"The center of the Milky Way is a messy place, full of stars and star remnants. There's so much going on that it's hard to observe in visible light, so precision measurements rely on radio, X-ray, or infrared (IR) wavelengths. Astronomers using the Keck telescope on Mauna Kea in Hawaii have been watching stars near the galactic center in IR for 17 years, providing a detailed view of their dynamics. The fruits of these observations include the measurement of the mass of the Milky Way's central black hole: approximately 4 million times the mass of the Sun. The Keck team, led by UCLA astronomer Andrea Ghez, has now identified a star that orbits the black hole in 11.5 years, the shortest orbital period for a star yet discovered. Thanks to this relatively quick motion, the astronomers have completely mapped the orbit of this star, known as S0-102, making it the second such star observed. Knowledge of complete orbits helps with modeling the black hole itself, which is invisible in IR light. While the data so far doesn't deviate from Newtonian gravity, observations over multiple orbits should allow for tests of general relativity in the region close to a black hole—something that hasn't been done yet using stellar orbits. THE DARKNESS AT THE GALAXY'S CENTER The central object in the Milky Way is known as Sagittarius A* (pronounced "ay star" and usually abbreviated Sgr A*). It lies approximately 25,000 light-years away from the Solar System in the region of the sky corresponding to the constellation of Sagittarius. While it is a relatively bright radio source, it's surprisingly faint in X-ray light compared to black holes of comparable sizes in other galaxies. Thanks to observations from the Keck/UCLA team and researchers at the Max Planck Institute for Extraterrestrial Physics in Germany, the mass of Sgr A* is known to be about 4 million times that of the Sun, while it occupies a smaller space than the Solar System. Only a black hole can be simultaneously so massive and so compact. Since 1995, researchers have mapped the motions of stars around the central black hole, using high-resolution IR images. At Keck, such imaging was facilitated by adaptive optics, wherein the shape of the 10-meter-diameter mirror was adjusted dynamically to correct for atmospheric distortion. With such techniques, astronomers were able to pinpoint the location and paths of a significant number of stars near the black hole, known as the S-stars. One of the earliest identified S-stars was S0-2, with an orbital period of about 16 years. Until the discovery of S0-102, it was the only star with a sufficiently short orbital period to enable a complete three-dimensional reconstruction of its trajectory, which provided the best data on the shape of the black hole's gravitational influence. The reason S0-102 evaded discovery is that it is faint—S0-2 is 16 times brighter. Because of its faintness, observations have suffered from "source confusion," where light from multiple objects mingles, affecting the appearance of the star. As a result, the astronomers used the black hole data from prior observations to determine S0-102's orbital properties, rather than using the star as a way to study the black hole itself." - Winckel