text-only page produced automatically by LIFT Text Transcoder Skip all navigation and go to page contentSkip top navigation and go to directorate navigationSkip top navigation and go to page navigation
National Science Foundation
 
News
design element
News
News From the Field
For the News Media
Special Reports
Research Overviews
NSF-Wide Investments
Speeches & Lectures
NSF Current Newsletter
Multimedia Gallery
News Archive
News by Research Area
Arctic & Antarctic
Astronomy & Space
Biology
Chemistry & Materials
Computing
Earth & Environment
Education
Engineering
Mathematics
Nanoscience
People & Society
Physics
 

All Images


Press Release 08-093
Small Planet, Small Star

Newly discovered extrasolar planet is the smallest known and has smallest host star

Back to article | Note about images

Artist's conception of the newly discovered planet MOA-2007-BLG-192Lb orbiting its star.

Artist's conception of the newly discovered planet MOA-2007-BLG-192Lb orbiting a brown dwarf "star" with a mass of only 6 percent of that of the Sun. Theory suggests that the 3-Earth-mass planet is made primarily of rock and ice. Observational and theoretical studies of brown dwarfs reveal that they have a magenta color due to absorption by elements such as sodium and potassium in their atmospheres. If the host star has a mass of 9 percent of that of the Sun, at the other end of the margin of error for the new microlensing data, the star would be a red dwarf about 100 times brighter than the brown dwarf, but 1000 times fainter than the Sun.

Credit: NASA's Exoplanet Exploration Program


Download the high-resolution JPG version of the image. (2.9 MB)

Use your mouse to right-click (or Ctrl-click on a Mac) the link above and choose the option that will save the file or target to your computer.

Artist's conception of the newly discovered planet orbiting  a brown dwarf star.

View video
David Bennett, associate professor of physics at the University of Notre Dame, discusses the most recent extrasolar planet discovery using the microlensing method.

Credit: National Science Foundation / University of Notre Dame

 

Illustration of gravitational microlensing.

View video
This animation explains gravitational microlensing.

Credit: Trent Schindler, National Science Foundation

 

Illustration showing the signature distortion caused by gravity.

View video
This animation explains how gravitational microlensing detects planets.

Credit: Andrew Williams, University of Western Australia / Trent Schindler, National Science Foundation

 



Print this page
Back to Top of page
  Web Policies and Important Links | Privacy | FOIA | Help | Contact NSF | Contact Webmaster | SiteMap  
National Science Foundation
The National Science Foundation, 4201 Wilson Boulevard, Arlington, Virginia 22230, USA
Tel:  (703) 292-5111, FIRS: (800) 877-8339 | TDD: (800) 281-8749
Last Updated:
Oct 14, 2008
Text Only


Last Updated: Oct 14, 2008