Black hole hair would change how such objects
orbit near the hole, and these changes could be detectable by telescopes that will come online within the next decade.
Not exact matches
Scientists can also do reverberation mapping, which uses X-ray telescopes to look for time differences between emissions from various locations
near the black
hole to understand the
orbits of gas and photons around the black
hole.
The
orbit of S0 - 2 (light blue) located
near the Milky Way's supermassive black
hole will be used to test Einstein's Theory of General Relativity and generate potentially new gravitational models.
Most stars
near the center manage to stay out of the clutches of the
hole, though, simply by virtue of being in ultrafast
orbits around it.
In the new study, Charles Hailey, an astrophysicist at Columbia University, and his colleagues scrutinized the past dozen years of data gathered by the Chandra X-ray Observatory, an
orbiting craft whose instruments are designed to detect high - energy radiation emitted by the immensely hot material surrounding exploded stars and
near black
holes.
The
orbits of two stars, S0 - 2 and S0 - 38 located
near the Milky Way's supermassive black
hole will be used to test Einstein's theory of General Relativity and potentially generate new gravitational models.
Ghez used this cutting - edge system to track the
orbits of stars
near the supermassive black
hole located at the center of the Milky Way.
By measuring the rapid
orbits of the stars
near the center of our galaxy, Dr. Ghez and her colleagues have moved the case for a supermassive black
hole at the heart of the Milky Way from a possibility to a certainty.
An image from W. M. Keck Observatory
near infrared data shows that G2 survived its closest approach to the black
hole and continues happily on its
orbit.