Примери за използване на Gas clouds на Английски и техните преводи на Български
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Gas clouds.
The lecture was on cosmic gas clouds.
Gas clouds in outer space expand;
They look like gas clouds, but behave like stars.
Gas clouds in outer space expand; they do not contract.
Хората също превеждат
Careful analysis has revealed that there is not enough matter in gas clouds to produce stars.
As the gas clouds enter a particular galaxy, they fall into haphazard orbits.
Careful analysis has revealed that there is not enough m atter in gas clouds to produce stars.
Large gas clouds could also be responsible, collapsing together and rapidly accreting mass.
First, the team fitted the overall rotation of the galaxy, andthen the turbulence in the gas clouds.
The outwardly flowing matter and/or gas clouds would keep moving outward without ever slowing.
When galaxies form,they accumulate mass by gravitationally attracting vast, external gas clouds.
Apart from the gas clouds, Saturn constantly has very strong winds which can reach 1800 km per hour.
When galaxies form,they accumulate mass because their gravity attracts vast, external gas clouds.
In certain open areas there are giant gas clouds, for the lack of a better word, that we have been aware of for a long time.
Most astronomers attribute the effect to interactions between stars and gas clouds throughout the galaxy.
Massive gas clouds started to collapse, but because they were made up of hydrogen and helium alone, they struggle to radiate heat away and dissipate their energy.
The first image according to many experts is the best picture of Jupiter so far that shows gas clouds giant.
That's not the sort of behavior they would expect from the gas clouds around a black hole, even in its most excited state, Haggard said.
On the one hand, it is said to be responsible for the initial uneven distribution that led to the agglomeration of the gas clouds.
Alternatively, galactic collisions can trigger massive starbursts of star formation as the gas clouds in each galaxy are compressed and agitated by tidal forces.
An enormous spiral form with collapsing gas clouds, condensing planetary systems, luminous supergiants, stable middle-aged suns, red giants, white dwarfs, planetary nebulas, supernovas, neutron stars, pulsars, black holes and, there is every reason to think.
It's basically very hot,very low-density gas-- nearly all the gas clouds have been swept out of it.
Astronomers tell us that the solar wind and interstellar gas clouds are over a thousand degrees and sometimes in the millions, but also that the cosmic background temperature is minus 455 degrees Fahrenheit.
These atoms then changed direction further(this time toward one another) and formed gas clouds which then pushed together into stars.
There was going to be an interlude before all this got complicated enough to produce gas clouds, galaxies, planets and continents, let alone tiny corkscrew-shaped things wiggling around in slimy pools and wondering whether evolution was worth all the bother of growing fins and legs and things.
Radio waves can pass through more easily, butordinary radio dishes are still hampered by ionized gas clouds and low resolution.
This material is then heated and radiated by the radiation of the rest of the stars,resulting in glowing gas clouds that can have complex structures, since the emission of the mass from the star is uneven depending on time and direction.
One critic notes on this occasion:"When you open an ordinary scientific book in astronomy you will be showered with pictures of gas clouds and protostars;
Eventually, these rotating clouds flatten themselves to become protostellar disks(protostellar disks are gas clouds around a forming star that are flattened by rotation).