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Refer to Figures 10-17, 10-23a, and 10-24 in the Text

Question 91

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Refer to Figures 10-17, 10-23a, and 10-24 in the text. The surfaces of Ida, Mathilde, and Eros, asteroids photographed by the Galileo and NEAR Shoemaker spacecraft are Refer to Figures 10-17, 10-23a, and 10-24 in the text. The surfaces of Ida, Mathilde, and Eros, asteroids photographed by the Galileo and NEAR Shoemaker spacecraft are A) densely covered with ancient large and small overlapping craters, similar to the surface of the highland areas of the Moon. B) irregular, somewhat rounded, and moderately cratered. C) covered with ice that is crisscrossed with cracks and systems of parallel grooves. D) covered with young, sharp, jagged protrusions, due to fragmentation by collision with other asteroids, and few craters. Refer to Figures 10-17, 10-23a, and 10-24 in the text. The surfaces of Ida, Mathilde, and Eros, asteroids photographed by the Galileo and NEAR Shoemaker spacecraft are A) densely covered with ancient large and small overlapping craters, similar to the surface of the highland areas of the Moon. B) irregular, somewhat rounded, and moderately cratered. C) covered with ice that is crisscrossed with cracks and systems of parallel grooves. D) covered with young, sharp, jagged protrusions, due to fragmentation by collision with other asteroids, and few craters. Refer to Figures 10-17, 10-23a, and 10-24 in the text. The surfaces of Ida, Mathilde, and Eros, asteroids photographed by the Galileo and NEAR Shoemaker spacecraft are A) densely covered with ancient large and small overlapping craters, similar to the surface of the highland areas of the Moon. B) irregular, somewhat rounded, and moderately cratered. C) covered with ice that is crisscrossed with cracks and systems of parallel grooves. D) covered with young, sharp, jagged protrusions, due to fragmentation by collision with other asteroids, and few craters.


A) densely covered with ancient large and small overlapping craters, similar to the surface of the highland areas of the Moon.
B) irregular, somewhat rounded, and moderately cratered.
C) covered with ice that is crisscrossed with cracks and systems of parallel grooves.
D) covered with young, sharp, jagged protrusions, due to fragmentation by collision with other asteroids, and few craters.

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