MIT: 3 Questions - Evidence for Planetary Formation Through Gravitational Instability
September 04, 2024
September 04, 2024
CAMBRIDGE, Massachusetts, Sept. 4 (TNSres) -- The Massachusetts Institute of Technology issued the following Q&A by Richard Teague, the Kerr-McGee career development professor:
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Assistant Professor Richard Teague describes how movement of unstable gas in a protoplanetary disk lends credibility to a secondary theory of planetary formation.
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Exoplanets form in protoplanetary disks, a collection of space dust and gas orbiting a star . . .
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Assistant Professor Richard Teague describes how movement of unstable gas in a protoplanetary disk lends credibility to a secondary theory of planetary formation.
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Exoplanets form in protoplanetary disks, a collection of space dust and gas orbiting a star . . .