Southwest Research Institute
10/01/2024 | Press release | Distributed by Public on 10/01/2024 09:10
SwRI-led team discovers carbon dioxide and hydrogen peroxide on Pluto’s moon Charon
October 1, 2024 - A Southwest Research Institute-led team has detected carbon dioxide and hydrogen peroxide for the first time on the frozen surface of Pluto's largest moon, Charon, using observations from the James Webb Space Telescope. These discoveries add to Charon's known chemical inventory, previously identified by ground- and space-based observations, that includes water ice, ammonia-bearing species and the organic materials responsible for Charon's gray and red coloration.
"Charon is the only midsized Kuiper Belt object, in the range of 300 to 1,000 miles in diameter, that has been geologically mapped, thanks to the SwRI-led New Horizons mission, which flew by the Pluto system in 2015," said SwRI's Dr. Silvia Protopapa, lead author of a new Nature Communications paper and co-investigator of the New Horizons mission. "Unlike many of the larger objects in the Kuiper Belt, the surface of Charon is not obscured by highly volatile ices such as methane and therefore provides valuable insights into how processes like sunlight exposure and cratering affect these distant bodies."
The Webb telescope is an ideal platform for detailed exploration of Charon and other icy bodies in the region beyond the orbit of Neptune. In 2022 and 2023, the team used Webb's Near-Infrared Spectrograph to obtain four observations of the Pluto-Charon system. Different viewing geometries provided full coverage of Charon's northern hemisphere.
"The advanced observational capabilities of Webb enabled our team to explore the light scattered from Charon's surface at longer wavelengths than what was previously possible, expanding our understanding of the complexity of this fascinating object," said Dr. Ian Wong, a staff scientist at the Space Telescope Science Institute and co-author of the paper.
The extended wavelength coverage of Charon's Webb measurements reveals signatures of carbon dioxide. The team compared the spectroscopic observations with laboratory measurements and detailed spectral models of the surface, concluding that carbon dioxide is present primarily as a surface veneer on a water ice-rich subsurface.
"Our preferred interpretation is that the upper layer of carbon dioxide originates from the interior and has been exposed to the surface through cratering events. Carbon dioxide is known to be present in regions of the protoplanetary disk from which the Pluto system formed," Protopapa said.
The presence of hydrogen peroxide on the surface of Charon clearly indicates that the water ice-rich surface is altered by solar ultraviolet light and energetic particles from the solar wind and galactic cosmic rays. Hydrogen peroxide forms from oxygen and hydrogen atoms originating from the breakup of water ice due to incoming ions, electrons or photons.
"Laboratory experiments conducted at SwRI's CLASSE (Center for Laboratory Astrophysics and Space Science Experiments) facility were instrumental in demonstrating that hydrogen peroxide can form even in mixtures of carbon dioxide and water ice under conditions analogous to those at Charon," said SwRI's Dr. Ujjwal Raut, leader of CLASSE lab and second author of the paper.
The team's research showcases the Webb telescope's unparalleled capability to uncover complex surface signatures shaped by impacts and irradiation processes.
"The new insights were made possible by the synergy between Webb observations, spectral modeling and laboratory experiments and are possibly applicable to other similar midsized objects beyond Neptune," said Protopapa.
To access the Nature Communications paper, "Detection of carbon dioxide and hydrogen peroxide on the stratified surface of Charon with JWST," see DOI.
See also the 'Behind the Paper' post(link is external) from lead author Dr. Silvia Protopapa on the Springer Nature Research Communities webpage.
The data used in this work were acquired with the JWST/NIRSpec instrument through Program 1191 (PI: J. Stansberry).
For more information, visit Planetary Science or contact Deb Schmid, +1 210 522 2254, Communications Department, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78238-5166.