Theories
Nebular Hypothesis
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The nebular hypothesis is the most widely accepted model in cosmogony explaining the formation and evolution of the Solar System, proposing that it formed from gas and dust orbiting the Sun that accreted to form the planets.
Facts
Proposed YearSourced to the subject's own account Proposed BySourced to the subject's own account Sources
1. Nebular Hypothesis (Wikipedia)
WikipediaLead section (entity-description)Quote, Lead section (entity-description)
The nebular hypothesis is the most widely accepted model in the field of cosmogony to explain the formation and evolution of the Solar System (as well as other planetary systems). It suggests the Solar System was formed from gas and dust orbiting the Sun which accreted to form the planets.
1. Nebular Hypothesis (Wikipedia)
WikipediaLead section (proposed-year)Quote, Lead section (proposed-year)
The theory was developed by Immanuel Kant and published in his Universal Natural History and Theory of the Heavens (1755) and then modified in 1796 by Pierre Laplace.
1. Nebular Hypothesis (Wikipedia)
WikipediaLead section (proposed-by)Quote, Lead section (proposed-by)
The theory was developed by Immanuel Kant and published in his Universal Natural History and Theory of the Heavens (1755) and then modified in 1796 by Pierre Laplace.
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