Примери за използване на Mercury's surface на Английски и техните преводи на Български
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Mercury's surface looks similar to our Moon's.
Watch a color movie of Mercury's surface captured by MESSENGER.
Mercury's surface is similar to that of Earth's moons.
It took photographs of 45% of Mercury's surface.
It revealed that Mercury's surface is pockmarked with craters like the Earth's moon.
The sensor's best resolution was 3 kilometers at Mercury's surface.
Prior to MESSENGER, only 45% of Mercury's surface had been seen by spacecraft during the Mariner 10 mission.
Mariner 10 was only able to photograph 45% of Mercury's surface.
The mission mapped 100% of Mercury's surface and crashed into the surface of Mercury in April 2015.
MESSENGER ended its mission on April 30 by crashing into Mercury's surface.
Just a little bigger than our moon and Mercury's surface resembles our Manes very much.
Mariner 10 snapped pictures of roughly 45 percent of Mercury's surface.
The temperature on Mercury's surface exceeds 430 degrees Celsius during the day; however, it falls to minus 180 degrees at night.
When it visited,it managed to take pictures of about 45% of Mercury's surface.
Mercury's surface resembles that of Earth's moon, scarred by many impact craters resulting from collisions with meteoroids and comets.
In 2015, its fuel depleted, MESSENGER crashed into Mercury's surface.
During the day, Mercury's surface temperatures reach 800 degrees Fahrenheit and dip to -290 degrees Fahrenheit at night because the planet has no atmosphere to retain heat.
While it visited it managed to take snap shots of approximately 45 of mercury's surface.
Mercury's surface appears heavily cratered and is similar in appearance to that of the moon, indicating that it has been geologically inactive for billions of years.
If they formed due to shrinkage,they should be uniform across Mercury's surface.
Mercury's surface is overall very similar in appearance to that of the Moon, showing extensive mare-like plains and heavy cratering, indicating that it has been geologically inactive for billions of years.
From this research,the group identified two main rock types on Mercury's surface.
The lack of atmosphere causes Mercury's surface temperature to vary by hundreds of degrees, whereas the thick mantle of carbon dioxide keeps the surface temperature of Venus steady, hardly varying at all, anywhere on the planet or any time of day or night!
Back in 1974, Mariner 10 surveyed only 45% of Mercury's surface on a fly-by mission.
Multi-spectral imaging helped scientists investigate the diversity of rock types that formed Mercury's surface.
In 2018, Europe andJapan plan to launch BepiColombo to better map Mercury's surface and probe its magnetic field.
Researchers want to better understand how energy moves through the corona, andto learn more about the composition and properties of Mercury's surface.
The planet-pointing detectors measured fluorescence, the X-ray emissions coming from Mercury's surface after solar X-rays hit the planet.
The goal is to better understand how energy moves through the corona as well as learning more about the composition and properties of Mercury's surface.
The magnesium/silicon, aluminum/silicon, and calcium/silicon ratios averaged over large areas of the planet's surface show that,unlike the surface of the Moon, Mercury's surface is not dominated by feldspar-rich rocks.