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  • Our Galaxys Monster Black Hole Is Spinning Almost as Fast as . . .
    The colossal black hole lurking at the center of the Milky Way galaxy is spinning almost as fast as its maximum rotation rate That's just one thing astrophysicists have discovered after developing and applying a new method to tease apart the secrets still hidden in supermassive black hole observations collected by the Event Horizon Telescope
  • Monster black hole at Milky Way Galaxy’s core spinning at . . .
    Monster black hole at Milky Way Galaxy’s core spinning at physics’ speed threshold The study focused on two black holes — our galaxy's Sgr A* and M87*, located 55 million light-years away
  • Our Galaxys Monster Black Hole Is Spinning Almost As Fast As . . .
    The study of the black hole in our galaxy has taken years to analyze A large number of images were taken during an observing campaign in 2017, producing six terabytes of data These data had to be processed and analyzed – a process that took years, and the development of new algorithms to compensate for the rapid changeability
  • Record-Breaking Cosmic Structure Discovered in Colossal . . .
    In the center of the cluster, some of these features may be caused by a merger of two smaller galaxy clusters, or from outbursts produced by a supermassive black hole, or both Resources K Rajpurohit et al "Diffuse Radio Emission Spanning 6 Mpc in the Highly Disturbed Galaxy Cluster PLCK G287 0+32 9," pending submission
  • NASA’s Roman to Peer Into Cosmic ‘Lenses’ to Better Define . . .
    Gravitational lenses are made up of at least two cosmic objects In some cases, a single foreground galaxy has enough mass to act like a lens, magnifying a galaxy that is almost perfectly behind it Light from the background galaxy curves around the foreground galaxy along more than one path, appearing in observations as warped arcs and crescents
  • Our Galaxy - SKAO
    The SKA has the potential to make a tremendous impact on many key areas in Galactic Physics thanks to its transformative ability in wide-area, sensitive high angular resolution spectroscopy and its unparalleled astrometric measurements in line and continuum





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