An article published in the journal “Nature Geoscience” describes a research in which a team of researchers argues that the signs of liquid water flows found on Mars are actually made up of dry sand. The possible existence of what are technically called RSLs (recurring slope lineae), streaks of sand washed by liquid water, was announced in September 2015 by NASA. A new study of data collected by NASA’s MRO (Mars Reconnaissance Orbiter) space probe may, however, show a different situation.
An article published in the journal “Nature” describes a research on the haze present in the atmosphere of the dwarf planet Pluto’s and its effects on its temperatures. According to a team led by Xi Zhang of the University of California at Santa Cruz, the haze absorb the already low heat from sunlight and emits infrared radiation cooling the atmosphere. That’s the explanation for the fact that NASA’s New Horizons space probe measured a temperature even lower than expected.
An article published in the journal “Nature Astronomy” describes a research that presents a possible explanation for the long-term existence of hydrothermal activities and an underground ocean of liquid water on Enceladus, one of Saturn’s moons. A team of researchers led by Gaël Choblet of the University of Nantes in France analyzed data collected by the Cassini space probe concluding that a porous core can be a key factor in generating heat for billions of years supporting an environment potentially favorable to life.
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.
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.