Advanced Search
Astrobiology Magazine Facebook  Astrobiology Magazine Twitter
Extrasolar Life
These theoretical models plot a planet's size and mass given a certain
composition. Future observations might be able to distinguish a pure
water planet from a pure iron planet, but might have difficulty
distinguishing a carbon planet from a silicate planet, for example.
Click here to download an unlabeled version of this image.
Credit: Marc Kuchner/NASA GSFC.


Viewed:  977 times




About Us
Contact Us
Podcast Rss Feed
Daily News Story RSS Feed
Latest News Story RSS Feed
Learn more about RSS
Chief Editor & Executive Producer: Helen Matsos
Copyright © 2014,