Kepler Mission Research Paper

Copernicus was a student of astronomy and astrology. He invented astronomy, as we now know it. Moreover, he was greatly shunned for his theory that the earth moves around the sun. This idea was called hello centric. The common theory was geocentric this was the idea that the earth is the center of the universe and everything moved around it. This idea was widely accepted. It was even taught by the church. However, when the church needed a better calendar they turned to a highly famous astrologer named, Copernicus.

Our new understanding of the solar system and the technology we’ve developed through conducting missions has benefitted our society by helping us understand things about other planets, space, and most importantly help us understand more things about our home, planet Earth.

The centuries old quest maybe as old as NASA has been started for other words like our earth has been rejuvenated by the intense surrounding the discovery of hundreds of planets. The kepler mission, which is one of NASA’s best discovery missions it is specifically designed to survey our region of the Milky Way galaxy to discover hundreds of Earth-size and smaller planets in or near a habitable zone.

The topic of finding life on another planet, or seeing if we are the only ones in our Universe has been a mystery to us since the beginning of time. One of the closest findings NASA has found to this topic was exoplanets. Exoplanet is defined as a planet that orbits a star outside the solar system. NASA’s Kepler Space Telescope is the main telescope used to search for exoplanets that have similar features to Earth, and habitability on these exoplanets. NASA has found over 2,000 exoplanets so far, and out of those, there are only about eight exoplanets that seem to have a possibility on being a habitable exoplanets. Among these eight, Kepler 62f seems to be the most plausible.

Johannes Kepler's most important discovery was the three laws of planetary motion. These laws explain the motion the planets have as they orbit around the sun. Kepler

The Kepler spacecraft is a large telescope with .95 meter diameter and a 105 degree view. The telescope's mission is to find earth-like planets that may have an atmosphere and have water. Kepler tries to find planets in habitable zones that are one half-two times

The Kepler Space telescopes was designed to scope out a section of the night sky and take many pictures so it could get a good

The Kepler Mission began in March 7th, 2009. The goal of The Kepler Mission is to “survey a portion of our region of the Milky Way galaxy to discover dozens of Earth-size planets in or near the habitable zone” (NASA). This is accomplished by using a photometer to look for transits, then transferring the data to earth through the Deep Space Network. Once a planet has been detected, a number of different methods can be used to determine the planet’s size, composition and habitability. In order to understand The Kepler Mission completely, one must understand the structure of Kepler, the search methods used, how the data is interpreted, and the implications of the results.

Astronomers began looking for another way to find new planets and cosmos. They needed new equipment and stated Using several South American, African, and Australian telescopes. When scientists started using new telescopes, they were able to detect bigger planets that are farther away from their stars, like Jupiter or Saturn. However, this method does not reveal smaller planets that are close to their stars. Scientist needed another way to find stars so they began to use NASA's Kepler telescope. NASA's Kepler telescope can detect planets as small as Earth. So far astronomers have discovered that there are probably 2 or more planets per star.

The Kepler mission is searching for planets that are enough like Earth to be considered habitable. Discovered in January 2015, Kepler-438b looked like an excellent candidate. The planet fit the two key characteristics for a Kepler candidate to a T. The first of these is that the planet has to be rocky, like Earth or Mars, rather than gaseous, like Jupiter or Saturn. The second is that it has to orbit its star in the habitable zone, where temperatures are neither too hot nor too cold to support life.

Kepler-186f is an ‘Earth cousin’ rather than an ‘Earth twin’ because it orbits a red dwarf star (also known as an M dwarf), a type of star much smaller and dimmer than Earth's own sun. The newfound exoplanet is probably one of many Earth cousins out there, researchers said. The Kepler-186 planetary system lies in the direction of the constellation Cygnus, about 500 light-years away.

After Brahe’s death in 1601, Johannes Kepler took on the position as an imperial mathematician and court astronomer for the Holy Roman emperor, Rudolf II. In 1609, Kepler published his first two laws in ‘Astronomia Nova’. The laws stated “The orbit of a planet is an ellipse where one focus of the ellipse is the sun”, and “A line from the planets to the sun sweep out equal areas in equal

Kuhn (1957) explained that by the sixteenth century, Johannes Kepler (1571-1630) revised the Copernican system in a fundamental way (p. 210). Kepler's arguments are the same as Copernicus', according to Kuhn (p. 210). However, Kepler discarded all epicycles and thought the earth including other planets orbit the sun in elliptic orbits (Kuhn, 1957, p. 210). Also, Kepler resolved the problem of the planets, transformed Copernicus' cumber some system to a sample and correct technique for computing planetary place, according to Kuhn (p. 211). According to Kuhn (1957), Kepler thought the planes of the orbits should intersect in the sun since the sun is central to all planets (p. 210).

position of the planets than any of its kind before it.Before Kepler, Copernicus had proposed

The curriculum included geocentric astronomy. This is the study of how all seven planets at the time - Moon, Mercury, Venus, Sun, Mars, Jupiter and Saturn - moved around the Earth. Their positions to the stars were being calculated by combining circular motions. This system was what worked with the current physics of the time, although there were certain difficulties. However, these astronomers, who also saw themselves as mathematicians, were content to carry on calculating positions of planets. They figured they would leave it to natural philosophers to worry about whether the mathematical figures added up to the physical ones. Kepler, however, did not take like this attitude. His earliest published work in 1956 says that people should consider the actual paths of the planets, and not just the circles used to construct them.