Thursday, January 12, 2012
New evidence that will help to answer long-standing questions about the history of stars in the disk of our galaxy is being released this week at a meeting of the American Astronomical Society by a team that includes a Penn State astronomer. The research reveals some stars with orbits that take them to interesting places and that reveal interesting stories about how these stars were formed.
Donald Schneider, Head of Penn State's Department of Astronomy and Astrophysics, is one of the coauthors of the study. The study uses data from the Sloan Digital Sky Survey (SDSS), which has been mapping the stars in our galaxy for more than a decade. "The SDSS results are providing another window into the structure and history of our galaxy," said Schneider, who is the SDSS Survey Coordinator. More information is online at www.science.psu.edu/news-and-events/2012-news/Schneider1-2012. (more)
Wednesday, July 07, 2010
A wave of massive star formation appears poised to begin within a mysterious, dark cloud in the Milky Way. NASA's Spitzer Space Telescope has revealed a secluded birthplace for stars within a wispy, dark cloud named M17 SWex. The dark cloud is part of the larger, parent nebula known as M17, a vast region of our galaxy with a bright, central star cluster. "We believe we've managed to observe this dark cloud in a very early phase of star formation before its most massive stars have ignited," said Penn State astronomer Matthew Povich, a postdoctoral fellow and the lead author of a study published recently in The Astrophysical Journal Letters. The new research could shed light on the question of how and when massive stars form. (more)
Wednesday, April 07, 2010
A mysterious planet-like object orbiting a not-quite-starlike "brown dwarf" is the most recent enigma discovered by astronomers with their ever-more powerful telescopes. Kamen Todorov, a graduate student at Penn State, and a team of co-investigators including Kevin Luhman, assistant professor of astronomy and astrophysics at Penn State, used the keen eyesight of the Hubble Space Telescope and the Gemini observatory to directly image the planet-like object. The astronomers estimate that the smaller orbiting object is five to 10 times the mass of Jupiter and that it orbits at roughly the distance from the Sun to Saturn or Uranus, which makes it planet-like, but it formed only 1 million years ago -- much faster than the time some theories predict is needed to build a planet. The team's discovery, which resulted from a survey of 32 brown dwarfs in the Taurus star-forming region, will be published in the Astrophysical Journal. (more)
