416 Vaticana
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) |
Jupiter Tisserand parameter | 3.258 |
Physical characteristics | |
Dimensions |
±1.7 km 85.47[1] 87.10 ± 2.57 km[2] |
Mass | (3.27 ± 3.10) × 1018 kg[2] |
5.372 h (0.2238 d) | |
±0.007 0.1689 | |
7.89 | |
|
416 Vaticana is a large Main belt asteroid.
It was discovered by Auguste Charlois on May 4, 1896 in Nice.
References
- 1 2 "416 Vaticana (1896 CS)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 10 May 2016.
- 1 2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 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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