Приклади вживання Protoplanetary disk Англійська мовою та їх переклад на Українською
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while grains of ice and dust within the protoplanetary disk slowly accrete together,
type of light waves, scientists found a very large planet inside the protoplanetary disk of the PDS 70 star.
originate from direct-collapses and not from stellar remnants,” said Basu, an internationally recognized expert in the early stages of star formation and protoplanetary disk evolution.
not from stellar remnants,” Basu, an astronomy professor at Western and internationally recognized expert in the early stages of star formation and protoplanetary disk evolution said in a statement.
themselves formed by the coalescence of dust from the protoplanetary disk surrounding the star shortly after its formation.
not from stellar remnants,” says Basu, an astronomy professor at Western who is internationally recognized as an expert in the early stages of star formation and protoplanetary disk evolution.
it was easier for astronomers to search for a probable planet located inside a protoplanetary disk.
researchers detected something weird about the dust in the edge-on protoplanetary disk.
if it was created later on,“inside the protoplanetary disk that surrounded the young sun.”.
Such a debris disk could be formed from the collisions of planetesimals that survive from the early period of the star's protoplanetary disk.
not from stellar remnants,” says Basu, an astronomy professor at Western who is internationally recognized as an expert in the early stages of star formation and protoplanetary disk evolution.
Substantial research progressThe protoplanetary disk of the star PDS 70 was reached in 2012,
start a model out for it from a protoplanetary disk through to its eventual death.
Bodies orbited so slowly in the outer parts of the sun's protoplanetary disk that the slow process of gravitational accretion would need more time than the age of the solar system to form bodies with 14.5
a rotating protoplanetary disk formed, from which subsequently the planets,
Younger debris disks can constitute a phase in the formation of a planetary system following the protoplanetary disk phase, when terrestrial planets may finish growing.[2]
Prior work found that nearly all young stars are initially surrounded by protoplanetary disks.
However, computer simulations have previously suggested that after protoplanetary disks have formed,
But, computer simulations have previously suggested that after protoplanetary disks have formed,
Protoplanetary disks have been observed around several young stars in our galaxy,