Pluto's Haze as a Surface Material
W.M. Grundy, T. Bertrand, R.P. Binzel, M.W. Buie, B.J. Buratti, A.F., Cheng, J.C. Cook, D.P. Cruikshank, S.L. Devins, C.M. Dalle Ore, A.M. Earle,, K. Ennico, F. Forget, P. Gao, G.R. Gladstone1, C.J.A. Howett, D.E. Jennings,, J.A. Kammer, T.R. Lauer, I.R. Linscott, C.M. Lisse

TL;DR
This paper investigates how atmospheric haze deposits influence Pluto's surface appearance, proposing that regional differences in color and geology result from local interactions or non-uniform haze supply.
Contribution
It introduces a model for haze deposition on Pluto and suggests mechanisms for regional color differences involving local interactions or variable haze supply.
Findings
Haze accumulates differently across Pluto's regions.
Color differences may result from local chemical interactions.
Haze supply may be non-uniform over time and space.
Abstract
Pluto's atmospheric haze settles out rapidly compared with geological timescales. It needs to be accounted for as a surface material, distinct from Pluto's icy bedrock and from the volatile ices that migrate via sublimation and condensation on seasonal timescales. This paper explores how a steady supply of atmospheric haze might affect three distinct provinces on Pluto. We pose the question of why they each look so different from one another if the same haze material is settling out onto all of them. Cthulhu is a more ancient region with comparatively little present-day geological activity, where the haze appears to simply accumulate over time. Sputnik Planitia is a very active region where glacial convection, as well as sublimation and condensation rapidly refresh the surface, hiding recently deposited haze from view. Lowell Regio is a region of intermediate age featuring very distinct…
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