Kepler Telescope

Their limited telescope technology had peaked and they were unable to see any further. With the new star being found, new telescopes created, it was opened up for more discoveries and open mindedness towards astrology. The discovery of Uranus sparked a renewed interest and search for more planets and other things in our solar system. This was the beginning of the “second phase” in the search for more planets. Most people agree that the discovery by William Herschel was a check point in discovery, with the planets before Uranus being the first phase of discovery and the ones after that being the second

The Kepler Mission (NASA Discover mission #10) is designed to survey a portion of the Milky Way galaxy to discover Earth-size planets in or near the habitable zone and determine how many of our galaxy’s billions of stars have such planets. Results from this mission will allow the placing of our solar system within the continuum of planetary systems in the galaxy.

In the article called “Another Earth” by Alice Savage and David Wiece started with the sharing of the theory that life outside of Earth could exist. The author’s son thinks that it’s possible for other living being to exist and live on other planets, but the author had this theory as just a theory until the moment when scientist found a lot of planets that can potentially have live life on them. After that, he starts to share his memories about what people thought about life outside of Earth back in the 70’s. He shares this idea that to find a planet we have to look at stars. He talks about two methods of how we can find a planet looking at a star. Planets have their gravitational pull and when they are moving around a star we can see them

Explore and observe the objects in the solar system to understand how they formed and evolve

One of the first thing that he came up with was he made three laws, later known to be called Kepler’s laws. The first law he came up with is that planets rotate in elliptical paths around the sun. Which leads to his second finding and then later became known as his second law, he figured out that planets rotations are faster as they get more near the sun, then slower as they get further away from the sun. His third and final law dealt with the distance between the planet and the sun and how long it completed an orbit around the sun. Kepler used basic and simple mathematics to figure out how planets move, which proves him to be a very intelligent man at his time and in history. Kepler’s discoveries as well as many other astronomers put him and

NASA Confirms Planet Discovery Only 21 Light Year Away; Comments on Kepler 452b: 'So What Else Is New?'

Since the very beginning of exoplanet discovery, astronomers have been seeking to find an earth-like habitable planet. This search especially rose in importance in the 21st century when we were faced with intensifying problems of resource scarcity and environmental deterioration which directly influence our being on earth. In order to investigate regions in the Milky Way to discover Earth-sized exoplanets in and approximate to a habitable zone, NASA sent Kepler, a Discovery-class mission spacecraft to identify planets in the Habitable Zone of main sequence stars and to generate a better estimate of how many stars in the Milky Way have such planets (Overbye,

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

First off, the most common way to find new planets is Radial Velocity. The Radial Velocity method relies on the fact that a star does not remain completely stationary when it is orbited by a planet. It moves, ever so slightly, in a small circle or ellipse, responding to the gravitational tug of its smaller companion. When viewed from a distance, these slight movements affect the star's normal light spectrum, or color signature. If the star is moving towards the observer, then its spectrum would appear slightly shifted towards the blue; if it is moving away, it will be shifted towards the red. Secondly, Transit Photometry is the second most common method. This method detects distant planets by measuring the minute dimming of a star as an orbiting planet passes between it and the Earth. The passage of a planet between a star and the Earth is called a "transit." If such a dimming is detected at regular intervals and lasts a fixed length of time, then it is very probable that a planet is orbiting the star and passing in front of it once every orbital period. Lastly, the method of Microlensing is Microlensing is the only known method capable of discovering planets at truly great distances from the Earth. Whereas radial velocity searches look for planets in our immediate galactic neighborhood, up to 100 light years from Earth, and transit photometry can potentially detect planets at a distance of hundreds of light-years, microlensing can find planets orbiting stars near the center of the galaxy, thousands of light-years away ( How to Search for Exoplanet.). These methods are detrimental to the discovery of new planets from far

Since its conception in 1958, NASA has been a pivotal organization in innovative technology and space exploration. With inventions such as the Hubble telescope, or the space shuttle, NASA has provided the world with existential research regarding space. With a renewal of popular interest in NASA, the organization would be able to continue contributing vital research in the medical, and technological fields, as well as the future exploration of space as humans know it, and the future habitation of other planets.

To begin with, there is more than one sun out there in space, and a sun can contain about one million planets in space. Scientists have discovered about one thousand planets orbiting distant stars. They have much more to discover! There is a big possibility that in one of those planets life could exist. Another big clue that scientist have discovered is that there are many galaxies in space and we live in one. The galaxy that Earth is located at is called the Milky Way Galaxy. A galaxy can contain many planets just like our galaxy can contains over billions of planets.

Many scientist used telescopes to look at the planets and turned up the brightness. It helped showing how far the planet was and to show there are planets between the star and earth. Scientist started looking for pulsating stars and using them to find different planets. To find smaller planets scientist used NASA’s Kepler telescope. The telescope was very helpful for NASA and it proved that there are smaller planets. They figured out that some stars have planets. NASA’s help was very successful and they found different planets by the

In this article about a natural satellite in space, talks about how one of the biggest moon's in our Solar System has an ocean 10 times the depth of the earth's oceans, About 100 kilometers thick. This was found on Jupiter’s largest moon called Ganymede by using The Hubble Telescope. They’ve first noticed that the moon’s surfaces was flooding, presumably caused by bubbling up from the interior of the moon which could be cause by cryovolcanoes (or ice volcano), which was soon discovered that the moon’s surface is made out of a thick crust of ice. They’ve discovered this ocean through The Hubble Telescope by monitoring Ganymede and Jupiter's auroras, to see the change in their magnetic field, and they’ve noticed that the moon’s aurora does not

As the 25th birthday of the Hubble space telescope (en.wikipedia.org/wiki/Hubble_Space_Telescope) is being celebrated by space enthusiasts, others at the Goddard Space Flight Center (http://www.nasa.gov/centers/goddard/home), located in Greenbelt, Maryland, are working diligently to get the new space telescope James Webb Space Telescope all put together and ready for its travel into space in October 2018.

In 1609, Galileo Galilei, using “spyglass” which allowed one to see things closer than they appeared, made an early version of the telescope. With it, he observed the skies in a way no one had before. He discovered the moon isn’t perfectly globular, it has craters, the Sun has sunspots, Venus orbits the Sun (contrary to widespread belief in his time), and then he observed four “stars” around Jupiter (“Our Solar System”). Within