In the course of the Conference of the American Astronomical Society’s 49th Division for Planetary Sciences Meeting, SwRI (Southwest Research Institute) scientist Simone Marchi presented the results of a study on the origin of the organic compounds discovered on the dwarf planet Ceres by NASA’s Dawn space probe. There were some doubts about the possibility they had formed on Ceres but according to Marchi and his team the evidence they collected that’s the most likely theory.
During the American Astronomical Society Division for Planetary Science meeting some of the latest discoveries were presented about the planet Saturn and its rings obtained from data collected by the Cassini space probe before disintegrating in the planet’s atmosphere on September 15. Some of the results were published in “The Astrophysical Journal”.
An article published in the journal “Nature Communications” describes the discovery of evidence of the existence of very ancient hydrothermal deposits on a seabed in the Eridania region on Mars. A team of researchers studied data collected by NASA’s Mars Reconnaissance Orbiter (MRO) space probe to reconstruct the presence of massive deposits in a basin in the red planet’s southern hemisphere. It’s a type of environment favorable to the birth of life forms, similar to that in which scientists think life on Earth was born.
ESA has released the last image taken by its Rosetta space probe before clashing on the surface of comet 67P/Churyumov-Gerasimenko at the end of its mission along with the story of its reconstruction. The image was incomplete, so initially it wasn’t recognized as such by the automatic processing software among the packets containing telemetry data it was transmitted with.
An article published in the magazine “Icarus” describes a research that offers an explanation for the origin ice blades that are tens of meters high found on Pluto. According to a team of researchers led by Jeffrey Moore, one of NASA’s New Horizons mission scientists, those blades originated in the freezing and subsequent erosion of methane at the highest altitudes of the dwarf planet, with a process similar to what happens on the Earth, for example on the Andes, but with much larger sizes.