Chamberlin–Moulton planetesimal hypothesis
GPTKB entity
Statements (17)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
scientific theory
|
| gptkbp:alternativeTo |
nebular hypothesis
|
| gptkbp:describes |
formation of the Solar System
|
| gptkbp:field |
gptkb:astronomy
|
| https://www.w3.org/2000/01/rdf-schema#label |
Chamberlin–Moulton planetesimal hypothesis
|
| gptkbp:influencedBy |
observations of binary stars
|
| gptkbp:involves |
close stellar encounter
condensation of planetesimals ejection of material from the Sun |
| gptkbp:proposedBy |
gptkb:Forest_Ray_Moulton
gptkb:Thomas_Chrowder_Chamberlin |
| gptkbp:replacedBy |
modern nebular hypothesis
|
| gptkbp:state |
planets formed from smaller bodies called planetesimals
|
| gptkbp:status |
largely obsolete
|
| gptkbp:yearProposed |
1905
|
| gptkbp:bfsParent |
gptkb:Thomas_C._Chamberlin
|
| gptkbp:bfsLayer |
7
|