Inside Andromeda Galaxy M31 astronomers do it in the dark m31 the andromeda galaxy Andromeda Galaxy Inside M31

Inside Andromeda Galaxy M31 astronomers do it in the dark m31 the andromeda galaxy Andromeda Galaxy Inside M31

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A little interesting about space life.

Triton was the second moon in our Solar System that was found to have a substantial atmosphere, which is primarily composed of nitrogen--with smaller quantities of carbon monoxide and methane. Discovered by William Lassell in 1846, only seventeen days after the discovery of Neptune, Triton is one of the most frigid worlds in our Solar System, with a surface temperature of only about 38 Kelvin. Triton's frozen surface is coated by nitrogen, carbon dioxide, methane, and water ices, and it has a high geometric albedo of more than 70%. Surface features include a large southern polar cap, ancient cratered planes that are cross-cut by scarps and graben, as well as much younger features thought to have been formed by endogenic processes like cryovolcanism (ice volcanoes).

and here is another

Dr. Lieber and his colleagues did a study to test the theory of full-moon "lunacy". They studied data on murders in Dade County of Florida which covered 15 years and a total of 1,887 deaths by homicide. When they compared the deaths with the phases of the moon, they found that the two rose and fell together for the entire 15 years! With the approach of a full or new moon, there was a sharp spike in the murder rate, and then a decline during the first and last quarters of the moon.

and finally

Dr. Le Gall and her team used the newly acquired depth-sounding information in order to separate the contributions made to the sea's detected temperature by the liquid sea and the seabed, which provided new insights into their compositions.

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Earth's Moon is our planet's closest neighbor in space, but it is remarkable how even neighbors can keep secrets from each other. For years, astronomers thought that Earth's Moon was barren of water and other volatile compounds, but this notion began to change in 2008, when a team of planetary scientists announced that they had discovered small quantities of water imprisoned within volcanic glass beads, that astronauts had carried back to Earth from the Apollo 13 and 17 missions to our Moon. In 2011, additional research revealed extremely tiny crystalline formations within those beads--indicating that they contained quantities of water similar to some basalts on Earth.

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.

"The distribution of these water-rich deposits is the key thing. They're spread across the surface, which tells us that the water found in the Apollo samples isn't a one-off. Lunar pyroclastics seem to be universally water-rich, which suggests the same may be true of the mantle," Dr. Milliken continued to explain in the Brown University Press Release.