Eratosthenian
Template:Short description Template:More references Template:Infobox geologic timespan The Eratosthenian period in the lunar geologic timescale runs from 3,200 million years ago to 1,100 million years ago. It is named after the crater Eratosthenes, which displays characteristics typical of craters of this age, including a surface that is not significantly eroded by subsequent impacts, but which also does not possess a ray system. The massive basaltic volcanism of the Imbrian period tapered off and ceased during this long span of lunar time. The youngest lunar lava flows identified from orbital images are tentatively placed near the end of this period.Template:Lead citation needed
Its equivalent on Earth consists of most of the Mesoarchean and Neoarchean eras (Archean eon), Paleoproterozoic and Mesoproterozoic eras (Proterozoic eon).Template:Lead citation needed
ExamplesEdit
Other than Eratosthenes itself, examples of large Eratosthenian craters on the near side of the Moon include Langrenus, Macrobius, Aristoteles, Hausen, Moretus, Pythagoras, Scoresby, Bullialdus, Plutarch, and Cavalerius. On the far side, examples include Olcott, Hamilton, Birkeland, Finsen, Kirkwood, and Ricco.<ref>Unified Geologic Map of the Moon, C. M. Fortezzo, P. D. Spudis, S. L. Harrel, 2020. United States Geological Survey.</ref>
- Eratosthenes (LRO).png
Eratosthenes
- Macrobius crater AS17-M-0296.jpg
Macrobius
- Hausen crater 4193 h2.jpg
Hausen
- Olcott crater AS16-M-3001 ASU.jpg
Olcott
- Kirkwood crater 5029 h3.jpg
Kirkwood