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Earth has wind, and water, and tectonic plates. This causes impact craters to be destroyed relatively quickly, over the course of hundreds of thousands of years.

Jupiter is a gas giant, and has no crust. Since there's nothing for the meteor to crash into, there's no impact crater at all!

As for Venus, it actually does have a large number of impact craters, they just can't be seen easily underneath the thick atmosphere. However, Venus does have some volcanic activity which damages the craters. This process is so slow that it takes about 500 million years to destroy them all.

Mars, on the other hand, has no processes that destroy craters other than a very thin atmosphere with a little bit of wind. Therefore, the craters there last far longer. In addition, Mars is nearer to the asteroid belt, and is more likely to attract meteors from there than Earth and Venus.

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Q: Why are impact structures more common on the surface of Mars than on the surfaces of Venus Earth and Jupiter?
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