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A little interesting about space life.

With such intriguing results before them, the team of astronomers studied the data to determine if Kepler-22b actually has a moon. Unfortunately, their analysis reveals no evidence for the existence of an exomoon circling Kepler-22b. This non-detection suggests that the mass of any companion world around Kepler-22b must be less than 0.54 times the mass of our planet--with an impressive confidence rate of 95%! Therefore, it is very unlikely that Kepler-22b is circled by an Earth-like moon. Nevertheless, it is still too soon to give up hope. The Hunt for Exomoons with Kepler project has studied nine planetary systems in search of exomoons. Although none were detected, with the team's new results about the possibility of finding Earth-sized moons and the remaining treasure trove of Kepler data to sift through, large and possibly even habitable exomoons may start being spotted in the near future.



and here is another

For this reason, for many years astronomers considered the possibility that hydrocarbon lakes and seas might exist on this fantastic moon-world. Data that finally arrived courtesy of the joint NASA and European Space Agency's (ESA's) Cassini-Huygens mission lived up to their expectations. Since arriving at the Saturn system in 2004, the Cassini spacecraft has revealed more than 620,000 square miles of Titan's long-hidden, bewildering surface--and it has shown that almost two percent of Titan's entire surface is covered in liquid.



and finally

Titan possesses a smooth, young surface, scarred by comparatively few impact craters. The climate of this frigid moon--including its fierce winds and showers of hydrocarbon rain--carves out surface features that bear an eerie resemblance to those on Earth, such as lakes, sand dunes, rivers, seas, and deltas. Indeed, planetary scientists propose that Titan bears a haunting resemblance to Earth, and is believed to be similar to the way our planet was before life had a chance to evolve out of non-living substances (prebiotic).

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Dr. Alice Le Gall commented in the same JPL Press Release that "Before Cassini, we expected to find that Ligeia Mare would be mostly made up of ethane, which is produced in abundance in the atmosphere when sunlight breaks methane molecules apart. Instead, this sea is predominantly made of pure methane." Dr. Le Gall, a Cassini radar team associate, is of the French research laboratory LATMOS, in Paris, and lead author of the new study.



However, this did not prove to be the case. Instead, Cassini's measurements did not suggest any great difference in temperature between the surrounding shore and the methane sea over this span of time. This finding indicates that the terrains surrounding the lakes and seas on Titan are wet with liquid hydrocarbons, which would cause them to warm up and cool down in much the same way as the methane sea itself.



The researchers continued to explain that their scenario makes strong predictions for how the tortured, misty large moon Titan formed, what the icy mid-sized moons are made of, and how they began as rapidly spinning lumps of ice-laden material. The little moons could provide valuable clues that reveal to planetary scientists what happened in this mysterious outer region of our Solar System--as well as when it happened.