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Analysis of the mare regions demonstrate a limited amount of impact structures indicating that O the mare regions are still presently volcanically active O the mare formed after the lunar highlands making the mare younger than 3.6 billion years old O the mare are around 3.6 billion years old the mare formed well before the Late Heavy Bombardment and is remnants of the oldest crust on the lunar surface

Analysis of the mare regions demonstrate a limited amount of impact structures indicating that O the mare regions are still presently volcanically active O the mare formed after the lunar highlands making the mare younger than 3.6 billion years old O the mare are around 3.6 billion years old the mare formed well before the Late Heavy Bombardment and is remnants of the oldest crust on the lunar surface

Applications and Investigations in Earth Science (9th Edition)
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
Problem 1LR
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Analysis of the mare regions demonstrate a limited amount of impact structures indicating that O the mare regions are still presently volcanically active old O the mare formed after the lunar highlands making the mare younger than 3.6 billion years O the mare are around 3.6 billion years old O the mare formed well before the Late Heavy Bombardment and is remnants of the oldest crust on the lunar surface 自|
Transcribed Image Text:Analysis of the mare regions demonstrate a limited amount of impact structures indicating that O the mare regions are still presently volcanically active old O the mare formed after the lunar highlands making the mare younger than 3.6 billion years O the mare are around 3.6 billion years old O the mare formed well before the Late Heavy Bombardment and is remnants of the oldest crust on the lunar surface 自|
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