Publication Date:
2019-07-18
Description:
Mars has been modified by endogenic and exogenic processes similar in many ways to Earth. However, evidence of Mars embryonic development is preserved because of low erosion rates and stagnant lid convective conditions since the Late Noachian. Early plate tectonism can explain such evidence. Additional information is contained in the original extended abstract.
Keywords:
Lunar and Planetary Science and Exploration
Type:
Lunar and Planetary Science XXXIII; LPI-Contrib-1109
Format:
text
Permalink