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Interesting facts about space.

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.



and here is another

Last night there was a full moon. One of my dogs was very on edge, starting at every sound, staring out into the darkness at something I could neither hear nor see. The other 4 dogs were sound asleep. Did she sense something different about the moonlit night?



and finally

Neptune, the eighth major planet from the Sun, and its neighboring sister-planet, Uranus--the seventh planet from the Sun--are both classified as ice-giants because their large cores are icy, and they never managed to acquire the immense gaseous envelopes of the two true gas-giants, Jupiter and Saturn. The gas giants are possibly composed entirely of gas and liquid, although they may have small solid cores. In contrast, the ice-giants have large solid cores and thinner atmospheres. The two gas-giants, being mostly atmosphere, are very lightweight for their size. Saturn is the lightest planet in our Solar System, despite its immense diameter. In fact, Saturn is light enough to float like a huge raft in water, provided there was an ocean big enough for it to bob around in.

Other facts:

Europa, is a fascinating, frigid little world. It is one of the four Galilean moons, discovered in January 1610 by the great Galileo Galilei when he was gazing up into the night sky with his small, primitive "spyglass". The other Galilean moons, the weird sisters of Europa, are Io, Ganymede, and Callisto.



The crust of Earth's Moon is 43 miles thick on the near-side hemisphere, and 93 miles on the far-side. It is composed of silicon, magnesium, oxygen, calcium, aluminum, and iron. There are also trace amounts of titanium, uranium, thorium, hydrogen, and potassium.



In order to do precisely that, Dr. Li and Dr. Milliken used laboratory-based measurements of samples returned from the Apollo missions, combined with a detailed temperature profile of the areas of interest on the lunar surface. Using the new thermal correction, the two astronomers studied the data derived from the Moon Mineralogy Mapper, which is an imaging spectrometer that was carried aboard India's Chandrayaan-1 lunar orbiter.