Remarkable Flares From The Galactic Center

Sagittarius A* (Sgr A*), the supermassive black hole at the center of our Milky Way Galaxy, is 100 times closer to us than any other SMBH and therefore a prime candidate for studies of how matter radiates as it accretes onto black holes. SgrA* has been observed for decades and rapid fluctuations reported from X-ray to the near infrared wavelengths (intervening dust reduces optical light signals by a factor of over a trillion) and at submillimeter and radio wavelengths. Modeling the mechanisms of light variability is a direct challenge to our understanding of accretion onto SMBHs, but it is thought that correlations between flare timing at different wavelengths could reveal information about the spatial structure, for example if hotter material is located in a smaller zone closer to the black hole. One of the chief barriers to progress is the paucity of simultaneous multi-wavelength observations.

CfA astronomers Giovanni Fazio, Joe Hora, Steve Willner, Matt Ashby, Mark Gurwell and Howard Smith and a team of colleagues carried out a series of multiwavelength monitoring campaigns that included the IRAC camera onboard the Spitzer Space Telescope and the Chandra X-ray Observatory as well as the ground-based Keck telescope and the Submillimeter Array. Spitzer was able to monitor the black hole fluctuations continuously for 23.4 hours during each session, something that no ground-based observatory is capable of doing, and something that reliably enables scientists to spot slow trends (as distinct from short bursts).

Computational modeling of the emission from the vicinity of a black hole is a complex undertaking that among other things requires simulating how the material accretes, how it is heated and radiates, and (since all this happens close to a possibly rotating black hole) how general relativity predicts the radiation will appear to distant observers. Theorists suspect that shorter wavelength emission arises closer in and cooler emission farther out, with the former produced first and the latter subsequently. A time delay therefore might reflect the distance between these zones, and indeed previous sets of observations, some by this same team, did find evidence that hot, near-infrared flaring preceded the submillimeter flares seen by the SMA. In their new paper, the scientists report on two flares that apparently violate these and other previous patterns: the first event occurred simultaneously at all wavelengths; in the second event the X-ray, near-infrared and submillimeter flares all turned on within one hour of each other, not quite simultaneous but still unexpectedly close. The new observations will be extended with future simultaneous campaigns, and will help theorists refine their still quite speculative set of choices.

Author: Mitch Battros

Mitch Battros is a scientific journalist who is highly respected in both the scientific and spiritual communities due to his unique ability to bridge the gap between modern science and ancient text. Founded in 1995 – Earth Changes TV was born with Battros as its creator and chief editor for his syndicated television show. In 2003, he switched to a weekly radio show as Earth Changes Media. ECM quickly found its way in becoming a top source for news and discoveries in the scientific fields of astrophysics, space weather, earth science, and ancient text. Seeing the need to venture beyond the Sun-Earth connection, in 2016 Battros advanced his studies which incorporates our galaxy Milky Way - and its seemingly rhythmic cycles directly connected to our Solar System, Sun, and Earth driven by the source of charged particles such as galactic cosmic rays, gamma rays, and solar rays. Now, "Science Of Cycles" is the vehicle which brings the latest cutting-edge discoveries confirming his published Equation.