Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.
about
Penitentes as the origin of the bladed terrain of Tartarus Dorsa on Pluto.Reorientation of Sputnik Planitia implies a subsurface ocean on Pluto.Reorientation and faulting of Pluto due to volatile loading within Sputnik Planitia.Untangling the methane chemistry in interstellar and solar system ices toward ionizing radiation: a combined infrared and reflectron time-of-flight analysis.The rapid formation of Sputnik Planitia early in Pluto's history.Corrigendum: Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.Recent tectonic activity on Pluto driven by phase changes in the ice shellWater and Volatiles in the Outer Solar System
P2860
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P2860
Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.
description
2016 nî lūn-bûn
@nan
2016 թուականի Յունիսին հրատարակուած գիտական յօդուած
@hyw
2016 թվականի հունիսին հրատարակված գիտական հոդված
@hy
2016年の論文
@ja
2016年論文
@yue
2016年論文
@zh-hant
2016年論文
@zh-hk
2016年論文
@zh-mo
2016年論文
@zh-tw
2016年论文
@wuu
name
Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.
@ast
Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.
@en
type
label
Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.
@ast
Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.
@en
prefLabel
Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.
@ast
Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.
@en
P2093
P2860
P50
P356
P1433
P1476
Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigour.
@en
P2093
A D Howard
J H Roberts
J R Spencer
New Horizons Geology, Geophysics and Imaging Theme Team
O M Umurhan
Oliver L White
P2507
P2860
P2888
P356
10.1038/NATURE18289
P407
P577
2016-06-01T00:00:00Z
P698
P818
1903.05571