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August 25 th , 1989 Voyager 2 encounters with Uranus and Neptune January 24 th , 1986 August 25 th , 1989
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August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Dec 21, 2015

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Page 1: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

August 25th, 1989

Voyager 2 encounters with Uranus and Neptune

January 24th, 1986 August 25th, 1989

Page 2: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

The English astronomer, William Herschel, discovered Uranus in 1781

Page 3: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

McDonald Observatory image of Uranus and some of its moons

Page 4: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

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Page 5: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Uranus is the only planet whose axis of rotation lies in its orbital plane (tilt of 98°), probably caused by a large impact.

Page 6: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Comparison of the densities and compositions of the Jovian planets

Page 7: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Interior Structure of Uranus and Neptune

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Page 8: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Approach of Viking 2 on July 15, 1985 of Uranus and 4 of its moons (composite).

Page 9: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

False color (left) and true color images of Uranus, taken by Viking 2

Page 10: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

The ring system of Uranus

Page 11: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Some of the rings of Uranus,

discovered by the Viking spacecraft

Page 12: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Rings of the planet Uranus, with two shepherd moons which keep the ring particles in place, discovered by the Viking spacecraft

Page 13: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Continuous distribution of small particles throughout the ring system of Uranus. Picture taken while the Viking spacecraft was in the shadow of Uranus. These dust lanes were previously unknown. 96 second exposure, hence, background stars form streaks.

Page 14: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Epsilon ring of Uranus, and three of the moons

discovered by the Viking spacecraft

Page 15: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Size comparison of the larger moons of Uranus

Page 16: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Miranda, ~468 km in diameter

Page 17: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

5 km high scarp on Miranda – Miranda may have split apart and reassembled

Page 18: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.
Page 19: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

50 km wide “chevron” on Miranda indicates complex history

Page 20: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Ariel – 1,160 km in diameter; shows many tectonic features

Page 21: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Umbriel - 1,168 km in diameter

Resolution of this Viking image is ~ 10 km. Umbriel

is highly cratered, particularly on its

southern hemisphere (right). It is the darkest

moon of Uranus, with an albedo of ~ 16 %, like our moon. It also is the moon

with lowest internally-generated geologic

activity. The bright spot at the top of the image (near the equator) may be frost.

Page 22: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Titania – 1,580 in diameter; heavily cratered but also has long scarps

Page 23: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.

Oberon – 1,520 km in diameter; bright surface markings, many impact craters

Page 24: August 25 th, 1989 Voyager 2 encounters with Uranus and Neptune January 24 th, 1986August 25 th, 1989.