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Frozen surfaces of small bodies in the outer Solar System are exposed to cosmic and solar energetic ions. Thanks to laboratory experiments, scientists from the “Astrochemistry and Origins” team at IAS and the Florida Space Institute (USA) estimated the alterations induced by ion irradiation on the methanol-rich surfaces of such objects.
The Planck collaboration has just published its last series of articles, for a total of 164. These papers have been cited more than 90,000 times, which demonstrates the long lasting influence of this experiment for cosmology, including the study of the mass of neutrinos, the density of dark matter, the characteristics of primordial fluctuations, the formation and evolution of galaxies and clusters or even the magnetic field of the Milky Way.
The first images from ESA’s new Sun-observing spacecraft Solar Orbiter have just been released. Solar Orbiter, launched on 10 February, completed its commissioning phase in mid-June and performed its first close approach to the Sun. Shortly thereafter, the European and US science teams behind the mission’s 10 instruments were able to test the entire instrument suite in concert for the first time.
Despite the drastic constraints driven by the sanitary limitations to technical activities at IAS, and the travel ban to Japan, the MicrOmega team at IAS managed to thoroughly develop, test, and calibrate the MicrOmega instrument, and to deliver it to the curation facility of the Hayabusa2 at ISAS, the Japanese Institute of Space and Astronautical Science, on Friday July 3, 2020, after its performances had been demonstrated as excellent.
Although there are evidences of relationships between the most primitive bodies of the solar system and differentiated planetary bodies with a metallic core, no sample has been found up to now that bears information on the onset of planetary differentiation. Researchers have recently described a volcanic rock produced by extremely limited partial melting of a parent body chemically similar to the most primitive meteorites (carbonaceous chondrites) and crystallized upon ascent toward the surface of the body. This sample proves that some carbonaceous bodies from the outer solar system are partially differentiated and is the missing link in a continuum between comets and iron meteorites from metallic planetary cores.
