410 Chloris
| Discovery | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery date | 7 January 1896 |
| Designations | |
| (410) Chloris | |
Named after | Chloris |
| 1896 CH | |
| Main belt (Chloris) | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 105.91 yr (38683 d) |
| Aphelion | 3.38204 AU (505.946 Gm) |
| Perihelion | 2.0659 AU (309.05 Gm) |
| 2.72395 AU (407.497 Gm) | |
| Eccentricity | 0.24159 |
| 4.50 yr (1642.1 d) | |
| 125.79° | |
| 0° 13m 9.228s / day | |
| Inclination | 10.963° |
| 96.940° | |
| 172.945° | |
| Physical characteristics | |
| Dimensions | 123.57±5.4 km[1] 115.55 ± 8.22 km[2] |
| Mass | (6.24 ± 0.30) × 1018 kg[2] |
Mean density | 7.72 ± 1.69 g/cm3[2] |
| 32.50 h (1.354 d)[1] | |
| 0.044±0.007[1] | |
| C [1] | |
| 8.30 [1] | |
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[3] and is probably composed of primitive carbonaceous material. The spectra of the asteroid displays evidence of aqueous alteration.[4] It is the namesake of the Chloris family of asteroids.
Photometric 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.[3]
References
- ^ a b c d e f Yeomans, Donald K., "410 Chloris", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 10 May 2016.
- ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
- ^ a b 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, vol. 53, pp. 71–75, Bibcode:1983A&AS...53...71S.
- ^ 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.
External links
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