Kepler Mission
One of the biggest questions in astronomy and astrophysics is if there are planets like Earth somewhere beyond our solar system. For the longest time it was impossible to find out for sure. This was for several reasons. First stars are much bigger than planets. Second, stars are much brighter than planets. Because of these to facts it was impossible for telescopes to find planets beyond our solar system. It is like a normal person trying to find to seen an atom beneath someone's show with their naked eye. Then came the Kepler observatory.
Scientist have developed many indirect methods to guess if a star had planets. They could observes a star's motion or see if its light was bent by gravity. These methods were based on the fact that a star with planets would move in a small circle caused by the center of mass of shared star and it planets. With the right instruments and calculations astronomers could determine if a star had planets.
The Kepler observatory is a space observatory that was launched March 9 last year. It had new instrument that would allow for more rapid and efficient discovery of extrasolar planets. It does so by observing the light of stars. The is called the transit method and it is actually quite simple and effective. A star should emit a steady amount of light if it has no planets. However, if a planet were to pass in between it and Earth we would be able to notice a slight dip in the amount of light we observe from the star. The Kepler space observatory does this using a photometer that measures the apparent magnitude of target stars. However there are some drawbacks. The dip in magnitude can be caused by the star itself. For this reason such stars are excluded. Another problem is line of sight. Only a percentage of all stars are observable from earth and an even smaller percentage likely have planets whose orbits are on the same plane as ours. However this still leaves a large number of stars to observe.
The main mission of the Kepler Observatory is to find planets in the habitable zones of stars that might have similar characteristics to Earth. We are able to do this because we can calculate the diameter of found planets from the dip in apparent magnitude caused when they pass in front of their stars. The Kepler mission is expected to last 3.5 years.
If you enjoyed this article there are several others Universe Today that you will enjoy. There is a good article about Kepler's first planet sighting. There is also an interesting article about Kepler being used to measure the size of the Universe.
You can also find great resources online. You can go to NASA's Kepler web site. You can also check out seti.org.
You can also listen Astronomy Cast. Episode 34 talks about looking for other Earths.
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