416 Vaticana
.png) A three-dimensional model of 416 Vaticana based on its light curve. | |
| Discovery | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery date | 4 May 1896 |
| Designations | |
Named after | Vatican Hill |
| 1896 CS | |
| Main belt | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 117.37 yr (42868 d) |
| Aphelion | 3.4019 AU (508.92 Gm) |
| Perihelion | 2.18001 AU (326.125 Gm) |
| 2.79098 AU (417.525 Gm) | |
| Eccentricity | 0.21891 |
| 4.66 yr (1703.1 d) | |
Average orbital speed | 17.83 km/s |
| 267.98° | |
| 0° 12m 40.968s / day | |
| Inclination | 12.859° |
| 58.117° | |
| 198.162° | |
| Earth MOID | 1.16918 AU (174.907 Gm) |
| Jupiter MOID | 1.66115 AU (248.505 Gm) |
| TJupiter | 3.258 |
| Physical characteristics | |
| Dimensions | 85.47±1.7 km[1] 87.10 ± 2.57 km[2] |
| Mass | (3.27 ± 3.10) × 1018 kg[2] |
| 5.372 h (0.2238 d) | |
| 0.1689±0.007 | |
| 7.89 | |
416 Vaticana is a large Main belt asteroid.
It was discovered by Auguste Charlois on May 4, 1896 in Nice.
References
- ^ a b "416 Vaticana (1896 CS)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 10 May 2016.
- ^ a b Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
External links
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