su201736

The Mass of the Milky Way
Friday, September 1, 2017
Science Update - A look at CfA discoveries from recent journals

The physical properties of the Milky Way, our home galaxy, and its evolutionary history are keys to understanding the history of galaxy formation across the cosmos, and details like the efficiency of converting atoms into stars, the development of satellite galaxies like the Magellanic Clouds, and more. One parameter, the total mass of the Milky Way, is particularly relevant but still quite uncertain. It is difficult to measure not only because we lie deep in the innards of the galaxy itself, but also because most of the mass is in the form of dark matter that does not radiate. Current estimates of the galaxy’s total mass are based on the motions of tidal streamers of gas and globular clusters, both influenced by the gravitational mass of the galaxy, and range from one to several trillion solar-masses.

CfA astronomer Avi Loeb and his colleague have come up with a novel and effective way of estimating the Milky Way’s total mass: modeling the motions of hypervelocity stars, stars that are thought to be ejected from the galaxy as a result of interactions of binary stars with the supermassive black hole at our galaxy’s center. More than twenty of these stars have been found so far, moving at velocities of up to 700 kilometers/second and located at distances more than one hundred and fifty thousand light-years from the galactic center. While the exact mechanism for producing these stars is still debated, their orbits are completely determined by the gravitational field of the galaxy, which can be deduced.

The astronomers adopt a nominal travel time for these observed hypervelocity stars of three hundred and thirty million years, which corresponds to their average lifetime burning hydrogen fuel. Combined with other kinematic information about these stars, the scientists calculate that the mass of the galaxy is between 1.2 and 1.9 trillion solar masses, adding significant precision to the previous estimates.

Reference(s): 

"Constraining Milky Way Mass with Hypervelocity Stars," G. Fragione and A. Loeb, A&A, in press (2017).