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The sunlight that penetrates through the transparent crust helps the growth of vegetation in the caves to a substantial extent. However sunlight is not the main light source in the caves. The types of vegetation found in the moon are markedly different from the ones on earth. The plants commonly seen in the caves are quite short and look very much like the miniature trees, bushes and shrubs grown using Japanese "Bonsai" techniques.
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Using N-body simulations that model a recently snared Triton, and a likely primordial prograde system of moons, Dr. Rufu and Dr. Canup show that if the moons sport a mass ratio comparable to that of Uranus's system of moons or smaller, Triton's destructive dance with them has the tragic likelihood of reproducing the system that astronomers now observe. The simulations even demonstrate that the interactions decrease Triton's original semi-major axis rapidly enough to to stop smaller, outer moons like Nereid from being unceremoniously evicted from the system.
The team also considered whether it would be possible to determine, with an adequate degree of certainty, if a detected moon could bear life-loving liquid water. In their analysis, the "input" climate for the moon is habitable, which is identified with high probability. However, there still remains approximately a one in six failure rate.
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Dr. Le Gall and her team used the newly acquired depth-sounding information in order to separate the contributions made to the sea's detected temperature by the liquid sea and the seabed, which provided new insights into their compositions.
Ever since their discovery in 1877, Phobos and Deimos have both bewildered and bewitched astronomers trying to answer the question of how Mars ended up with its duo of misshapen little moons. However, this perplexing riddle might have been solved by a multidisciplinary study conducted by French, Belgian, and Japanese scientists.
Planetary scientists usually calculate the Moon's age by using the radioactive decay of elements like uranium, explained Dr. John Chambers in the April 2, 2014 National Geographic News. Dr. Chambers is a planetary scientist at the Carnegie Institution for Science in Washington, D.C. By studying an element with a recognized decay rate, and knowing its concentration in Moon rocks or the Earth's surface, scientists are able to calculate back in time to when the material first formed. However, there are numerous and varying radioactive materials that can provide differing timelines, added Dr. Chambers, who was not involved in the study.