Late Heavy Bombardment era
E459077
The Late Heavy Bombardment era was a hypothesized period about 4.1–3.8 billion years ago during which the inner Solar System, including bodies like the Moon and Mercury, experienced an intense spike in asteroid and comet impacts that heavily cratered their surfaces.
All labels observed (3)
| Label | Occurrences |
|---|---|
| Late Heavy Bombardment (if it occurred) | 1 |
| Late Heavy Bombardment era canonical | 1 |
| Late Heavy Bombardment era in inner Solar System | 1 |
Statements (50)
| Predicate | Object |
|---|---|
| instanceOf |
event in the early Solar System
ⓘ
hypothesized geological era ⓘ impact bombardment period ⓘ |
| alsoKnownAs |
LHB
NERFINISHED
ⓘ
Late Heavy Bombardment NERFINISHED ⓘ lunar cataclysm NERFINISHED ⓘ |
| appliesTo |
Earth
NERFINISHED
ⓘ
Mars NERFINISHED ⓘ Mercury NERFINISHED ⓘ Moon NERFINISHED ⓘ asteroid belt ⓘ inner Solar System ⓘ |
| associatedWith |
Nice model of Solar System evolution
NERFINISHED
ⓘ
migration of Jupiter and Saturn ⓘ scattering of Kuiper belt objects ⓘ scattering of asteroids ⓘ |
| characterizedBy |
frequent asteroid impacts
ⓘ
frequent comet impacts ⓘ intense spike in impact rate ⓘ |
| controversy |
interpretation of lunar sample ages
ⓘ
whether bombardment was a sharp spike or gradual decline ⓘ |
| effectOn |
formation of large impact basins on Mars
ⓘ
formation of large impact basins on Mercury ⓘ formation of large impact basins on the Moon ⓘ heavy cratering of planetary surfaces ⓘ intense resurfacing of early Earth ⓘ |
| endTime | about 3.8 billion years ago ⓘ |
| evidenceFrom |
ages of lunar basins such as Imbrium and Nectaris
ⓘ
cratering records on Mars ⓘ cratering records on Mercury ⓘ lunar crater density ⓘ meteorite age distributions ⓘ radiometric dating of lunar impact melt rocks ⓘ |
| follows | initial planetary accretion phase ⓘ |
| hypothesized | to result from dynamical instability in giant planets ⓘ |
| impactOn |
early Earth environment
ⓘ
thermal state of Earth’s crust and oceans ⓘ |
| partOf | early history of the Solar System ⓘ |
| possibleEffect |
delivery of organic compounds to Earth
ⓘ
delivery of volatiles to terrestrial planets ⓘ delivery of water to Earth ⓘ sterilization of early surface life on Earth ⓘ |
| relevanceTo |
habitability of early Earth
ⓘ
origin of life on Earth ⓘ |
| startTime | about 4.1 billion years ago ⓘ |
| status | subject of active scientific debate ⓘ |
| studiedBy |
dynamical astronomers
ⓘ
geochemists ⓘ planetary scientists ⓘ |
| timeSpan | approximately 300 million years ⓘ |
Referenced by (3)
Full triples — surface form annotated when it differs from this entity's canonical label.
this entity surface form:
Late Heavy Bombardment (if it occurred)