SYNOPTICAL TABLES.
351
No. | Name. | Sidereal Revolution. |
Mean Apparent Distance. |
Discoverer, | Year of Discovery. | |||
d. | h. | m. | s. | ″ | ||||
1 | Ariel | 2 | 12 | 29 | 21 | 13.54 | Lassell | 1851 |
2 | Umbriel | 4 | 3 | 28 | 8 | 19.28 | Lassell | 1851 |
3 | Titania | 8 | 16 | 56 | 31 | 31.44 | Herschel | 1787 |
4 | Oberon | 13 | 11 | 7 | 13 | 42.87 | Herschel | 1787 |
Additional satellites seen by Herschel, but not re-observed, | 4 |
Direction of movement of satellites | retrograde |
Inclination of the orbits of Titania and Oberon to ecliptic, | 78° 58′ |
Distance from the planet -when satellites become invisible (Herschel), | 14″ |
IMagnifying power required for sustained view, | 300 |
Volume (Earth's = 1), | 76.6 |
Mass (Earth's = 1), . | 18.900 |
Density (Earth's = 1), | .321 |
Diameter (Earth's = 1), | 4.246 |
Diameter |
33,610 |
Diameter |
2.″4 |
Gravity (Earth = 1), | 1.36 |
Gravity |
21.8 |
Light and heat from Sun, perihelion, | .0011 |
Light and heat from Sun |
.0011 |
Year in which Adams computed its place within 2 degrees, | 1845 |
Year in which Leverrier computed its place, | 1846 |
First observed by M. Galle, from Leverrier's indications, 23d Sept., | 1846 |