[LINK] "Galaxy Grande: Milky Way May Be More Massive Than Thought"
Scientific American's Ken Croswell reports on yet another amazing feat of modern astronomy: measuring the mass of our Milky Way Galaxy through painstakingly charting the motion of one of its dwarf satellites.
Although scientists know the masses of the sun and Earth, it's a different story for the galaxy. Mass estimates range widely: At the low end, some studies find that the galaxy is several hundred billion times as massive as the sun whereas the largest values exceed two trillion solar masses. Astronomers would have an easier task if the galaxy consisted solely of stars. But a huge halo of dark matter engulfs its starry disk and vastly outweighs it. Now remarkable observations of a small galaxy orbiting our own have led to a new number.
In studies of the Milky Way's mass one little galaxy plays an outsize role: Leo I. "The value of Leo I is twofold," says Michael Boylan-Kolchin of the University of California, Irvine. "It's both very distant and moving quite quickly." Discovered in 1950 and located 850,000 light-years from the Milky Way's center, Leo I is a dwarf spheroidal galaxy and the farthest of the many galaxies that are thought to orbit our own. Most of the Milky Way's dark matter halo should fit inside Leo I's orbit—that is, if the dwarf galaxy is actually in orbit and not just passing by.
Astronomers know from Leo I's Doppler shift that it is racing away from us. If the Milky Way has enough mass, its gravity will hold it in orbit. Moreover, astronomers would be able to observe the motion of Leo I and use it to deduce the Milky Way's total mass—including its dark matter halo—out to the dwarf galaxy's great distance. But if the Milky Way does not have enough mass, Leo I will fly away, its high speed revealing little of consequence.
To deduce Leo I's path through space, astronomers have to determine the small galaxy's precise motion. The Doppler shift reveals Leo I's velocity along our line of sight, but no one knew how fast the little galaxy was moving across it. Determining that requires measuring its proper motion—the change in the galaxy's position from one year to the next. Proper motion is easy to gauge for a nearby star but difficult to measure for another galaxy, because far-off objects have tiny proper motions.
Sangmo Tony Sohn of the Space Telescope Science Institute and his colleagues therefore used the Hubble Space Telescope to compare Leo I's position in 2006 and 2011 with more than a hundred background galaxies. In work submitted to The Astrophysical Journal, Sohn's team reports success: the first proper motion measurement of Leo I.
[. . .]
Combined with the Doppler shift, the proper motion reveals that Leo I orbits the Milky Way at 200 kilometers per second. By comparison, that's nearly as fast as the sun orbits the Milky Way's center, even though the dwarf galaxy is much farther away. Says Boylan-Kolchin, "To sustain a similar velocity at that far a distance requires a lot of extra mass."
How much mass? In a companion study Boylan-Kolchin and his colleagues simulate how giant galaxies such as the Milky Way grow by swallowing lesser galaxies, finding that dwarf galaxies moving as fast as Leo I are almost always bound to the giants, which means Leo I is a true satellite. His team then derives a mass for the Milky Way of 1.6 trillion suns.