120 Lachesis
Discovery | |
---|---|
Discovered by | Alphonse Borrelly |
Discovery date | 10 April 1872 |
Designations | |
Pronunciation | /ˈlækᵻsɪs/ |
Named after | Lachesis |
Main belt | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 143.70 yr (52485 d) |
Aphelion | 3.2814 AU (490.89 Gm) |
Perihelion | 2.95390 AU (441.897 Gm) |
3.11767 AU (466.397 Gm) | |
Eccentricity | 0.052528 |
5.50 yr (2010.7 d) | |
Average orbital speed | 16.86 km/s |
56.2095° | |
0° 10m 44.558s / day | |
Inclination | 6.9643° |
341.193° | |
232.822° | |
Earth MOID | 1.95464 AU (292.410 Gm) |
Jupiter MOID | 1.72275 AU (257.720 Gm) |
Jupiter Tisserand parameter | 3.204 |
Physical characteristics | |
Dimensions | ±2.9 km ( 174.10IRAS)[2] |
Mass | 5.5×1018 kg |
Equatorial surface gravity | 0.0487 m/s² |
Equatorial escape velocity | 0.0920 km/s |
46.551 h (1.9396 d)[2][3] | |
±0.002 0.0463[2] | |
Temperature | ~158 K |
C[4] | |
7.75[2] | |
|
120 Lachesis is a large main-belt asteroid. It was discovered by French astronomer Alphonse Borrelly on April 10, 1872, and independently by German-American astronomer Christian Heinrich Friedrich Peters on April 11, 1872, then named after Lachesis, one of the Moirai, or Fates, in Greek mythology.[5] A Lachesean occultation of a star occurred in 1999 and was confirmed visually by five observers and once photoelectrically.[6]
Photometric observations of this asteroid were made in early 2009 at the Organ Mesa Observatory in Las Cruces, New Mexico. The resulting light curve shows a synodic rotation period of 46.551 ± 0.002 hours with a brightness variation of 0.14 ± 0.02 in magnitude.[3] It has the longest rotation period of an asteroid more than 150 km in diameter.[7] As a primitive C-type asteroid[4] it is probably composed of carbonaceous material.
References
- ↑ Yeomans, Donald K., "120 Lachesis", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 2013-03-25.
- 1 2 3 4 "JPL Small-Body Database Browser: 120 Lachesis". Jet Propulsion Laboratory. Retrieved 12 May 2016.
- 1 2 Pilcher, Frederick (July 2009), "Rotation Period Determinations for 120 Lachesis, 131 Vala 157 Dejanira, and 271 Penthesilea", The Minor Planet Bulletin, 36 (3), pp. 100–102, Bibcode:2009MPBu...36..100P.
- 1 2 Tedesco, E. F.; et al. (February 1989), "A three-parameter asteroid taxonomy", Astronomical Journal, 97, pp. 580–606, Bibcode:1989AJ.....97..580T, doi:10.1086/115007.
- ↑ Schmadel, Lutz D. (2003), Dictionary of Minor Planet Names, 1 (5th ed.), Springer, p. 26, ISBN 3540002383.
- ↑ Dunham, D. W.; et al. (September 2002), "Asteroidal occultation results multiply helped by Hipparcos", The Minor Planet Bulletin, 73 (3), p. 662, Bibcode:2002MmSAI..73..662D.
- ↑ "JPL Small-Body Database Search Engine: diameter > 150 (km) and rot_per > 24 (h)". JPL Solar System Dynamics. Retrieved 2015-06-06.