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Uranus
Seventh planet from the Sun, discovered in 1781.
William Herschel
Astronomer who discovered Uranus in 1781.
Georgium Sidus
Original name given to Uranus by William Herschel.
Voyager 2
NASA spacecraft that visited Uranus in 1986.
Uranus’s Distance from the Sun
Approximately 1,780,000,000 miles.
Uranus’s Size
31,693 miles in diameter.
Uranus’s Orbital Period
84.01 years.
Uranus’s Rotational Period
17.24 hours (retrograde).
Uranus’s Inclination of rotation axis
97.86Âş, causing extreme seasonal variations.
Impact Theory of Uranus
Hypothesis that an Earth-sized protoplanet caused Uranus' high inclination of rotation axis.
Uranus’s Number of Satellites
27 known moons.
Uranus’s Atmosphere Composition
Hydrogen (83%), helium (15%), and methane (2%).
Ammonia
Not observed in Uranus' upper atmosphere due to low temperature.
Uranus Atmospheric Structure
Blue-green color, few discernible features, seasonal weather effects.
Clouds in Uranus atmosphere
Composed of condensed methane, exhibit banded pattern parallel to latitude lines.
Haze
Tenuous haze in Uranus' upper atmosphere, giving the planet its blue-green hue.
Uranus’s Interior Composition
Core of silicate rock, icy mantle, and gaseous hydrogen/helium envelope.
Diamonds
Extreme pressure and temperature may cause methane molecules to break up into _____ crystals.
Magnetic Field
Generated by ionized water and ammonia within the mantle.
Offset and Tilted Magnetic Field
Uranus' magnetic field is not centered and tilted almost 60Âş with respect to the axis of rotation.
Internal Heat
Uranus radiates less heat than it receives from the Sun, reasons still under debate.
Discovery of Uranus Rings
Discovered unexpectedly in 1977 during a stellar occultation experiment.
Ring Structure and Composition
Eleven narrow rings composed of dark particles, possibly carbonaceous material.
Outer Ring System of Uranus
Two additional rings discovered in 2005, possibly composed of water-ice particles originating from small impacts of a minor moon
Uranus’s Ring Origin
Thought to be the result of collisional fragmentation of moons that once existed around Uranus.
Major Moons
Miranda, Ariel, Umbriel, Titania, and Oberon.
Miranda
Moon with extreme and varied topography, including the tallest known cliff in the solar system.
Ariel
Moon with bright and young surface, extensive system of fractures and faults.
Umbriel
Moon with dark surface, heavily impacted, presence of canyons that suggests early tectonic process
Titania
Moon with similar surface to Ariel, intersected by scarps and canyons and underwent an active phase in which cyrovolcanism erased the early craters
Oberon
the oldest of Uranus’ moons. with heavily cratered surface, intersected by canyons, and a multi-ringed
Uranus’s Minor Moons
22 irregularly shaped and dark moons, possibly captured asteroids or fragments from collisions.
Coronae
Miranda’s broken terrain consists of three large grooved
structures referred to as coronae, which may be the result of “warm” ice upwelling from the moon’s interior.