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Surface compositions across Pluto and Charon
- Source :
- Science, Science, 2016, 351, ⟨10.1126/science.aad9189⟩
- Publication Year :
- 2016
-
Abstract
- The New Horizons spacecraft mapped colors and infrared spectra across the encounter hemispheres of Pluto and Charon. The volatile ices CH$_4$, CO, and N$_2$, that dominate Pluto's surface, have complicated spatial distributions resulting from sublimation, condensation, and glacial flow acting over seasonal and geological timescales. Pluto's H$_2$O ice "bedrock" is also mapped, with isolated outcrops occurring in a variety of settings. Pluto's surface exhibits complex regional color diversity associated with its distinct provinces. Charon's color pattern is simpler, dominated by neutral low latitudes and a reddish northern polar region. Charon near infrared spectra reveal highly localized areas with strong NH$_3$ absorption tied to small craters with relatively fresh-appearing impact ejecta.<br />Comment: in Science 351, aad9189 (2016)
- Subjects :
- 010504 meteorology & atmospheric sciences
Outcrop
FOS: Physical sciences
01 natural sciences
Charon
Astrobiology
Latitude
Impact crater
0103 physical sciences
Glacial period
Ejecta
010303 astronomy & astrophysics
0105 earth and related environmental sciences
Physics
Earth and Planetary Astrophysics (astro-ph.EP)
Pluton
geography
Multidisciplinary
geography.geographical_feature_category
Bedrock
Pluto
Surface
New Horizons mission
composition
[SDU]Sciences of the Universe [physics]
Protoplanet
Astrophysics - Earth and Planetary Astrophysics
Subjects
Details
- ISSN :
- 10959203 and 00368075
- Volume :
- 351
- Issue :
- 6279
- Database :
- OpenAIRE
- Journal :
- Science (New York, N.Y.)
- Accession number :
- edsair.doi.dedup.....bb6770bfc799ba2b8fdf7ab91228e94d
- Full Text :
- https://doi.org/10.1126/science.aad9189⟩