Protoplanetary disk formation in rotating, magnetized and turbulent molecular cloud

Kumssa, Gemechu M.; Tessema, Solomon Belay

doi:10.1007/s12036-023-09960-w

Search citation statements

Order By: Relevance

Paper Sections

Select...

Formation Of the Solar System1

Citation Types

Supporting

Mentioning

Contrasting

Year Published

2024

Publication Types

Select...

Article1

Relationship

Self Cite0

Independent1

Authors

Journals

Cited by 1 publication

(1 citation statement)

References 22 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…The latter is thought to have formed about 4.6 billion years ago from an interstellar cloud of gas and dust (protosolar molecular cloud). The cloud collapsed, perhaps because of a shock wave from a nearby supernova, and subsequently flattened into a swirling disk of material (Kumssa and Tessema, 2023). Gravity pulled material into the centre, and the sun was born when hydrogen atoms combined to form helium under extreme pressure in the core (Fig.…”

Section: Formation Of the Solar Systemmentioning

confidence: 99%

Ratification of the base of the ICS Geological Time Scale: the Global Standard Stratigraphic Age (GSSA) for the Hadean lower boundary

Halla,

Noffke,

Reis

et al. 2024

Episodes

View full text Add to dashboard Cite

chemical, physical, and chronological evidence point to the very fast formation of the Solar System and rapid accretion and differentiation of the proto-Earth in only a few million years. Compared to the half-billion-year duration of the Hadean, it is reasonable to set the age of the Earth at the beginning of the formation of the Solar System. This communication explains and justifies the selection of the GSSA for the Hadean base.

show abstract

Section: Formation Of the Solar Systemmentioning

confidence: 99%