Large changes in Pluto's atmosphere as revealed by recent stellar occultations

Sicardy B.; Widemann T.; Lellouch E.; Veillet C.; Cuillandre, JC; Colas, F; Roques F.; Beisker W.; Kretlow M.; Lagrange, AM; Gendron, E; Lacombe, F; Lecacheux J.; Birnbaum, C.; Fienga, A; et. al.

Abstract

Pluto's tenuous nitrogen atmosphere was first detected by the imprint left on the light curve of a star that was occulted by the planet in 1985 (ref. 1), and studied more extensively during a second occultation event in 1988 (refs 2-6). These events are, however, quite rare and Pluto's atmosphere remains poorly understood, as in particular the planet has not yet been visited by a spacecraft. Here we report data from the first occultations by Pluto since 1988. We find that, during the intervening 14 years, there seems to have been a doubling of the atmospheric pressure, a probable seasonal effect on Pluto.

Más información

Título según WOS: Large changes in Pluto's atmosphere as revealed by recent stellar occultations
Título según SCOPUS: Large changes in Pluto's atmosphere as revealed by recent stellar occultations
Título de la Revista: NATURE
Volumen: 424
Número: 6945
Editorial: NATURE PORTFOLIO
Fecha de publicación: 2003
Página de inicio: 168
Página final: 170
Idioma: English
URL: http://www.nature.com/doifinder/10.1038/nature01766
DOI:

10.1038/nature01766

Notas: ISI, SCOPUS