Forming in the system's
colder outer regions, where volatile compounds such as water and carbon dioxide freeze out, makes it possible that the planets incorporated those ices and carried them along to a warmer place where they could melt, evaporate, and become oceans and atmospheres.
Not exact matches
In the second paper, physicist Dejan Vinković of the University of Split in Croatia developed a model that shows how a combination of stellar wind and infrared radiation from the inner disk can blow the ultrafine crystallized silicate particles billions of kilometers from the inner
regions of a protoplanetary disk to its
colder outer sections, where comets and other
cold but rocky objects, such as Pluto, can form.
Imagine that such a black hole is orbited by a wide,
cold disk of material — like the rings of Saturn but larger than our entire solar system — and that this disk possesses an almost transparent
outer region and a denser inner
region.
The
outer region gets much
colder toward the
outer edge.
The brown
region shows the
outer extension of the habitable zone for planets that are massive and
cold enough to hold onto molecular hydrogen — a potent greenhouse gas.
Both this molecule and its simpler cousin hydrogen cyanide (HCN) were found in the
cold outer reaches of the star's newly formed disk, in a
region that astronomers believe is analogous to our own Kuiper Belt — the realm of icy planetesimals and comets beyond Neptune.
For a
region to be
colder it must be losing energy to a heat sink
colder than it is but the only thing
colder than the tropopause at -57 C is
outer space at -269 C.