Evidence for Complex Molecules on Pluto's surface
Such chemical species can be produced by the interaction of sunlight or cosmic rays with Pluto's known surface ices, including methane, carbon monoxide and nitrogen.
The project, led by SwRI's Dr. Alan Stern, also included SwRI researchers Dr. John Spencer and Adam Shinn, and Nebraska Wesleyan University researchers Dr. Nathaniel Cunningham and student Mitch Hain.
"This is an exciting finding because complex Plutonian hydrocarbons and other molecules that could be responsible for the ultraviolet spectral features we found with Hubble may, among other things, be responsible for giving Pluto its ruddy color," said Stern.
The team also discovered evidence of changes in Pluto's ultraviolet spectrum compared to Hubble measurements from the 1990s. The changes may be related to differing terrains seen now versus in the 1990s, or to other effects, such as changes in the surface related to a steep increase in the pressure of Pluto's atmosphere during that same time span.
Pluto is not thought to be capable of supporting life, but studying the small, distant world can help scientists understand the diversity of rocky bodies in the Universe. Determining the composition of Pluto can also help astrobiologists catalog the many materials that occur naturally in our solar system. This information is important in understanding the types of molecules that could have been available for the origin of life on the early Earth.
This research was supported by a grant from the Space Telescope Science Institute.