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It is important to know at any age!

In order to spot such a remote exomoon, the authors of this new study, The Hunt for Exomoons with Kepler (HEK): III. The First Search for an Exomoon around a Habitable-Zone Planet, used a technique that models the dips and features of the parent star's light-curve (stellar brightness vs. time), which are caused by transits of the planet (and any accompanying moons) in front of the face of its star. This is a complicated and difficult endeavor because numerous and diverse models of planet-moon dynamics must be taken into consideration. Each one of these models possesses parameters that describe physical properties belonging to the planet or moon, as well as parameters describing the orbital system. The authors use what is termed Bayesian statistics to account for the fact that the true orbital model of this planetary system is still not known--and this enables them to calculate if a model with our without a moon fits the observed light-curve the best.



and here is another

Since the beginning of civilization, mankind has always been looking toward the stars. Perhaps this is because mankind is always looking for ways to expand his sphere of influence. In order to achieve this, it is essential that mankind to expand further out into space. Especially when mankind stepped onto the Lunar soil for the first time; the possibility of expanding further towards the stars became a true reality. Of course, that feat has not been repeated after the original 6 lunar flights. Nowadays, there is a lot of talk in various space agencies about the possibility of sending a new mission to the moon again.



and finally

NASA's Galileo spacecraft imaged Europa during a flyby on September 7, 1996. In fact, so far there have only been flyby missions to this fascinating object. Galileo viewed Europa's surface much more closely than the Pioneers and Voyagers, and it revealed to astronomers a bizarre surface that looked like broken glass, repaired by an icy glue oozing up from below.

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Over the passage of billions of years, this ceaseless rain of falling objects have pulverized the lunar surface, creating fragments ranging in size from a fine powder to enormous, heavy boulders. Almost the entire lunar surface is literally blanketed by a pile of ground up rubble composed of charcoal gray, powdery dust and rocky debris collectively termed the lunar regolith. Beneath the regolith there is a region composed of shattered bedrock that is called the megaregolith.



Mars may be circled by many moons smaller than 160 to 330 feet in diameter, and a ring of dust has been predicted to circle Mars between Phobos and Deimos.



Following that last giant impact, Earth put on some weight, but this new weight gain was derived from impacts of much smaller bodies, only about the size of asteroids like Vesta. Dr. Jacobson and his team used the later weight gain in order to determine when the unfortunate Theia struck.

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