Two articles, one published in the journal “Astronomy & Astrophysics” and one in the journal “Nature Astronomy”, describe two researches on the TRAPPIST-1 system’s rocky planets. Various telescopes, both space and ground-based, allowed to gather more information on those 7 exoplanets and to improve the measurements of their characteristics. An important result is the estimate of their density, which suggests that some of them are composed up to 5% of water. Spectroscopic detections suggest that at least 3 of them have a compact atmosphere that could allow liquid water to exist on their surface.
An article published in the journal “The Astrophysical Journal Letters” describes the detection of hot cores and the most complex molecules detected outside the Milky Way in the Large Magellanic Cloud, one of the Milky Way’s satellite dwarf galaxies. A team led by astronomer Marta Sewilo of NASA’s Goddard Space Flight Center used the ALMA radio telescope to conduct those measurements that contradict previous observations in what was considered a chemically primitive galaxy.
An article published in the journal “The Astrophysical Journal” describes the most accurate measurement of the characteristics of the ultra-cold dwarf star TRAPPIST-1. A team led by astronomer Valérie Van Grootel of the University of Liège in Belgium used new observations and analysis techniques to refine the measurements of TRAPPIST-1. It’s become the subject of a lot of research after the confirmation in February 2017 that 7 rocky planets orbit this tiny star and knowing its characteristics with precision helps to study the whole system.
An article published in the journal “Nature Astronomy” describes a research that provides a way to use methanol to measure magnetic fields existing in space. A team of researchers led by Boy Lankhaar of the Chalmers Univerisity in Gothenburg, Sweden, studied the properties of methanol to use it in the calculation of magnetic fields that play an important role in the formation of massive stars.
An article to be published in the journal “Monthly Notices of the Royal Astronomical Society” describes the study of the supernova ASASSN-15no. A team of astronomers, especially from the National Institute of Astrophysics in Padua, Italy, led by Stefano Benetti used a number of telescopes to observe an explosion that was initially hidden by a thick layer of gas and dust ejected by the progenitor star a few years before. For this reason, the astronomers have called it a supernova that plays hide and seek but in the end it popped out and was at least ten times brighter than normal.