Astrophysicists using NASA's James Webb Space Telescope discovered constant flares from the accretion disk around the supermassive black hole at the center of the Milky Way.
Sagittarius A* is significant due to its mass equivalent to billions of suns and proximity, allowing for detailed observations of gas and dust flow.
Flares varying in duration and brightness were observed, with the black hole displaying continuous activity without a steady state.
Studying Sagittarius A* can provide insights into black hole behavior, interactions with surroundings, and galaxy evolution.
The team monitored the black hole over 48 hours using JWST's NIRCam, revealing ongoing fireworks with significant flares and sub-flares.
The unpredictability and randomness of the black hole's activity, including sudden bursts of brightness, were noted.
Minor disturbances within the accretion disk generate faint flickers, while longer and brighter flares are akin to tidal waves caused by significant events.
Events similar to solar flares and magnetic reconnection were observed, showcasing the extreme and energetic nature around black holes.
The team found a time delay in measurements at different wavelengths, providing insights into particle energy loss during flares.
Future studies aim to observe Sagittarius A* for longer periods using JWST to uncover finer details and potential periodicity in the flares.