| Lightcurve-base 3D-model of 365 Corduba. | |
| Discovery | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery date | 21 March 1893 |
| Designations | |
| (365) Corduba | |
| Pronunciation | /ˈkɔːrdjʊbə/ [1] [2] |
Named after | Possibly Córdoba, Spain [3] |
| 1893 V | |
| Main belt | |
| Orbital characteristics [4] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 117.96 yr (43084 d) |
| Aphelion | 3.2417 AU (484.95 Gm) |
| Perihelion | 2.36078 AU (353.168 Gm) |
| 2.80122 AU (419.057 Gm) | |
| Eccentricity | 0.15723 |
| 4.69 yr (1712.5 d) | |
| 233.78° | |
| 0° 12m 36.792s / day | |
| Inclination | 12.792° |
| 185.196° | |
| 216.45° | |
| Physical characteristics | |
| Dimensions | 105.92±3.0 km [4] 104.51 ± 2.42 km [5] |
| Mass | (5.84 ± 0.95) × 1018 kg [5] |
Mean density | 9.76 ± 1.73 g/cm3 [5] |
| 12.705 h (0.5294 d) | |
| 0.0335±0.002 | |
| C | |
| 9.2 | |
365 Corduba is a very large main-belt asteroid that was discovered by the French astronomer Auguste Charlois on 21 March 1893 from Nice. It is classified as a C-type asteroid and is probably composed of carbonaceous material.
Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado, during 2007 gave a light curve with a period of 6.551 ± 0.002 hours and a brightness variation of 0.05 in magnitude. This differs somewhat from a 2004 study that gave a period of 6.354 hours, but this difference may be explained by the small magnitude variation which tends to increase the randomizing effect of noise in the data. [6]