The slopes of a hypothetical Martian volcano have a crater density twice that of the lunar maria. Use Table 11.2 to estimate the age of the volcano.
Table 11.2 Ages of Martian Volcanic Regions
| CRATER DENSITY (RELATIVE TO LUNAR MARIA) | AGE ESTIMATE (BILLIONS OF YEARS) |
Olympus Mons | <0.1 | <0.2 |
Arsia Mons | 0.1 | 0.2 |
Tharsis volcanic plain | 0.5 | 1.6 |
Elysium volcanos | 0.7 | 2.5 |
Chryse volcanic plain | 1.1 | 3.2 |
Alba Patera | 1.8 | 3.5 |
Cratered highlands | 13.0 | 3.8 |
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