93 Minerva

93 Minerva
A three-dimensional model of 93 Minerva based on its light curve on the top and an image of the asteroid on the bottom.
Discovery
Discovered byJames Craig Watson
Discovery siteAnn Arbor, Michigan
Discovery date24 August 1867
Designations
(93) Minerva
Pronunciation/mɪˈnɜːrvə/
Named after
Minerva
1949 QN2, A902 DA
Main belt
AdjectivesMinervian, Minervean /mɪˈnɜːrviən/
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc146.14 yr (53379 d)
Aphelion3.1429 AU (470.17 Gm)
Perihelion2.3711 AU (354.71 Gm)
2.7570 AU (412.44 Gm)
Eccentricity0.13998
4.58 yr (1672.0 d)
~17.86 km/s
262.022°
0° 12m 55.116s / day
Inclination8.56143°
4.06265°
274.543°
Physical characteristics
154.155±1.298 km (IRAS)
156 km
Mass3.8×1018 kg (calculated)
Mean density
1.9 g/cm3
Equatorial surface gravity
4.139 cm/s2 (0.004221 g)
Equatorial escape velocity
81 m/s
5.982 h (0.2493 d)
0.056±0.008
C
G?
7.91

93 Minerva is a large triple main-belt asteroid. It is a C-type asteroid, meaning that it has a dark surface and possibly a primitive carbonaceous composition. It was discovered by J. C. Watson on 24 August 1867, and named after Minerva, the Roman equivalent of Athena, goddess of wisdom. An occultation of a star by Minerva was observed in France, Spain and the United States on 22 November 1982. An occultation diameter of ~170 km was measured from the observations. Since then two more occultations have been observed, which give an estimated mean diameter of ~150 km.