Примери за използване на The terrestrial planets на Английски и техните преводи на Български
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Exploration of the terrestrial planets- what can we learn for Earth?
Three worlds, and our own,are known as the terrestrial planets.
How did the terrestrial planets form in the early solar system?
Its liquid hydrosphere(oceans and seas)is unique among the terrestrial planets.
Volatile accretion history of the terrestrial planets and dynamic implications".
All the terrestrial planets and moons… show the marks of these deadly blows, including Earth.
It's difficult to tell,because Earth is the largest of the terrestrial planets.
Europa is similar in bulk composition to the terrestrial planets, being primarily composed of silicate rock.
Is it true that the Earth has the largest diameter of the terrestrial planets?
The terrestrial planets in our solar system are enormously diverse, and I expect the same will be true for exoplanet systems.”.
Indeed, the moon is a linchpin for understanding how the terrestrial planets evolved.
The terrestrial planets all have roughly the same structure: a central metallic core, mostly iron, with a surrounding silicate mantle.
Except for Earth, Mars has the most highly varied andinteresting terrain of any of the terrestrial planets.
Venus has the densest atmosphere of all the terrestrial planets, consisting mostly of carbon dioxide.
Examples are mountains, hills, polar caps, and valleys,which are found on all of the terrestrial planets.
Mars has some of the most highly varied andinteresting terrain of any of the terrestrial planets, some of it quite spectacular.
Imaging this"end member" among the terrestrial planets is crucial to developing a better understanding of how the planets formed and evolved.
Except for Earth, Mars has the most highly varied andinteresting terrain of any of the terrestrial planets.
Understanding this"end member" among the terrestrial planets is crucial to developing a better understanding of how the planets in our Solar System formed and evolved.
Except for Earth, Mars has the most highly varied andinteresting terrain of any of the terrestrial planets, some of it quite spectacular.
Because the terrestrial planets form close to the proto-sun(the Sun at this point has not initiated fusion)the warmth melts away any ices so rocky planets form.
At the centre of the map is the Sun, andclose to it the tiny orbits of the terrestrial planets(Mercury, Venus, Earth and Mars).
Unlike the terrestrial planets and gas giants, whose orbits all lie roughly in the same plane as the Earth's, 2003 UB313's orbit is inclined at an angle of about 44 degrees to the ecliptic.
This figure shows the ratio by weight of potassium to thorium for the terrestrial planets and Moon, plotted versus distance from the Sun.
This is the substance of the Nice Model,which asserts that this migration had a profound effect on the evolution of the Solar System and the formation of the terrestrial planets.
By having a more complete picture of how these impact events affected the evolution of the terrestrial planets, we may gain new insight into how life-bearing planets formed.
Jupiter's gravity disrupted the asteroid belt, tossing many asteroids closer to the Sun,where some collided with the terrestrial planets, including Earth.
Together, this helps us understand whether these planets are small and rocky, like the terrestrial planets in our own Solar System, and also how much light they receive from their parent sun.
In accordance with this theory, the Moon formed during the first 10 to 100 million years of the Solar System, when the terrestrial planets were still forming.