An article published in the journal “Nature Physics” describes the study conducted on the supermassive black hole known as PKS 1830-211 using observations made with ESA’s Integral and NASA’s Fermi and Swift space telescopes. The peculiarity is that these observations used a gravitational lensing effect created by a galaxy to explore the inner regions of the area around the black hole and the gamma rays that come from it.
Astronomy / Astrophysics
In the journal “Nature Communications” an article was published on the study of images of the planet Venus taken during its transit, its passage between the Sun and the Earth, which occurred in June 2012, taken by two satellites: NASA’s SDO and NASA and JAXA’s Hinode. This research allowed to look at Venusian atmosphere in a different way measuring the way it absorbs the different types of light. This type of study allows to get important clues about the presence of various chemical elements in the atmosphere’s layers. It will also be useful to improve the techniques to examine exoplanets’ atmosphere.
An article published in “Nature” describes the research conducted by an international team led by Jochen Greiner of the Max-Planck-Institut für extraterrestrische Physik, Garching, Germany who studied a gamma-ray burst (GRB) detected on December 9, 2011 by NASA’s Swift satellite and called GRB 111209A. It was an exceptional phenomenon because it lasted more than three hours when gamma-ray bursts typically last from a few seconds to a few minutes. It was the first case of GRB associated with a supernova, called SN 2011kl, which produced a magnetar, a neutron star with an incredibly strong magnetic field.
Yesterday at the Royal Astronomical Society’s National Astronomy Meeting (NAM2015), at the Venue Cymru centre in Llandudno, Wales, evidence were presented of the discovery of supermassive black holes found thanks to the NASA’s NuSTAR (Nuclear Spectroscopic Telescope Array) space telescope. An international team led by astronomers at the British Durham University detected the high energy X-ray emission from five black holes that were previously hidden by dust and gas.
An article published in the journal “Nature” describes a research on a series of 18 pits on the comet 67P/Churyumov-Gerasimenko. They are nearly circular and some of them are a source of activity, emitting jets of gas and dust. They were discovered a long time ago but an analysis of the images collected by ESA’s space probe Rosetta’s OSIRIS camera allowed to establish that probably they were formed following a collapse of the surface.