Sagittarius A* -- The Milky Way Supermassive Black Hole

Abstract

This chapter provides a detailed overview of Sagittarius A* (Sgr A*), the supermassive black hole at the center of the Milky Way, located in the dense Galactic Center region approximately 8 kpc from Earth. Despite its relatively low activity compared to more luminous active galactic nuclei, Sgr A* has provided invaluable insights into black hole physics due to its proximity, enabling high-resolution observations of stellar orbits, gas dynamics, and variable emissions. In addition, Sgr A* illustrates how supermassive black holes influence galaxy evolution through energy feedback and matter redistribution. Early identification as a compact radio source and subsequent measurements of stellar orbits confirmed Sgr A* as a black hole with a mass near 4 million solar masses. Observations of stars moving on tight, short-period orbits around the black hole have allowed direct tests of general relativity, such as gravitational redshift and orbital precession, under the influence of extreme gravitational fields. Sgr A* displays variability across the electromagnetic spectrum, with flares in radio, infrared, and X-rays revealing complex interactions in the accretion flow, while outflows redistribute energy into the surrounding environment. Together, Sgr A* and its environment offer a crucial window into the behavior of galactic nuclei.