Surface Geology Of Mercury Research Paper

Mercury is like a large rock. Its surface geology is quite similar to Earth's moon. It has many craters from ancient impacts, and also basins and plains. Some of the craters have filled with lava from the planet's interior, and have become lava plains as a result. Boulders and dust from pulverized rock are found on the surface. There are no rivers. The Mariner 10 and Messenger missions sent back many pictures of Mercury's surface, so we know that there is no weather there to affect the surface. From a geological standpoint, Mercury is identified as a planet that has been long dead. Even though it has not been completely mapped by cameras, scientists studying Mercury believe that its surface has not changed for billions of years.

The planet Mercury, named after the Roman God of Thievery, has an incredible grey surface, littered with craters. Whilst it may lack an environment, pulverised dust roams across its massive stretches of grey fields, and rocky cavities form the land of mercury, resulting in a lack of any possibility of life, unfortunately. Images taken from powerful telescopes give the resemblance of this planet to Earth's own moon, through the grey colours and rocky formations. From Muggle Space Probes, we know that there have not been any signs of clouds, dust storms, or any form of a source of water, further connecting it to the moon. The Caloris Basin, the largest crater on the planet, stretches for 1,550 kilometres across Mercury's fields of grey;

The first planet after the Sun, Mercury, has very similar geological features with the Earth's moon. Its surface is covered with varying sizes of craters which was used by scientists to determine the planet's age. It is said that these craters are the "scars" from asteroid and comets during the Late Heavy Bombardment Period. Measuring 1550km, the Caloris Basin is the largest crater in Mercury's surface and 14 other large crater basins were found. Although it has been identified that Mercury's surface is geologically inactive, large deposits of water ice can be found near its poles. These bodies of water ice were found on deep craters around Mercury's poles and are always in the shadows. If one side of the planet is covered with craters, another

Mercury is the smallest planet and is closest to the sun. It's a small, rocky planet that resembles the moon superficially. While the pockmarked surface and rugged terrain suggests a turbulent history, Mercury is no longer geologically active and has not been active for a long time. Mercury has a heavy iron-based core that is proportionally larger than that of any other planet, including Earth. Mercury has a much longer "day" than Earth. For every two Mercury-years, there are only three days. If earth rotated as slowly, each day would last about eight months. This really puts into perspective how slowly the small planet rotates. Despite its slow rotation, its magnetic field has become stronger and more dynamic since its first discovery. There has been a significant change in the geological instant of 35 years.

Mercury, named after the Roman God of Thievery, Commerce, and Travel, is the first planet from the Sun. It is unique because it shows at both morning rise and evening set of the sun. It is rocky, heavily cratered, covered in boulders, and also pulverized dust. The majority of it's surface bears a strong resemblance to that of Earth's moon. It's lack of atmosphere causes wild temperature fluctuations. Temperatures can range from 90 kelvin to 700 kelvin thus creating a planet, from all observations, that cannot sustain life--it is geologically dead. Mercury also has a magnetic field generated by the planet's core that can deflect solar wind and which has a magnetosphere that changes. This was surprising for such a slow rotating planet--one that rotates completely every 88 Earth days.

Mercury, the closest planet to the Sun, is a rocky planet. The heavily cratered planet suggests that meteors or comets were frequent many, many years ago. Mercury's boulder littered surface and pale gray appearance slightly resembles Earth's moon. Like Mars, Mercury is covered in pulverized dust. What Mercury lacks in this, is weather. Muggle probes bring images to us that show no signs of wind, dust storms, or clouds. No rivers have been found on Mercury. Lack of clouds and rivers, (and oceans) suggests that there is no water on the closest planet to the Sun, Mercury. One of Mercury's most famous craters is Caloris basin, which is 1550 km in diameter. Another of Mercury's most famous craters is called Rachmaninoff. Rachmaninoff is 306 km in diameter. These two very large craters were created by astroids impacting the planet in Mercury's early history.

Mercury: the planet mercury is a greyish brown planet that resembles to the moon so much that they are nearly identical. The planet Mercury is, just like the moon, filled with many, many, craters. The planet mercury is the planet closest to the sun or of the eight planets. The planet mercury is also filled with many, many rocks. In our lesson we learned that mercury travels around the orbit in not 88 earth days, but 59 earth days. In 1974, a muggle prove was sent up there to the planet mercury to study it. The planet mercury is, one of the 7 planets that don't have a single life form on it, well that's in any records. The planet mercury is 1,516 miles in size. Next i will move on to venus.

Mercury is a rocky, gray planet that very closely resembles the Earth’s Moon on the surface. Mercury’s surface is full of craters, boulders, and pulverized dust. Its many craters can be tiny or massive. Mercury is geologically inactive, and has been for an extended amount of time. There is an absence of weather on Mercury, and it does not have an atmosphere. Because it has no atmosphere, it cannot control the variations in temperature from day to night, and the temperatures on the planet can range from 90 Kelvin to 700 Kelvin. There are no signs of clouds, rivers (or any other body of water), or dust storms on Mercury. What we know about Mercury and its surface is from information brought back by Mariner 10 and the Messenger mission in the last few decades.

Because of the atmosphere being so dense, it mostly consisting of carbon dioxide and small amounts of nitrogen. With the atmosphere containing large amounts of CO2, along with thick clouds of sulfur dioxide, it causes one of the strongest greenhouse effect in our solar system, making temperatures sky-rocket to at least 735 K. That's hotter than Mercury is! Studies have shown that Venus may have been like Earth and that there was substantial quantities of liquid water on the surface, but after a period of 600 million years to a billion years, the runaway greenhouse effect came to be present after the original water evaporated, generating those gases. The surface of Venus is isothermal, meaning that the temperature remains constant between day and night but also between the equator and the

Mercury's surface is covered with craters, rocks and dust, resulting in a rather barren appearance. It is thought that Mercury's surface greatly resembles that of our Moon which orbits Earth. The study of the surface features by Schiaparelli and his logging of their movements led him to conclude that Mercury always faces the same side towards the Sun. The craters on Mercury's surface range in size from the relatively small, to huge impact craters caused by collisions with asteroids or meteors. The biggest known crater on Mercury, the Caloris Basin, was one of these, with a diameter of 1550km square. The Messenger spacecraft has created a digital imagery of some of Mercury's surface, and identified 15 of these impact craters. There can also be found plains, such as the Odin Planitia, named for the Norse God Odin. There are also mountains, such as the Caloris Montes, valleys such as

Which is the smallest of the eight planets in our solar system? That would be the first planet in our solar system, Mercury. According to www.coolcosmos.com (2012), Mercury is named after the Roman messenger god. This planet was discovered around the 265 B.C. Mercury has 2 nicknames; Quicksilver and Hermes. It is located 28.6 million miles away from the Sun, and 47,845,581.802 miles away from Venus. Mercury is an exciting planet to research because of the missions that have been accomplished on the planet, its composition, and its location in the solar system.

The atmosphere on Venus is composed of mostly Carbon dioxide with small amounts of nitrogen and sulphuric acid. This composition causes a runaway greenhouse gas effect that makes the planet even hotter than Mercury, despite the fact that Mercury is much closer to the sun. The air on Venus is incredibly dense due to the Nitrogen content, which, whilst admittedly is only a small part of the atmospheric composition, is at least four times the amount on Earth. This Atmospheric composition therefore creates a thick layer of

Venus's atmosphere is made up of carbon dioxide. Nitrogen and clouds of sulfuric acid are also there. Nitrogen makes up three fourths of the atmosphere. This causes a greenhouse gas effect that heats the planet, making it even hotter than Mercury. Venus's clouds also shield the planet. Venus has wind speeds of up to 224 mph, keeping Venus's clouds in constant motion. The planet spins very slowly, only once every 243 Earth days, but the clouds circle the planet every four days. On Venus the sun's light rays usually fail to get through Venus's thick atmosphere. That means that Venus's temperature changes a lot from night to day. Venus's clouds appear to be white or yellow. That is why Venus's atmosphere and climate is the way it

The theory of plate tectonics states that the Earth’s lithosphere (top layer of the Earth’s crust) is split up into rigid sections called plates that are moving relative to one another as they move on top of the underlying semi-molten mantle. These plates are either continental, The North American Plate, or oceanic, The Nazca Plate.

The atmosphere of Venus made up of 98% carbon dioxide and 2% Nitrogen. This atmosphere also has the presence of helium, neon and argon. This is yet another thing which makes Venus different from Earth.