Wednesday, November 13, 2013

The Kepler Mission by John Howlette




Overview:
The Kepler Mission, launched on March 7, 2009, is a program implemented by NASA, with the goal of finding potentially life supporting planets within the habitable zone of their parent stars in the Milky Way Galaxy. These planets are being explored with the help of the Kepler spacecraft. So far the Kepler spacecraft has been able to detect thousands of planet candidates, with as many as 40 billion total planet candidates possibly residing within the Milky Way Galaxy. Currently the Kepler Mission is delayed due to a spacecraft malfunction, a new Kepler mission objective is currently being discussed.

Kepler Spacecraft:
The Kepler spacecraft is a space observatory designed and launched by NASA to find Earth-like planets orbiting a parent star. The Spacecraft has a mass of 1,039 kilograms and utilizes a system of strategically placed mirrors for its telescope. It has about a 12 degrees diameter field of view, which is only about the size of ones fist when it is held at arms length. The Kepler spacecraft is able to catch its amazing images with the help of 42 CCDs at 2200x1024 pixels, which at its time of launch, made it the largest camera to be launched into space. Kepler orbits the sun at a height of 1AU and a period of 372.5 days. Kepler points its photometer to a field in the northern constellations of Cygnus, Lyra, and Draco, which assures that light from the sun, earth, and other stray light, doesn’t disrupt the sensitive light detectors of the photometer. Kepler is operated out of the Boulder, Colorado at the University of Colorado.


Kepler Mission:
Other extrasolar planets founds on projects prior to the Kepler mission, were all the size of Jupiter or larger. The Kepler spacecraft is specially designed to look for planets 30 to 600 times less massive, in order to assure that these planets are more to the order of Earth’s mass. The Kepler spacecraft roams the Milky Way Galaxy locating Earth-sized exoplanets within the habitable zone of a sun-like star, such exoplanets are called “Goldilock planets” because they are not too larger or small, or too far or close to their star, but instead just right!   

Discoveries:
Kepler-69c
The method the Kepler spacecraft uses to locate exoplanets is called the transit method of planet finding. This method involves detecting the depletion of light that occurs when a planets passes in front of its parent star. If the object causes these light depletions on a regular basis, it indicates that it is indeed a planets, and the planet’s size can be calculated from the brightness change, and the planet’s orbit and temperature can be calculated from the time between transits. The photometer has the ability to detect a brightness depletion of 1/100 of a percent. http://kepler.nasa.gov/multimedia/Interactives/HowKeplerDiscoversPlanetsElementary/flash.cfm this simulator animates how the Kepler spacecraft detects new exoplanets, and how the information is then transmitted back to Earth. As of now, the Kepler spacecraft has been able to find 167 confirmed earth-sized “goldilock” exoplanets, with thousands of other unconfirmed exoplanets that are still being observed and researched. Scientists have estimated that there are at least 50 billion planets within the Milky Way Galaxy, and at least 500 million of these planets are within the habitable zone of their parent stars. The first Earth-sized exoplanets discovered by the Kepler spacecraft, were announced on December 20, 2011. These planets included Kepler-20e, and Kepler-20f, which orbit within the habitable zone of their parent star Kepler-20. Although, possibly Kepler’s best exoplanets discovery, and one of its most recent, that is a “prime candidate to host alien life” is Kepler -69c. Kepler-69c is 70% larger than Earth is 2,700 light years away in the constellation Cygnus.


Currently:
As of now the Kepler spacecraft is in a state of rest due to the crippling of two of its reaction wheels. In July 2012 wheel 2 of the Kepler spacecraft fail, later on May 11, 2013, wheel 4 of the spacecraft also failed. Due to the loss of the proper functioning from these two wheels, the Kepler spacecraft can no longer continue its current mission of hunting for Earth-sized exoplanets because it no longer possesses the ability to sufficiently point with accuracy using the transit method. A new mission objective for the Kepler spacecraft is currently being discussed, and such mission candidates include searching for asteroids and comets, looking for evidence of supernovas, and finding huge exoplanets through gravitational microlensing.

Conclusion:
With the estimation of 500 million planets within the habitable zone of a star, out of the 50 billion planets within the Milky Way Galaxy zone alone, it appears as though it is very unlikely that there exists no other life elsewhere in the universe, considering that there are 50 billion other galaxies. Theoretically, this provides the potential for one-sextillion Earth-like goldilock planets alone, within the universe. Considering there are at least 30,000 habitable planets within only 1,000 light years of Earth, it is only a matter of time until alien life is discovered.

                              
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