1992
DOI: 10.1007/bf00054651
|View full text |Cite
|
Sign up to set email alerts
|

Impacts and tectonism in Earth and Moon history of the past 3800 million years

Abstract: The Moon's surface, unlike the Earth's, displays a comparatively clear record of its past bombardment history for the last 3800 Myr, the time since active lunar tectonism under the massive pre-mare bombardment ended. From Baldwin's tabulation of estimated ages for a representative sample of large lunar craters younger than 3800Ma, six major cratering episodes can be discerned. These six bombardment episodes, which must have affected the Earth too, appear to match in time the six major episodes of erogenic tect… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

1994
1994
2005
2005

Publication Types

Select...
3
2

Relationship

0
5

Authors

Journals

citations
Cited by 7 publications
(1 citation statement)
references
References 22 publications
0
1
0
Order By: Relevance
“…However, there is evidence for six major cratering episodes over the past 3800 Myr. Stothers (1992) has correlated these with the six major episodes of erogenic tectonism on Earth, which is of interest with regard to the Earth's history, but also may be interpreted as (i) Providing supportive evidence that the approximate dating of the lunar cratering is correct; and (ii) Indicating that on the longest time-scales (hundreds of Myr) th e errestrial influx is variable. t On time-scales of tens of Myr the influx is also variable.…”
Section: Terrestrial Cratersmentioning
confidence: 99%
“…However, there is evidence for six major cratering episodes over the past 3800 Myr. Stothers (1992) has correlated these with the six major episodes of erogenic tectonism on Earth, which is of interest with regard to the Earth's history, but also may be interpreted as (i) Providing supportive evidence that the approximate dating of the lunar cratering is correct; and (ii) Indicating that on the longest time-scales (hundreds of Myr) th e errestrial influx is variable. t On time-scales of tens of Myr the influx is also variable.…”
Section: Terrestrial Cratersmentioning
confidence: 99%