72 Feronia
A three-dimensional model of 72 Feronia based on its light curve. | |
| Discovery | |
|---|---|
| Discovered by | Christian Heinrich Friedrich Peters |
| Discovery date | May 29, 1861 |
| Designations | |
| (72) Feronia | |
| Pronunciation | /fɛˈroʊniə/ |
Named after | Feronia |
| Main belt | |
| Adjectives | Feronian |
| Orbital characteristics | |
| Epoch December 31, 2006 (JD 2454100.5) | |
| Aphelion | 2.539 AU (379.8 Gm) |
| Perihelion | 1.993 AU (298.1 Gm) |
| 2.266 AU (339.0 Gm) | |
| Eccentricity | 0.121 |
| 1,246.123 days (3.41 a) | |
| 146.950° | |
| Inclination | 5.417° |
| 208.137° | |
| 102.608° | |
| Physical characteristics | |
| Dimensions | 83.95±4.02 km |
| Mass | (9.45 ± 3.76/1.75)×1017 kg |
Mean density | 3.045 ± 1.212/0.565 g/cm3 |
| 8.09068 h | |
Pole ecliptic latitude | 287 or 102 |
Pole ecliptic longitude | −39 or −55 |
| 0.063 | |
| TDG | |
| 8.94 | |
72 Feronia is a quite large and dark main belt asteroid. It was the first asteroid discovery by C. H. F. Peters, on May 29, 1861, from Hamilton College, New York State. It was initially thought that Peters had merely seen the already known asteroid 66 Maja, but T.H. Safford showed that it was a new body. Safford named it after Feronia, a Roman fertility goddess.
This asteroid is orbiting the Sun with a period of 3.41 years, having a semimajor axis of 2.266 AU and an eccentricity of 0.121. The orbital plane is inclined by an angle of 5.4° to the plane of the ecliptic. This is a spectral type TDG asteroid with a cross-section size of 84 km. The asteroid has an estimated rotation period of 8.09 h. Hanuš et al. (2013) gives two possible solutions for the pole in ecliptic coordinates: (λ1, β1) = (287°, −39°) or (λ1, β1) = (102°, −55°).