346 Hermentaria

Main-belt asteroid From Wikipedia, the free encyclopedia

346 Hermentaria is a very large main-belt asteroid. It was discovered by French astronomer Auguste Charlois on 25 November 1892, in Nice. It is probably named for the town of Herment in the region of Auvergne, France.[5] The asteroid orbits the Sun with a period of 4.68 years and an eccentricity (ovalness) of 0.10. The orbital plane is inclined by 8.7° to the plane of the ecliptic.

Discoverydate25 November 1892
(346) Hermentaria
Quick facts Discovery, Discovered by ...
346 Hermentaria
Orbital diagram
Discovery
Discovered byAuguste Charlois
Discovery date25 November 1892
Designations
(346) Hermentaria
Pronunciation/hɜːrmənˈtɛəriə/
Named after
Herment
1892 P
Main belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc123.38 yr (45,066 d)
Aphelion3.08 AU (460.65 Gm)
Perihelion2.51 AU (376.15 Gm)
2.80 AU (418.40 Gm)
Eccentricity0.10098
4.68 yr (1,708.5 d)
188.671°
0° 12m 38.578s / day
Inclination8.74967°
91.9628°
292.035°
Physical characteristics
Dimensions106.52±2.2 km[1]
93.27±3.05 km[2]
Mass(6.33±0.18)×1018 kg[2]
Mean density
14.89±1.52 g/cm3[2]
28.43 h (1.18 d)[1]
17.790 h (0.74 d)[3]
28.523 h (1.19 d)[4]
0.2189±0.009
S
7.13
Close

This body has a rotational period of 28.523±0.001 h during which it varies in brightness with an amplitude of 0.14±0.01 magnitude.[4] It has a cross-section diameter of ~100 km. 346 Hermentaria is classified as a (stony) S-type asteroid, indicating a siliceous mineralogical composition. The near infrared spectra of this object show absorption features that suggest a mix of the minerals clinopyroxene and orthopyroxene.[6] It may be thermally–evolved, having at least partially melted at some point.[7] The overall shape resembles a prolate spheroid.[3]

References

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