*** Welcome to piglix ***

Umbriel (moon)

Umbriel
A round spherical body with its left half illuminated. The surface is dark and has a low contrast. There are only a few bright patches. The terminator is slightly to the right from the center and runs from the top to bottom. A large crater with a bright ring on its floor can be seen at the top of the image near the terminator. A pair of large craters with bright central peaks can be seen along the terminator in the upper part of the body. The illuminated surface is covered by a large number of craters.
Umbriel as seen by Voyager 2 in 1986. At the top is the large crater Wunda, whose walls enclose a ring of bright material.
Discovery
Discovered by William Lassell
Discovery date October 24, 1851
Designations
Pronunciation /ˈʌmbriɛl/ UM-bree-el
Uranus II
Adjectives Umbrielian
Orbital characteristics
266000 km
Eccentricity 0.0039
4.144 d
Average orbital speed
4.67 km/s (calculated)
Inclination 0.128° (to Uranus's equator)
Satellite of Uranus
Physical characteristics
Mean radius
584.7±2.8 km (0.092 Earths)
4296000 km2 (0.008 Earths)
Volume 837300000 km3 (0.0008 Earths)
Mass (1.172±0.135)×1021 kg (2 × 10−4 Earths)
Mean density
1.39±0.16 g/cm3
0.2 m/s2 (~ 0.023 g)
0.52 km/s
presumed synchronous
0
Albedo
  • 0.26 (geometrical)
  • 0.10 (Bond)
Surface temp. min mean max
solstice ? ≈ 75 K 85 K
14.5 (V-band, opposition)
Atmosphere
Surface pressure
zero

Umbriel is a moon of Uranus discovered on October 24, 1851, by William Lassell. It was discovered at the same time as Ariel and named after a character in Alexander Pope's poem The Rape of the Lock. Umbriel consists mainly of ice with a substantial fraction of rock, and may be differentiated into a rocky core and an icy mantle. The surface is the darkest among Uranian moons, and appears to have been shaped primarily by impacts. However, the presence of canyons suggests early endogenic processes, and the moon may have undergone an early endogenically driven resurfacing event that obliterated its older surface.

Covered by numerous impact craters reaching 210 km (130 mi) in diameter, Umbriel is the second most heavily cratered satellite of Uranus after Oberon. The most prominent surface feature is a ring of bright material on the floor of Wunda crater. This moon, like all moons of Uranus, probably formed from an accretion disk that surrounded the planet just after its formation. The Uranian system has been studied up close only once, by the spacecraft Voyager 2 in January 1986. It took several images of Umbriel, which allowed mapping of about 40% of the moon’s surface.

Umbriel, along with another Uranian satellite, Ariel, was discovered by William Lassell on October 24, 1851. Although William Herschel, the discoverer of Titania and Oberon, claimed at the end of the 18th century that he had observed four additional moons of Uranus, his observations were not confirmed and those four objects are now thought to be spurious.


...
Wikipedia

...