If the protoplanet grows by frost line, and become a hot Jupiter orbiting very close to its star, then gradually losing small amounts of mass as the star's radiation strips its atmosphere.
12.
The most widely accepted theory of the Moon's origin, the giant-impact hypothesis, states that it formed from the collision of a Mars-size protoplanet called Theia with the early Earth.
13.
The accumulation of gas by the core is initially a slow process, which continues for several million years, but after the forming protoplanet reaches about 30 Earth masses ( ) it accelerates and proceeds in a runaway manner.
14.
The clouds of captured hydrogen and helium gas contracted, spun up, flattened, and deposited gas onto the surface of each giant protoplanet, while solid bodies within that disk accreted into the giant planet's regular moons.
15.
The reason for Uranus's unusual axial tilt is also not known with certainty, but the usual speculation is that during the formation of the Solar System, an Earth-sized protoplanet collided with Uranus, causing the skewed orientation.
16.
The star is surrounded by a circumstellar disk from a distance of 0.2 to 4 AU, and again from 13 AU out to a few hundred AU, with evidence for a protoplanet forming at a distance of around 47 AU.
17.
I just read that Vesta has an iron core with radius 107 to 113 km; the protoplanet has overall dimensions of " 572.6?57.2?46.4 km " as our article summarizes this ( I can't access the original report at the moment, despite how much the taxpayers paid for this probe . . . ).
18.
My edits vary from myofibril to German auxiliary cruiser Atlantis, from Procedural defense to Military history of the Philippines, from calculus to New Imperialism, from protoplanet to SmarTruck II, from wind winnowing to tanning-- so I suppose I have made a vague effort to comply; however, since I have edited so many thousands of articles . . . these are just a few-- frankly, the list of topics which I have edited is longer than this sampling of random articles.
19.
It has a substellar companion calculated to have a mass 9.2 times that of Jupiter and an orbital period of 124.6 days at a distance of approximately 0.57 AU . Yet another member of the Lower Centaurus Crux subgroup, It is surrounded by a circumstellar debris disk from a distance of 0.2 to 4 AU, and again from 13 AU out to a few hundred AU, with evidence for a protoplanet forming at a distance of around 47 AU . There is a gap between 4 and 13 AU, which appears to contain a large planet around 20 times the mass of Jupiter, although further examination of the disk profile indicates it might be a more massive object such as a brown dwarf or more than one planet.
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