NASA has published a series of images taken by its Mars Rover Curiosity in the Gale Crater area of Mars called the Vera Rubin Ridge created putting together photos taken using filters that allow the mission scientists to identify some minerals. The instruments that have this capability are the MastCam (Mast Camera) and ChemCam (Chemistry and Camera). On this occasion, the MastCam allowed to highlight an iron oxide called hematite.
An article published in the magazine “Monthly Notices of the Royal Astronomical Society” describes the discovery of a hot Jupiter-type gas giant planet orbiting the star NGTS-1, a red dwarf. This is an extraordinary pair that’s in conflict with the current planetary formation models. The exoplanet NGTS-1b is the first to be discovered with the new Next Generation Transit Survey (NGTS) instrument installed at ESO’s Paranal Observatory in Chile.
An article published in the journal “Nature Astronomy” describes a research on the auroras on the planet Jupiter. A team of researchers used ESA’s XMM-Newton and NASA’s Chandra space telescopes to observe the pulsations of Jovian auroras. The study shows that the auroras pulsate independently at the two poles, unlike what happens on Earth.
The announcement of the discovery of a possible asteroid coming from another solar system is a big deal. Named as A/2017 U1, it was detected on October 19 by the Pan-STARRS 1 telescope in Hawaii, part of a sky observation system normally used to detect celestial bodies of various kinds. Its motion seems incompatible with the trajectories of asteroids and comets gravitationally bound to the Sun so it could be the first celestial body discovered that came from another star, perhaps Vega.
Two articles published in the journal “Monthly Notices of the Royal Astronomical Society” describe two researches on comet 67P/Churyumov-Gerasimenko based on data collected by ESA’s Rosetta space probe. In an article, a team led by Jürgen Blum of the Technische Universität Braunschweig, Germany, used the data collected to find out how the comet formed. In the other article, a team led by Jessica Agarwal of the Max Planck Institute for Solar System Research in Göttingen, Germany, described a plume on the surface of the comet that could have been generated by pressurized underground gas or by the crystallization of amorphous water ice.