Solar gardening and the seasonal evolution of nitrogen ice on Triton and Pluto

被引:34
作者
Grundy, WM
Stansberry, JA
机构
[1] Lowell Observ, Flagstaff, AZ 86001 USA
[2] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
基金
美国国家航空航天局;
关键词
Pluto; Triton; surface evolution; volatile transport; ices;
D O I
10.1006/icar.2000.6510
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Nitrogen ice, probably the dominant high albedo surface material on Pluto and Triton, has optical constants that are more strongly absorbing in the thermal infrared than at visible wavelengths. This optical behavior results in absorption of sunlight, on average, at greater depths than the depths from which thermal emission emerges, producing a vertical imbalance between heating and cooling of a sunlit nitrogen ice surface. Assuming that the ice is sufficiently permeable to gas how that the bulk ice is in vapor pressure equilibrium with the nitrogen atmosphere, this vertical distribution of heating and cooling drives net sublimation at depth and condensation closer to the surface. Over time scales much shorter than seasonal time scales on Triton and Pluto, this process of solar gardening will tend to produce a characteristic textural and compositional distribution which has important photometric, spectroscopic, and seasonal consequences. Solar gardening may help explain several previously puzzling observations including the anomalously strong spectral absorption by methane ice in spectra of Triton and Pluto in the 0.7- to 1.1-mum range and the surprising persistence of Triton's south polar cap at low latitudes during southern summer. (C) 2000 Academic Press.
引用
收藏
页码:340 / 346
页数:7
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