois
Discovery date21 March 1895
Designations
(402) Chloë
Pronunciation/ˈkli/ KLOH-ee[1]
Named after
Χλόη Khloē
1895 BW
Main 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)
Aphelion2.84302 AU (425.310 Gm)
Perihelion2.27556 AU (340.419 Gm)
2.55929 AU (382.864 Gm)
Eccentricity0.11086
4.09 yr (1,495.5 d)
263.333°
0° 14m 26.617s / day
Inclination11.8254°
129.415°
17.6154°
Physical characteristics
Dimensions54.21±2.5 km
10.664 h (0.4443 d)
0.1483±0.015
K
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 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, which means it belongs to a class of asteroids of which 234 Barbara is the prototype.[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

[edit]
  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ a b c d "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.
[edit]