Evidence for a molecule heavier than methane in the atmosphere of Pluto
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Charon's radius and atmospheric constraints from observations of a stellar occultation.Haze heats Pluto's atmosphere yet explains its cold temperature.Pluto's lower atmosphere structure and methane abundance from high-resolution spectroscopy and stellar occultationsHigh resolution spectroscopy of Pluto’s atmosphere: detection of the 2.3 μm CH4bands and evidence for carbon monoxide
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Evidence for a molecule heavier than methane in the atmosphere of Pluto
description
article publié dans la revue scientifique Nature
@fr
scientific article published in Nature
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wetenschappelijk artikel
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наукова стаття, опублікована в Nature в травні 1989
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name
Evidence for a molecule heavier than methane in the atmosphere of Pluto
@en
Evidence for a molecule heavier than methane in the atmosphere of Pluto
@nl
type
label
Evidence for a molecule heavier than methane in the atmosphere of Pluto
@en
Evidence for a molecule heavier than methane in the atmosphere of Pluto
@nl
prefLabel
Evidence for a molecule heavier than methane in the atmosphere of Pluto
@en
Evidence for a molecule heavier than methane in the atmosphere of Pluto
@nl
P356
P1433
P1476
Evidence for a molecule heavier than methane in the atmosphere of Pluto
@en
P2093
Jonathan I. Lunine
Roger V. Yelle
P2888
P304
P356
10.1038/339288A0
P407
P577
1989-05-01T00:00:00Z
P6179
1021268765