UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
11th Edition
ISBN: 9781319278670
Author: Freedman
Publisher: MAC HIGHER
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Question
Chapter 11, Problem 64Q
To determine
The angular sizes of Phobos and Deimos (the Martian moons) with reference to the point of view of an observer standing on the equator of Mars. Compare it with the size of the Moon, as seen from the Earth. If the size of the Martian moons is as impressive in the Martian sky as the Moon is in the Earth’s sky.
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Although Deimos is smaller than Phobos, Deimos has more debris on its surface. This difference in the two moons is probably the result of
a.
the greater number of impact craters on Deimos.
b.
Martian gravity, which is strong enough to pull debris off the surface of Phobos.
c.
the lack of volcanic activity on the surface of Phobos.
d.
the comparatively weaker gravity on Deimos.
e.
the slower rotation rate of Deimos on its axis.
Enceladus is a moon of Saturn. What unique feature does it possess? which is the correct answer?
Cryovolcanism, where water erupts instead of silicate rock
A dense system of rings
An atmosphere thicker than Earth's
Internal heating due to radioactivity
Has an orbit inside Saturn's rings
Chapter 11 Solutions
UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
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