Venus :: essays research papers

genus genus Venus is the second artificial satellite from the sun and the sixth largest. Venus orbit is the most circular of all planet, with an eccentricy of less than 1%. Venus, perchance because it is the brightest of planets known to the ancients, Is named after the Greek goddess of make protrude and beauty. The planet of Venus has been known since prehistoric times and is the brightest object in the sky with the exception of the sun and the moon. Venus rotation is somewhat fantastic in that it is both very slow ( 243 basis days per Venus day) and retrograde. In addition, the periods of Venus rotation and of its orbit are synchronized such(prenominal) that it always presents the same face toward Earth when the two planets are at their closest approach. The pressure of the planets ambiance at the rise is 90 atmospheres and is composed mostly of carbon dioxide. There are several(prenominal) layers of clouds which are more kilometers thick and composed of sulfuric acid. This dense atmosphere produces a run-away greenhouse effect that raises Venus surface temperature by active 400 degrees to over 740 K. The planet of Venus is often regarded as Earths sister planet, in some ways they are very similar. For example, Venus is only slightly smaller than Earth (95% of Earths diameter, 80% of Earths mass.) Both have few craters indicating comparatively young surfaces. Their densities and chemical compositions are also similar. Because of these similarities, it was once thought that to a lower place its dense clouds, Venus might be very earthlike, perhaps to the point of containing life. However, a more detailed study of Venus revealed that many aspects of Venus atmosphere was much different from that of Earth.There are no small craters on Venus. It appears that small meteoroids burn up in Venus dense atmosphere before reaching the surface. Craters on Venus take care to come in bunches indicating that the large meteoroids that do reach the surface unrem arkably break up in the atmosphere. The oldest terrains on Venus seem to be virtually 800 million years old. Extensive volcanisms at the time wiped out the earlier surface including any large craters from early Venus history.The inside(prenominal) of Venus is probably very similar to that of Earth. It consists of an iron core about 3000 km in radius, a molten rocky mantle comprising the bulk of the planet. Venus probably once had large