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Kepler-22b sports an orbital period of approximately 200 days. Its inclination is about 90 degrees, and it transits in front of the face of its star as observed by Earth-based astronomers. The shape of Kepler-22b's orbit is unknown, but it is known that its average orbital distance is well within its parent star's habitable zone. Many extrasolar planets are known to sport highly elliptical (football-shaped) orbits, and if Kepler-22b also travels along such a path around its star, it would only spend a tiny fraction of its time within this Goldilocks zone. This would cause the planet to undergo such extreme variations in temperature that it would not be a pleasant place for delicate living things to evolve and flourish. Kepler-22b is approximately 2.4 times the radius of Earth.
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The new study is based on data gathered by Cassini's radar instrument during flybys of Titan between 2007 and 2015.
The "chaos terrains" are those regions of the icy moon that are covered with shattered, scrambled, and rotated chunks of crust the size several city blocks. Galileo images show swirly and very rough-looking material between the broken blocks of ice, which indicates that the blocks may once have been lodged atop a bed of slushy stuff that ultimately froze at the very frigid surface temperatures of Europa.
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There probably are many more lakes under Europa's ice, Blankenship continued to note. Furthermore, the prospects of searching for life on Europa could greatly improve. This is because research indicates that a percentage of the icy lids that cover the embedded lakes may be considerably thinner than was previously supposed.
This later-forming time line for lunar birth is reasonable, Dr. William Hartmann noted in the April 2, 2014 National Geographic News. Dr. Hartmann, a researcher at the Planetary Science Institute in Tucson, Arizona, was one of the first to propose the giant impact theory of lunar formation. However, he added that the new study might depend too much on the idea of using the last giant impact as a marker for when such events occurred in the history of our planet.
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.