astroengine writes: "A new analysis of recent observations finds evidence for a protoplanetary disk around a red dwarf star plunging in the direction of the supermassive black hole at the center of our galaxy. Ruth Murray-Clay and Avi Loeb of the Harvard-Smithsonian Center for Astrophysics did the theoretical work. Stefan Gillessen of the Max-Planck-Institute for Extraterrestrial Physics made the observations using the European Southern Observatory's Very Large Telescope. The red dwarf star will make its closest approach in the summer of 2013, hurtling only 270 billion miles from black hole. (Or roughly 54 solar system diameters, as measured from the furthest edge of the Kuiper belt.) It won't get sucked into the black hole, but it will be flung back along its elliptical orbit out to a distance of a little more than 1/10 light-years."