Real Life Tatooine Research Paper

The possibility of life beyond Earth is a tantalizing idea long prompting our species to wonder if there are other worlds where life exists. As space technology advances, the chances of finding life on other planets are now greater than ever. With new technologies such as satellites and solar panels, scientists are able to expand their exploration farther into our solar system. In 1995, an astronomer named Michel Mayor together with Didier Queloz discovered 51 Pegasi b. This was truly an incredible discovery that rocked the science community. Pledges b, a wobbling star the size of our sun, was slowly approaching, and according to Mayor’s

the new planet with the 48-inch Samuel Oschin Telescope on October 31, 2003. The object was so far

This implies that the Kepler 11 planetary system is very much like our solar system. The distance (m) of Kepler-11b

Scientists have discovered a new planet that they believe may be capable of housing life. LHS 1140 b, the planet in question, is six times heavier than Earth, yet only 1.5 times as large, suggesting that it is an extremely dense ball of metal and rock. LHS 1140 b is ten times closer to its sun than Earth, as well, making the orbit only 25 days. The sun LHS 1140 b orbits, LHS 1140, is an old, dim red dwarf star, 40 light-years from Earth in the constellation Cetus. Everything about it is rather ordinary; red dwarfs are the most common type of star, and the light that LHS 1140 produces is too dim to be spotted with the naked eye.

Generally in astronomy, light pollution and thick atmospheres distort and impair images from optics like telescopes. Light pollution crowds out the targets being observed, while the atmosphere dims the light received from them. When choosing the location for the building of a new telescope, it is highly beneficial to build in areas with a thinner atmosphere and low light pollution . This is why mountaintops are typically the preferred sites for new telescopes, and why Mauna Kea is a highly desirable location. A new telescope called the Thirty Meter Telescope (TMT) is revolutionary in

As you will no doubt be aware, the plans for development of the outlying regions of the Galaxy require the building of a hyperspatial express route through your star system, and regrettably your planet is one of those scheduled for demolition. The process will take slightly less that two of your Earth minutes. Thank you.” (Adams,

can't help but think of Tatooine. Well both of these planets exist even Kamino grey water­world

two months ago a possible answer for a new home planet has been brought to the

It is truly amazing to think that an organization as big as NASA is even talking about Star Wars. Star Wars has truly become a global phenomenon and I do not think people realize how widespread it is. The upcoming movie is only helping matters, but even before then it was extremely popular. If NASA does eventually make their own Death Star, then it can be rest assured that Star Wars will hit even a new level of popularity. That is almost hard to imagine.

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.

Currently, there is only one planet we know of to host life, and that is our home planet Earth. The question remains as to what is exactly needed for a planet to be considered habitable, but scientists have developed a handful of criteria to help distinguish what planets could be “just right” for life. The ongoing search for possible habitable planets has produced many remarkable findings but nothing quite as extraordinary as the discovery of the system Trappist-1. According to nasa.gov, it is the first known system of seven Earth-size planets around a single star, and it meets the criteria to possibly sustain life (“NASA Telescope Reveals” p.1). This discovery poses a likely answer to the question “are we alone” and drives our search for finding out more about what is out there.

Batalha et al. (2011), Rowe et al. (2014), and Huber et al. (2014) validated and revised the data collected or simulated on Kepler planets. Natalie M. Batalha et al. (2011) utilized photometric and spectroscopic techniques to model the frequencies of Earth-sized planets near sun-like stars, which resulted in precise knowledge of the fundamental stellar properties, and thereby detected the nature of Kepler-10, which is the first rocky planet of Kepler and the smallest transiting exoplanet discovered to date. (Natalie M. Batalha et al 2011) Jason F. Rowe et al. (2014) used fundamental parameters to present fundamental planetary properties based on an analysis of Kepler light curves, spectroscopy based on ground analysis, imaging in high resolution, and Kepler light curves, (Jason F. Rowe et al 2014). The paper cited the research of Borucki et al. (2013) to back up the idea of effective temperatures of the stellar hosts to aid in investigations done by other researchers. Daniel Huber et al. (2014) provide revised properties of the many planetary systems the Kepler mission has discovered, using broadband photometry and asteroseismology in order to characterize 11,532 Kepler targets which were not classified in the KIC(Kepler Input Catalog)

Planet Nine is a hypothetical large planet in the far outer Solar System, the gravitational effects of which would explain the improbable orbital configuration of a group of trans-Neptunian objects (TNOs) that orbit mostly beyond the Kuiper belt.

Extra-terrestrial planets (Exoplanets) have captivated humans for hundreds of years, the idea that there are planets exist outside of our solar system. There are two types of planets: terrestrial planets, or rocky planets and gas giants. With the development of high zoom telescopes and arrays, we as a race, now have the technology to observe and recognise planets outside our solar system. NASA missions such as Hubble and Kepler have yielded huge results for the discovery of exoplanets, with over 3000 planets discovered as of April 2017. Scientist use multiple techniques to discover exoplanets. Spectroscopy (Radial velocity method), transit method,

The radial velocity method was used to detect the first exoplanet, 51 Pegasi b (51 Peg b) around a main sequence star, 51 Pegasi (51 Peg). The radial velocity method uses the variations in velocity of a star due to the gravitational pull from an exoplanet (Lissauer 2002). Furthermore the velocity isn’t measured in terms of actual speed but in terms of light based on the Doppler effect. The Doppler effect occurs when a star moves. When it moves toward us, its wavelengths of light are shortened and when a star moves away from us, its wavelengths of light are lengthened. Through the continued observation of the Doppler effect on a stars spectrum of light, the velocity of a star is inferred. Any change in a stars velocity is caused by a sufficiently massive companion, an exoplanet (Lissaeur 2002).