spitzer_ssc2005-06a July 2nd, 2004
Credit: NASA/JPL-Caltech/K. Luhman (Harvard-Smithsonian CfA)
This graph of data from NASA's Spitzer Space Telescope shows that an extraordinarily low-mass brown dwarf, or "failed star," is circled by a disk of planet-building dust. The brown dwarf, called OTS 44, is only 15 times the mass of Jupiter, making it the smallest known brown dwarf to host a planet-forming disk.
Spitzer was able to see this unusual disk by measuring its infrared brightness. Whereas a brown dwarf without a disk (red dashed line) radiates infrared light at shorter wavelengths, a brown dwarf with a disk (orange line) gives off excess infrared light at longer wavelengths. This surplus light comes from the disk itself and is represented here as a yellow dotted line. Actual data points from observations of OTS 44 are indicated with orange dots. These data were acquired using Spitzer's infrared array camera.
Provider: Spitzer Space Telescope
Image Source: http://www.spitzer.caltech.edu/images/1394-ssc2005-06a-Planetary-Building-Blocks-Found-in-Surprising-Place
Curator: Spitzer Space Telescope, Pasadena, CA, USA
Image Use Policy: http://www.spitzer.caltech.edu/info/18-Image-Use-Policy
Detailed color mapping information coming soon...
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