Makronomy Web Tra LESSON 2 4. How has the rate of crater formation in the solar system changed over time? Why has it cha

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Makronomy Web Tra Lesson 2 4 How Has The Rate Of Crater Formation In The Solar System Changed Over Time Why Has It Cha 1 (40.88 KiB) Viewed 54 times

Makronomy Web Tra LESSON 2 4. How has the rate of crater formation in the solar system changed over time? Why has it changed? 5. Why are there so many more impact caters on the Moon and Mercury than on Earth, even though i Earth is a bigger targer? Why are the craters on the Moon and Marcury so wall preserved? The Moon & Mercury has more Impact crater than there are on earth because the gravitational Pull is much stronger it burns up when it ent the atmost turn into asbes sed Planets don't hav atmosphere. tectonic Process, Notr Surthae. Which peologic processes are controlled by a planet's internal temperature? What factor affects how long these processes will continue on a planet Figure 12-217 Interid TemPature. 7. Why, unlike most other planets, is erosion a dominant process on Earth? Weathering is a fundamental torth Ploves & Caucam 9. What factors control the geologic evolution of a planet? Impact LESSON 3 8. Which geologic process occyrs at the same rate on at planets? Crater formation due to Impacts. Figure 12-2 Use this animation for besson 2 to help you answer question 6. ww Crafering, tectonic activity & erosio sion. 10. Which factor seems to control the types of geologic activity that occur on a planet? Cyg2009 Parsonar, pistingas Puny