Thursday, May 23, 2013

Venus and the Magellan Mapping Project by Emma Blahut 5/23/13


Venus and the Magellan mapping project:
1. What direction does Venus rotate?  Describe theories for why this might be.
If you look at the planets rotating on their planes from a Birdseye view, you’ll notice something unique about Venus. Almost all planets rotate in a counter clockwise manner around the plane. One of the two planets that rotates clockwise is Venus. This direction is east to west and is called a retrograde rotation.  This phenomenon is not very well understood but scientists do have some theories.


1. Some astronomers have a theory that billions of years ago, an extremely large object hit Venus. This collision would have been enough to reverse the direction of rotation. In addition some people believe that when the other object or planet hit, it’s rotational direction and speed averaged out with that of Venus. Below are some of the other theories, but this is the most common.


2. Another idea is that the axis could have flipped over, causing the retrograde rotation. This flip may have been a result of the Sun’s pull on Venus’s very dense atmosphere. This pull would have created very strong atmospheric tides. These strong tides and friction between the planet’s inner core and mantle might have caused Venus’s axis to flip 180 degrees. This means that the planet has in fact been spinning the same way forever, it might just appear to be spinning in the opposite direction because of the flip.


3. Also, instead of the axis flipping, some scientists believe that a result of the Sun’s gravitational force combined with the gravitational force of surrounding planets combined with the tides once caused Venus’s rotation to come to a complete stop before it continued to rotate the opposite direction.


4. A last idea is that during the formation of the solar system, a planet will rotate one way or another depending on which side had more impacts.


Oddly, Venus takes about 7.5 Earth months to revolve around the sun and 8 months to rotate on its axis. This is strange because it means that its “day” is longer than its “year.” One theory is that the planet that hit Venus and made it spin clockwise a million years ago, is also responsible for making Venus rotate around its axis at a slower rate.To further explain, when the unknown planet and Venus collided, it’s momentum combined with Venus’s. As a result the planet slowed down the rotational velocity that Venus might have today, had the other planet not hit. Another one of these theories is that the thick atmosphere that surrounds the planet is affected strongly by the tides, and might possibly be causing the planet to rotate around its axis at a very slow rate.  





                 

 Because of the extreme temperatures and pressure on Venus, it is very tricky to send landers, but the Soviets have done it. The first lander on Venus only lasted for about 23 minutes but it was the first to send information back and it did take some pictures along with measurements of Venus’s temperature. This was the Venera 7. The Venera 8 sent us atmospheric data and lasted for 50 minutes. The Venera 9 orbited Venus and it successfully land on the surface. When it landed, it took pictures along with a 180-degree panorama! The pictures were photographed in UV light and allowed us to see that the illumination at the surface was equivalent to a cloudy day on Earth. The rocky surface of Venus also appeared in the pictures. From Gamma rays, scientists could tell that they had landed on basalt. The Venera 9 was a great success, sending back information for 53 minutes. Veneras 10, 11,12,13,14 and 15 found additional data such as information about the soil, atmosphere, and rocks. The longest mission was the taken by the Venera 12, which sent info for 110 minutes before the heat and pressure got to it. Description: https://lh6.googleusercontent.com/jQy8Z_w12oo3YXwsKkifUCozD71hCMe3IdYIWmf0x0d12HVUWQdE5MGRs-exnCrgNuSHpwmaCY_P3FFfFO1gSDAJnHDjS-5tg1kQqm_LmwlUvLRLCvG-D4H9dgDescription: https://lh4.googleusercontent.com/_haDWHmH3q9akmuBvWJT3HjnWNBdlvSSLR8qfJlRZET_G3xlQJkOImsErSlPyWZH7hFrTNJH9bc8jQl6Pdwvdi8lWtk1PpgYypMlW_8ej6kXEjzKetnNZm5wxQ
The panorama taken by Venera 9.





                  The surface of Venus is actually pretty smooth in a lot of places. It is a very dry place. A lot of features that are found on our planet can be found on Venus. Some of these features are canyons, volcanoes, lava flows, rift valleys, mountains, craters, and plains. The surface looks to be in only one crustal plate unlike earth. Because most meteors burn up in Venus’s atmosphere their aren’t many craters. The few craters that were created are now covered by old lava flows.
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                  Imagine living on Venus. Venus has a very thick atmosphere, making everyday a cloudy day. There is never a time when Venus has a nice, sunny day. When astronomers try to look at it from earth, all that is visible is the smooth layer of cloud that is constantly surrounding the planet. The pressure of Venus’s atmosphere compared to Earth’s is 90 times greater! In addition you wouldn’t be able to breath if you went to Venus because the atmosphere is primarily made up of Carbon Dioxide (95.5 percent) and partly made up of sulfuric acid along with other trace gases. The last problem with living on Venus is the temperature. We have learned how the greenhouse effect takes a toll on Earth but lets think about Venus. On Venus, there is even more energy from the sun than on Earth. Light from the sun heats up Venus’s surface. When the surface heats up, it eventually begins to give off heat. Since Carbon Dioxide is a greenhouse gas and there is so much of it in the atmosphere, it absorbs the heat given off by the surface. This process called the greenhouse effect causes Venus to reach temperatures of about 460 degrees Celsius. To say the least, living on Venus wouldn’t be ideal because of the constant clouds, crushing atmosphere, lack of air, and greenhouse effect.Description: https://lh3.googleusercontent.com/uAwroOB75J6Iqx_bChJMImQxub0eZg1WU8qchm_d95P4bct140ums35HvQuLRx5vIZIYaqCMpmq-OS21_uZtL8RkuZqsj205fVbAVCog-P0oVlmeWUVYWYf2AQDescription: https://lh6.googleusercontent.com/HH_BBJsbalg69bNPkA9Y7BLsarsKhRHRCms6kOmL5kFJ8l3uCk8JimxwTf40GbjUNC7828WysTBJOotts5L37DyvcH0EsT7bQse5Fwc5Ss8qwM0gzhH_i7OHSw










                  Scientists have collected evidence mostly through the Magellan Probe. In 1990, the probe reached Venus. Magellan carried radar instruments, and since they are able to work through the clouds, Magellan mapped out the entire surface of Venus! The views from Magellan were amazingly detailed; allowing computers to show us what Venus would look like from just feet above the surface. These radar images showed that Venus is covered with rock, lava flows, craters, and unique domes that cannot be found on any other planet.


            Some scientists believe that there are still active volcanoes on Venus but they are not entirely sure. Almost the whole surface is made up of volcanoes so it would be unlikely that there are no active ones.  We know for certain that the volcanoes on Venus have once been active though because of the channels that scientists have seen on the surface. These channels would have to be made from lava, not water because we know that the water would’ve just boiled off. Also, there are other volcanic features that resemble pancakes, and volcanoes that are called tick volcanoes.  Because there are not many craters on Venus, it shows us that all craters recent, and old might have just been covered by recent lava.  A huge piece of evidence is that the European Space Agency found 3 volcanoes that were active between 200 and 2.5 million years ago. Around this area, scientists found lava flows that were fairly young. They know these lava flows are young because they are capable of emitting infrared heat.
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                  A common question people ask is: Are there plate tectonics on Venus? Well the answer is no. On Earth, we can clearly map out our volcanoes and see that they make up the right of fire, a string of volcanoes and earthquakes that border the plate boundaries. On Venus, there are no strings of volcanoes, they are randomly scattered. Lastly, there are no subduction zones, and although there may be rifts, there are no mid-ocean ridges.



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