Discovery | |
---|---|
Discovered by | H. Goldschmidt |
Discovery date | March 31, 1856 |
Designations | |
(40) Harmonia | |
Pronunciation | /hɑːrˈmoʊniə/[1] |
Named after | Harmonia |
1950 XU | |
Main belt | |
Orbital characteristics[2] | |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 355.021 Gm (2.373 AU) |
Perihelion | 323.537 Gm (2.163 AU) |
339.279 Gm (2.268 AU) | |
Eccentricity | 0.046 |
1,247.514 d (3.42 a) | |
249.120° | |
Inclination | 4.256° |
94.287° | |
268.988° | |
Physical characteristics | |
Dimensions | 111.251 ± 0.391 km[2] |
Mass | (2.206 ± 0.612/0.42)×1018 kg[3] |
Mean density | 2.867 ± 0.795/0.546 g/cm3[3][a] |
0.3712 d (8.909 h)[4] | |
0.242[5] | |
S | |
9.31 (brightest) | |
6.55[2] | |
40 Harmonia is a large main-belt asteroid. It was discovered by German-French astronomer Hermann Goldschmidt on March 31, 1856,[6] and named after Harmonia, the Greek goddess of harmony. The name was chosen to mark the end of the Crimean War.
The asteroid is orbiting the Sun with a period of 3.42 years and a relatively low eccentricity of 0.046. It has a cross-sectional size of 107.6 km. The spectrum of 40 Harmonia matches an S-type (silicate) in the Tholen classification system, and is similar to primitive achondrite meteorites.[7] Photometric observations at the Organ Mesa Observatory in Las Cruces, New Mexico during 2008–09 were used to generate a light curve that showed four unequal minima and maxima per cycle. The curve shows a period of 8.909 ± 0.001 hours with a brightness variation of 0.28 ± 0.02 in magnitude. This result is compatible with previous studies.[4]
Speckle interferometric observations carried out with the Nicholas U. Mayall Telescope at the Kitt Peak National Observatory during 1982–84 failed to discover a satellite companion.[8] In 1988 a search for satellites or dust orbiting this asteroid was performed using the UH88 telescope at the Mauna Kea Observatories, but the effort came up empty.[9]
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