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Mercury looks like the Moon: it is heavily cratered with regions of smooth plains, has no natural satellites and no substantial atmosphere. However, unlike the moon, it has a large iron core.
It's similar to the nearside but more heavily cratered. This is due to the nearside being more protected by the earth from bombardments.
It Looks Like Our Moon Just 40% Bigger
It is Venus.
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Mercury has no atmosphere, and its surface is heavily cratered much like Earth's moon. It is estimated that the planet has been geologically dormant for a few billion years.
Ganymede's surface is heavily cratered and crossed by strange grooves and ridges, wich have been described as tire tracks in the desert
Mercury looks like the Moon: it is heavily cratered with regions of smooth plains, has no natural satellites and no substantial atmosphere. However, unlike the moon, it has a large iron core.
Heavily cratered compared to the near side.See related link for a pictorial
The surface of Mercury is filled with craters of all size. The planet's core makes up 42 percent of the planet's volume.
Mercury is heavily cratered because it has virtually no atmosphere and because the surface is geologically inactive, and has been for a protracted period. Without atmospheric weathering or geologic reworking of the surface, any craters become permanent features of the planet.
Mercury is very cratered, like the Moon.
Mercury is sometimes referred to as the "rocky midget" because it is the smallest and innermost planet in our solar system, and it has a rocky, cratered surface.
It's similar to the nearside but more heavily cratered. This is due to the nearside being more protected by the earth from bombardments.
The surface of planet Mercury is fairly similar in appearance to our Moon - without atmosphere to moderate impacts, it is mostly heavily cratered plains. Mercury has a significant variety of features more greatly appreciated from recent observations, including ridges, valleys, plains, escarpments, and mountainous areas. One feature of interest is Apollodorus crater with an unusual radiating spider-like pattern. Surface composition is believed to be mostly silicates but to be poorer or lower in metal content (iron, titanium etc.) than other rocky planets.