2004 MN4 Apophis Asteroid is an asteroid apophis aka 2004 mn4 really going to hit Apophis MN4 Asteroid 2004
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University of Miami psychologist Arnold Lieber states a possible link between the fact that the human body is made up of nearly 80% water to the possibility that we experience "biological tides" effecting our emotions during different phases of the moon, the same as the oceanic tides are effected by the moon's activity.
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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.
A moon is a natural body that orbits a planet, and is held in its orbit by the force of both the host planet's gravity and the gravity of the moon itself. Some planets sport moons; some do not. Most of the moons dwelling in our Solar System are frigid (and sometimes weird) little worlds, made up of ice and rock, that swarm around the outer giant, gaseous planets of our Sun's bewitching family--Jupiter, Saturn, Uranus, and Neptune. One example of such bewitching weirdness is the frozen, little icy moon Hyperion, of the ringed-planet Saturn, that looks like an icy natural sponge.
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This model attempts to explain the distribution of moons circling giant, gaseous planets dwelling in the outer limits of our Solar System. However, it also provides an explanation for how the moons of planets such as our Earth and the dwarf planet, Pluto, were born. This research provides a valuable clue about how planetary systems developed throughout the entire Universe--not only in our own Solar System.
Saturn has 62 known moons. Most of them are very small, icy worldlets. On June 11, 2004, shortly before arriving at Saturn, the Cassini spacecraft made its only flyby--at an altitude of 2,000 kilometers--past the very tiny icy moon Phoebe. Phoebe is a heavily cratered worldlet that circles its planet backwards--indicating that it is a captured object, born elsewhere, and not an original member of Saturn's family.
Asphaug and co-author Dr. Andreas Reufer of the University of Bern in Switzerland, devised their new giant impact model using sophisticated computer simulations. They discovered that mergers between moons the size of Jupiter's Galilean satellites--which range in size from 1,940 miles wide (Europa) to 3, 271 miles across (Ganymede)--would tear icy stuff off the outer layers of the colliding moons. This icy material would then form spiral arms, which would ultimately merge together due to gravitational attraction to create Saturn's mid-sized icy moons.