From Wikipedia, the free encyclopedia

410 Chloris
Discovery
Discovered by Auguste Charlois
Discovery date7 January 1896
Designations
(410) Chloris
Pronunciation /ˈklɔːrɪs/ [1]
Named after
Chloris
1896 CH
Main belt ( Chloris)
AdjectivesChloridian
Orbital characteristics [2]
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)
2.72395 AU (407.497 Gm)
Eccentricity0.24159
4.50 yr (1642.1 d)
125.79 °
0° 13m 9.228s / day
Inclination10.963°
96.940°
172.945°
Physical characteristics
Dimensions123.57±5.4  km [2]
115.55 ± 8.22 km [3]
Mass(6.24 ± 0.30) × 1018 kg [3]
Mean density
7.72 ± 1.69 g/cm3 [3]
32.50  h (1.354  d) [2]
0.044±0.007 [2]
C [2]
8.30  [2]

Chloris ( minor planet designation: 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 [4] and is probably composed of primitive carbonaceous material. The spectrum of the asteroid displays evidence of aqueous alteration. [5] 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. [4]

References

  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ a b c d e f Yeomans, Donald K., "410 Chloris", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 10 May 2016.
  3. ^ a b c 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. ^ 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, 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.

External links


From Wikipedia, the free encyclopedia

410 Chloris
Discovery
Discovered by Auguste Charlois
Discovery date7 January 1896
Designations
(410) Chloris
Pronunciation /ˈklɔːrɪs/ [1]
Named after
Chloris
1896 CH
Main belt ( Chloris)
AdjectivesChloridian
Orbital characteristics [2]
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)
2.72395 AU (407.497 Gm)
Eccentricity0.24159
4.50 yr (1642.1 d)
125.79 °
0° 13m 9.228s / day
Inclination10.963°
96.940°
172.945°
Physical characteristics
Dimensions123.57±5.4  km [2]
115.55 ± 8.22 km [3]
Mass(6.24 ± 0.30) × 1018 kg [3]
Mean density
7.72 ± 1.69 g/cm3 [3]
32.50  h (1.354  d) [2]
0.044±0.007 [2]
C [2]
8.30  [2]

Chloris ( minor planet designation: 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 [4] and is probably composed of primitive carbonaceous material. The spectrum of the asteroid displays evidence of aqueous alteration. [5] 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. [4]

References

  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ a b c d e f Yeomans, Donald K., "410 Chloris", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 10 May 2016.
  3. ^ a b c 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. ^ 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, 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.

External links



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