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120 Lachesis
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Main-belt asteroid
October 2012
yes
#D6D6D6
120 Lachesis
Alphonse Borrelly
10 April 1872
(120) Lachesis
000120-asteroid shape model (120) Lachesis.png
3D convex shape model of 120 Lachesis
A872 GB; 1910 CF;1918 UB
ˈ l æ k ᵻ s ɪ s LAK iss isshttp://www.lexico.com/definition/Lachesis https://web.archive.org/web/20200323121500/https://www.lexico.com/definition/lachesis dead March 23, 2020 Lachesis Lexico UK English Dictionary Oxford University Press
Lachesian (l æ ˈ k iː ʃ ( i ) ə n ,_ l ə ˈ k iː ʒ ə n la KEE sh(ee )ən ,_ lə KEE zhən)
Lachesis
Main belt
31 July 2016 (JD 2457600.5)
3.11767 AU Gm on
2.95390 AU Gm on
3.2814 AU Gm on on
0.052528
5.50 yr (2010.7 d)
6.9643°
341.193°
232.822°
56.2095°
16.86 km/s
155.132 1.133 km (IRAS)
4.27 0.36 18 kgCalculated from its standard gravitational parameter GM = 0.285 0.024 km3 s2.
2.18 g/cm3
0.0487 m/s2
0.0920 km/s
46.551 h d on on
C
7.75
0.0463 0.002
~158 K
0.179044 ms / day
143.70 yr (52485 d)
0
1.95464 AU Gm on
1.72275 AU Gm on
3.204
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. A Lachesean occultation of a star occurred in 1999 and was confirmed visually by five observers and once photoelectrically, with the chords yielding an estimated elliptical cross-section of 184 × 144 km.
This body is orbiting the Sun with a period of 5.50 years and an eccentricity (ovalness) of 0.05. The orbital plane is inclined by 7° to the plane of the ecliptic. 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. It is a very slow rotator with the longest rotation period of an asteroid more than 150 km in diameter. As a primitive C-type asteroid it is probably composed of carbonaceous material.
Notes
References
JPL Small-Body Database Browser: 120 Lachesis
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=120
Jet Propulsion Laboratory
18 Dec 2022
120 Lachesis - a very slow rotator
Bembrick Colin Allen Bill
Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers
32 3 45–46 September 2005
2005MPBu...32...45B
JPL Small-Body Database Search Engine: diameter > 150 (km) and rot_per > 24 (h)
JPL Solar System Dynamics
https://ssd.jpl.nasa.gov/sbdb_query.cgi?obj_group=all;obj_kind=all;obj_numbered=all;OBJ_field=0;ORB_field=0;combine_mode=AND;c1_group=OBJ;c1_item=Ap;c1_op=%3E;c1_value=150;c2_group=OBJ;c2_item=As;c2_op=%3E;c2_value=24;table_format=HTML;max_rows=50;format_option=comp;c_fields=AcBhBgBjBiBnBsAiApAs;.cgifields=format_option;.cgifields=ast_orbit_class;.cgifields=combine_mode;.cgifields=table_format;.cgifields=obj_kind;.cgifields=obj_group;.cgifields=obj_numbered;.cgifields=com_orbit_class&query=1&c_sort=AsD
2015-06-06
Lutz D.
Schmadel
Dictionary of Minor Planet Names
Springer
26
1
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https://books.google.com/books?id=VoJ5nUyIzCsC&pg=PA26
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Asteroidal occultation results multiply helped by Hipparcos
The Minor Planet Bulletin
73
3
662
September 2002
2002MmSAI..73..662D
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Rotation Period Determinations for 120 Lachesis, 131 Vala 157 Dejanira, and 271 Penthesilea
The Minor Planet Bulletin
36
3
100–102
July 2009
2009MPBu...36..100P
.
Tedesco
E. F.
Williams
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97
580–606
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10.1086/115007
1989AJ.....97..580T
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Fuentes-Muñoz Oscar Farnocchia Davide Giorgini Jon D. Park Ryan S. 2025-12-01 Asteroid Mass Estimation by Mutual Perturbations During Close Encounters After Gaia Focused Product Release The Astronomical Journal 170 6 353 10.3847/1538-3881/ae0cc9 0004-6256 free 2025AJ....170..353F 283347135
External links
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119 Althaea 120 121 Hermione
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Category:Discoveries by Alphonse Borrelly
Category:Named minor planets
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