Uranus: Discovery, Atmosphere, Interior, Rings, and Moons

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33 Terms

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Uranus

Seventh planet from the Sun, discovered in 1781.

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William Herschel

Astronomer who discovered Uranus in 1781.

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Georgium Sidus

Original name given to Uranus by William Herschel.

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Voyager 2

NASA spacecraft that visited Uranus in 1986.

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Uranus’s Distance from the Sun

Approximately 1,780,000,000 miles.

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Uranus’s Size

31,693 miles in diameter.

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Uranus’s Orbital Period

84.01 years.

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Uranus’s Rotational Period

17.24 hours (retrograde).

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Uranus’s Inclination of rotation axis

97.86Âş, causing extreme seasonal variations.

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Impact Theory of Uranus

Hypothesis that an Earth-sized protoplanet caused Uranus' high inclination of rotation axis.

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Uranus’s Number of Satellites

27 known moons.

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Uranus’s Atmosphere Composition

Hydrogen (83%), helium (15%), and methane (2%).

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Ammonia

Not observed in Uranus' upper atmosphere due to low temperature.

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Uranus Atmospheric Structure

Blue-green color, few discernible features, seasonal weather effects.

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Clouds in Uranus atmosphere

Composed of condensed methane, exhibit banded pattern parallel to latitude lines.

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Haze

Tenuous haze in Uranus' upper atmosphere, giving the planet its blue-green hue.

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Uranus’s Interior Composition

Core of silicate rock, icy mantle, and gaseous hydrogen/helium envelope.

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Diamonds

Extreme pressure and temperature may cause methane molecules to break up into _____ crystals.

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Magnetic Field

Generated by ionized water and ammonia within the mantle.

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Offset and Tilted Magnetic Field

Uranus' magnetic field is not centered and tilted almost 60Âş with respect to the axis of rotation.

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Internal Heat

Uranus radiates less heat than it receives from the Sun, reasons still under debate.

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Discovery of Uranus Rings

Discovered unexpectedly in 1977 during a stellar occultation experiment.

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Ring Structure and Composition

Eleven narrow rings composed of dark particles, possibly carbonaceous material.

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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

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Uranus’s Ring Origin

Thought to be the result of collisional fragmentation of moons that once existed around Uranus.

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Major Moons

Miranda, Ariel, Umbriel, Titania, and Oberon.

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Miranda

Moon with extreme and varied topography, including the tallest known cliff in the solar system.

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Ariel

Moon with bright and young surface, extensive system of fractures and faults.

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Umbriel

Moon with dark surface, heavily impacted, presence of canyons that suggests early tectonic process

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Titania

Moon with similar surface to Ariel, intersected by scarps and canyons and underwent an active phase in which cyrovolcanism erased the early craters

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Oberon

the oldest of Uranus’ moons. with heavily cratered surface, intersected by canyons, and a multi-ringed

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Uranus’s Minor Moons

22 irregularly shaped and dark moons, possibly captured asteroids or fragments from collisions.

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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.