Uranus
(second outer-most solar system planet)
Uranus is the second outer-most planet in the solar system.
Characteristics:
Among the solar system planets,
it is easily most similar to Neptune,
with a slightly larger radius and a slightly smaller mass.
Its 28 known moons include
Miranda, Ariel, Umbriel, Titania and Oberon.
It has a ring system, and within the solar system,
only Saturn's is more extensive and was discovered earlier.
Reaching Uranus by spacecraft is a challenge
(suitable launch windows are very infrequent)
and the only mission to fly near it was Voyager 2 in 1986.
A plan for a future (2030s) mission is the Uranus Orbiter and Probe.
(planet,solar system)
Further reading:
https://en.wikipedia.org/wiki/Uranus
https://en.wikipedia.org/wiki/Exploration_of_Uranus
https://en.wikipedia.org/wiki/Moons_of_Uranus
https://www.britannica.com/place/Uranus-planet
http://hyperphysics.phy-astr.gsu.edu/hbase/Solar/uranus.html
http://astroa.physics.metu.edu/nineplanets/uranus.html
https://www.princeton.edu/~willman/planetary_systems/Sol/Uranus/
https://www.windows2universe.org/uranus/statistics.html
Redshift | Parsecs /Distance | Lightyears /Lookback Years | | |
~0 | 17AU | ~0ly | nearest | Uranus |
~0 | 21AU | ~0ly | furthest | Uranus |
|
Referenced by pages:
10199 Chariklo
astronomical symbol
atmosphere
equilibrium temperature (Teq)
gas giant
giant planet
ice
ice giant
Kuiper Airborne Observatory (KAO)
magnetic field
moment of inertia factor
moon
Neptune
obliquity
radiation belt
retrograde orbit
ring system
rotation period
shepherd moon
solar day
solar system object (SSO)
super-Earth
supercritical fluid (SCF)
superionic ice
Titius-Bode law
Uranus Orbiter and Probe
Venus
Voyager
Index