Examples of using Protoplanetary disk in English and their translations into Indonesian
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ALMA image shows the young star HI Tau and its protoplanetary disk.
The oldest protoplanetary disk ever discovered is 25 million years old.
These pre-main sequence stars are often surrounded by a protoplanetary disk.
The oldest known Protoplanetary disk has an estimated age of 25 million years.
A protostar forms at the core, surrounded by a rotating protoplanetary disk.
In its early days, the so-called protoplanetary disk has nothing particular to reveal.
The protoplanetary disk starts as a disk of gas and dust rotating around the proto-Sun.
Star formation is a complex process,which always produces a gaseous protoplanetary disk around the young star.
Although this protoplanetary disk is being destroyed, the stars that remain in the ring can hold onto their disks. .
Star formation is a complex process,which always produces a gaseous protoplanetary disk, around the young star.
Cha 110913-773444(sometimes abbreviated Cha 110913)is an astronomical object surrounded by what appears to be a protoplanetary disk.
A gas giant'score must form quickly since hydrogen in the protoplanetary disk dissipates rapidly, swept away by stellar winds in just a few million years.
Cha 110913-773444 is anastronomical object surrounded by what appears to be a protoplanetary disk….
During the Solar System's formation,Mars was created out of the protoplanetary disk that orbited the Sun as the result of a stochastic process of run-away accretion.
Iron planets are thought to form in the high-temperature regions close to a star,like Mercury, and if the protoplanetary disk is rich in iron.
The young Sun's solar wind clears away all the gas anddust in the protoplanetary disk, blowing it into interstellar space, thus ending the growth of the planets.
Meanwhile, in the outer part of the nebula, gravity caused matter to condense around density perturbations and dust particles,the rest of the protoplanetary disk beginning separating into rings.
The researchers speculate that following the grains' uptake of water from the protoplanetary disk, the minerals aggregated and stuck together to form pebbles and eventually larger bodies such as asteroids.
The first microscopic life forms are thought to have emerged about a billion years after Earth's formation from the dust,globs and chunks of material that made up the infant sun's protoplanetary disk.
A Sun-like star usually takesapproximately 1 million years to form, with the protoplanetary disk evolving into a planetary system over the next 10-100 million years.[1].
We know that when the conditions are right, like on Earth, life began to pop up on our planet 3.6 billion years ago,approximately a billion years after our planet formed from the protoplanetary disk surrounding our young sun.
Our database collects objects until 60 Jupiter masses andcontains a mix of the planetary brown dwarfs(formed in a protoplanetary disk around a star) and starry brown dwarfs(formed by collapse of interstellar cloud).
Recent computer simulations have even shown that extraterrestrialorganic molecules could have formed in the protoplanetary disk before the formation of the Earth.
Computer simulations show that extraterrestrialorganic molecules could have formed in the protoplanetary disk before the formation of the Earth.
As the cloud began to accelerate, its angular momentum,gravity and inertia flattened it into a protoplanetary disk, perpendicular to its axis of rotation.
As the cloud began to accelerate, its angular momentum, gravity,and inertia flattened it into a protoplanetary disk perpendicular to its axis of rotation.
