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410 Chloris

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Main-belt asteroid

410 Chloris
Discovery
Discovered byAuguste Charlois
Discovery date7 January 1896
Designations
MPC designation(410) Chloris
Pronunciation/ˈklɔːrɪs/
Named afterChloris
Alternative designations1896 CH
Minor planet categoryMain belt (Chloris)
AdjectivesChloridian
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc105.91 yr (38683 d)
Aphelion3.38204 AU (505.946 Gm)
Perihelion2.0659 AU (309.05 Gm)
Semi-major axis2.72395 AU (407.497 Gm)
Eccentricity0.24159
Orbital period (sidereal)4.50 yr (1642.1 d)
Mean anomaly125.79°
Mean motion0° 13 9.228 / day
Inclination10.963°
Longitude of ascending node96.940°
Argument of perihelion172.945°
Physical characteristics
Dimensions123.57±5.4 km
115.55 ± 8.22 km
Mass(6.24 ± 0.30) × 10 kg
Mean density7.72 ± 1.69 g/cm
Synodic rotation period32.50 h (1.354 d)
Geometric albedo0.044±0.007
Spectral typeC
Absolute magnitude (H)8.30 

410 Chloris is a very large main-belt asteroid that was discovered by Auguste Charlois on January 7, 1896, in Nice. It is classified as a C-type asteroid and is probably composed of primitive carbonaceous material. The spectrum of the asteroid displays evidence of aqueous alteration. It is the namesake of the Chloris family of asteroids.

Photometrics of this asteroid made in 1979 gave a light curve with a period of 32.50 hours with a brightness variation of 0.28 in magnitude.

References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ Yeomans, Donald K., "410 Chloris", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 10 May 2016.
  3. ^ Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73 (1): 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
  4. ^ Schober, H. J. (July 1983), "The large C-type asteroids 146 Lucina and 410 Chloris, and the small S-type asteroids 152 Atala and 631 Philippina - Rotation periods and lightcurves", Astronomy and Astrophysics Supplement Series, 53: 71–75, Bibcode:1983A&AS...53...71S.
  5. Fornasier, S.; et al. (February 1999), "Spectroscopic comparison of aqueous altered asteroids with CM2 carbonaceous chondrite meteorites", Astronomy and Astrophysics Supplement, 135: 65−73, Bibcode:1999A&AS..135...65F, doi:10.1051/aas:1999161.

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