Universe
Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 15, Problem 20Q
To determine

The diameter of the other members of the binary asteroid, when one of the members is 16 times brighter than the other and the larger member has a diamater of 120 km, given that the members have the same albedo.

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The Near Earth Asteroid Rendezvous (NEAR), after traveling 2.1 billion kmkm, is meant to orbit the asteroid Eros at a height of about 15 kmkm. Eros is roughly 40km×km× 6km×km×6kmkm. Assume Eros has a density (mass/volume) of about 2.3×103kg/m32.3×103kg/m3.     Part A What will be the period of NEAR as it orbits Eros?
Suppose an asteroid has a semimajor axis of 4 AU. How long does it take the asteroid to go around the Sun? (a) 2 years (b) 4 years (c) 6 years (d) 8 years
The condensation sequence predicts that asteroids consisting of carbonaceous material would form   a. in the inner solar system where it is warmer.   b. at random locations then migrating to the outer asteroid belt due to the gravitational influence of Jupiter and Saturn.   c. in the outer solar system where it is very cold.   d. between the orbits of Jupiter and Saturn.   e. in the outer asteroid belt where it is cooler.
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