about
The formation of Charon's red poles from seasonally cold-trapped volatiles.Surface compositions across Pluto and Charon.Observed glacier and volatile distribution on Pluto from atmosphere-topography processes.Reorientation and faulting of Pluto due to volatile loading within Sputnik Planitia.The rapid formation of Sputnik Planitia early in Pluto's history.Planetary science: Haze cools Pluto's atmosphere.Haze heats Pluto's atmosphere yet explains its cold temperature.Pluto's interaction with its space environment: Solar wind, energetic particles, and dust.Photochemistry on Pluto: part II HCN and nitrogen isotope fractionationImpacts of Cosmic Dust on Planetary Atmospheres and SurfacesAtmospheric escape from unmagnetized bodiesWeird and wonderful Pluto spills its secrets
P2860
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P2860
description
2016 nî lūn-bûn
@nan
2016年の論文
@ja
2016年学术文章
@wuu
2016年学术文章
@zh
2016年学术文章
@zh-cn
2016年学术文章
@zh-hans
2016年学术文章
@zh-my
2016年学术文章
@zh-sg
2016年學術文章
@yue
2016年學術文章
@zh-hant
name
The atmosphere of Pluto as observed by New Horizons.
@en
The atmosphere of Pluto as observed by New Horizons.
@nl
type
label
The atmosphere of Pluto as observed by New Horizons.
@en
The atmosphere of Pluto as observed by New Horizons.
@nl
prefLabel
The atmosphere of Pluto as observed by New Horizons.
@en
The atmosphere of Pluto as observed by New Horizons.
@nl
P2093
P2860
P50
P356
P1433
P1476
The atmosphere of Pluto as observed by New Horizons.
@en
P2093
Alex H Parker
Andrew F Cheng
Andrew J Steffl
Constantine C C Tsang
Darrell F Strobel
David C Slater
David P Hinson
Eliot F Young
Eric Schindhelm
G Leonard Tyler
P2860
P304
P356
10.1126/SCIENCE.AAD8866
P407
P577
2016-03-01T00:00:00Z
P698
P818
1604.05356