Mouse Mars Rover giant mouse found on mars life on mars confirmed with Mars Rover Mouse

Mouse Mars Rover giant mouse found on mars life on mars confirmed with Mars Rover Mouse

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Curious facts about cosmic life and their inhabitants.

The temperatures around the equatorial and mid latitude surface at daytime and in the night are around 225oF and minus 298oF respectively. As the moon day is approximately 28 earth days, heating and cooling of the moon's surfaces affects the inside cave temperature significantly. The temperature difference in the opposite side of the moon makes the air in the cave move from one area to the other creating complex wind movements. When high speed wind flows across the vertical rock structures, it makes gurgling sounds in the caves, resulting in eerie or weird echo effects. The blowing wind helps to mitigate the high humidity conditions.



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The lakes are the main supporting source sustaining life in the moon. The lakes support an array of living organisms including fish of various varieties and some small sized aquatic mammals also, like on the earth. Only a limited range of water plants grow in the lakes and these are all found in all the lakes in the moon. The most abundant water plant variety resembles seaweeds, but is very much thicker and stronger than the earth's variety. These water plants which grow very rapidly and proliferate in vast quantities are the primary source of food and nutrient for the moon people.



and finally

Kepler-22b's initial transit in front of the face of its fiery star was seen by Kepler on its third day of scientific observations, back in May 2009. The third passage was spotted in late 2010. Still more confirming evidence was provided by the infrared Spitzer Space Telescope, as well as by ground-based 'scopes. The confirmation of the existence of this interesting extrasolar planet world was announced on December 5, 2011.

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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 most detailed pictures of Europa show even more intriguing clues that there is slush lurking beneath its brightly shining icy surface. Slightly smaller than Earth's own beloved Moon, Europa's surface temperature could easily freeze an ocean solid over a span of only several million years. However, some astronomers think that warmth from a game of tidal tug-of-war between Europa and Jupiter, as well as other neighboring moons, could be keeping large regions of Europa's subsurface global ocean in a life-friendly liquid state. This process is termed tidal heating, and it refers to a mechanism whereby the gravitational tugs of a nearby object (or objects) flex and bend and contract and expand another object continually. This constant churning causes the victimized object, in this case Europa, to heat up and be considerably more balmy than its great distance from the Sun would otherwise allow it to be.



Mars hasn't always looked the way it does today. The planet suffered a monumental tilt billions of years ago. Before this great tilt occurred, the Martian poles were not where we see them now.