protoplanetary disk


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Related to protoplanetary disk: Proplyd, Debris disks

pro·to·plan·e·tar·y disk

 (prō′tō-plăn′ĭ-tĕr′ē)
n.
A disk of gas and dust, often geometrically thin and opaque, orbiting a newly formed star, from which planets may eventually form.
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References in periodicals archive ?
We can't explain their formation, whether through contraction of gas and dust, like a star, or by the accretion of material in a protoplanetary disk around a star, like planets.
At the center of the protoplanetary disk shines a young star, only a few million years old.
Located roughly 176 light years distant, scientists with the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile identified the protoplanetary disk.
1", or 910 AU in a typical protoplanetary disk or 5 AU in the nearest case.
as the protoplanetary disk in which the planet was formed was too hot for ice water or liquid to exist.
The protoplanetary disk may have a local rarefaction or condensation, i.
In computer simulations, scientists have analyzed what would happen to ice grains in the protoplanetary disk around the infant sun.
According to Lauretta, the findings show that comets experienced processes such as heating and chemical reasons in liquid water that changed the minerals they inherited from the time when the solar system still was a protoplanetary disk, a swirling mix of hot gases and dust, before it cooled dawn enough for planets to form.
Instead, they're part of a protoplanetary disk surrounding a young star.
Thus the protoplanetary disk doesn't heat up until the protostar lights up with the multifrequency radiation associated with stellar fusion.
Both teams focused on a star call HR 4796 that earlier studies had suggested could be at the centre of what is called a protoplanetary disk a disk of dust and gas from which planets are thought to form.
Chambers' framework differs from other models like the core accretion model, which dictates that the gas giants start as a solid core that, when it grows to a certain size, pulls in gas from the protoplanetary disk - the dense disk of gas and dust that rotates around a young star and contains the material from which the planets form.