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Автор Thompson, W. Reid
Дата выпуска 1989
dc.description Modeling of Triton's spectrum indicates a bright scattering layer of optical depth τ ≃ 3 overlying an optically deep layer of CH<sub>4</sub> with high absorption and little scattering. UV absorption in the spectrum indicates τ ≃ 0.3 of red‐yellow haze, although some color may also arise from complex organics partially visible on the surface. An analysis of this and other (spectro) photometric evidence indicates that Triton most likely has a bright surface, which was partially visible in 1977–1980. Geometric albedo p = 0.62<sub>−0.12</sub><sup>+0.18</sup>, radius r = 1480 ± 180km, and temperature T = 48 ± 6 K. With scattering optical depths of 0.3–3 and ∼ 1–10mb of N<sub>2</sub>, a Mars‐like atmospheric density and surface visibility pertain. Imaging with the 0.62 µm CH<sub>4</sub> filter of the Voyager 2 wide angle camera could show ∼20% contrast between the average surface and clean exposures of CH<sub>4</sub> ice (which is not limited to the polar caps). Low far‐infrared atmospheric opacity will in principle allow the detection of thermal gradients in the surface caused by optically transmitting but infrared opaque CH<sub>4</sub> and N<sub>2</sub> ice.
Формат application.pdf
Копирайт Copyright 1989 by the American Geophysical Union.
Тема Neptune Predictions
Тема Planetary Sciences: Solid Surface Planets
Тема Planetology: Solid Surface Planets and Satellites: Atmospheric composition and chemistry
Тема Planetology: Solid Surface Planets and Satellites: Composition
Тема Planetology: Solid Surface Planets and Satellites: Surfaces
Тема Planetary Sciences: Fluid Planets
Тема Planetology: Fluid Planets: Surfaces
Название Triton: Scattering models and surface/atmosphere constraints
Тип article
DOI 10.1029/GL016i008p00969
Electronic ISSN 1944-8007
Print ISSN 0094-8276
Журнал Geophysical Research Letters
Том 16
Первая страница 969
Последняя страница 972
Аффилиация Thompson, W. Reid; Center for Radiophysics and Space Research, Cornell University
Выпуск 8
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