An article published in the journal “Nature” describes research that has uncovered the place of origin of a Fast Radio Burst (FRB). These radio signals that last only a few milliseconds are picked up with no phenomenon that might warn about its arrival. An international team of astronomers used observations made by optical and radio telescopes to trace the origin of this phenomenon.
NASA announced the approval of a new astrophysics mission based on a space telescope called WFIRST (Wide-Field Infrared Survey Telescope). It’s a next-generation Instrument for a long-term project since it will be probably launched around the middle of next decade. It will have a mirror as large as Hubble’s but a field of view a hundred times wider to investigate even better on the secrets of the universe.
In Washington, D.C. a press conference was held to announce that the LIGO experiment found the gravitational waves predicted by Albert Einstein’s theory of general relativity. Two blacks holes about 1.3 billion light years from Earth merged as a result of a collision emitting those waves.
LIGO (Laser Interferometer Gravitational-Wave Observatory) is an instrument designed specifically to detect gravitational waves. It was created in a collaboration between Caltech (California Institute of Technology) and MIT (Massachusetts Institute of Technology) with funding from the American NFS (National Science Foundation).
An article published in the journal “Physical Review Letters” offers clues about the link between the internal structure of a galaxy cluster and the dark matter environment surrounding it. The study of dark matter is complex because it can only be done indirectly due to the fact that we can’t detect it directly. Until now, scientists believed that the greater the mass of a cluster the greater the amount of dark matter in its environment. This new research suggests that things are more complicated.
At the 227th meeting of the American Astronomical Society in Kissimmee, Florida there was a presentation of significant improvements that NASA obtained to the performance of its Fermi Gamma-ray Space Telescope. The data collected by its Large Area Telescope (LAT) instrument were analyzed again in what was called Pass 8 with a new software. That allowed to discover new gamma ray sources that previously weren’t identified. At the same time it was possible to improve the ability of the LAT to determine the direction of the incoming gamma rays.