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Bolometric Hemispherical Albedo Map of Pluto from New Horizons Observations

Abstract:
The New Horizons encounter with the Pluto system revealed Pluto to have an extremely spatially variable surface with expansive dark, bright, and intermediate terrains, refractory and volatile ices, and ongoing/recent endogenous and exogenous processes. Albedo is useful for understanding volatile transport because it quantifies absorbed solar energy; albedo may also provide insights into surface processes. Four filters of the New Horizons LORRI and MVIC imagers are used to approximate the bolometric (flux-weighted, wavelength-integrated) albedo. The bolometric hemispherical albedo (local energy balance albedo) as a function of the incidence angle of the solar illumination is measured for both Cthulhu and Sputnik Planitia, which are extensive, extreme dark and extreme bright terrains on Pluto. For both terrains, the bolometric hemispherical albedo increases by >30% from 0° to 90° incidence. The incidence-angle-average bolometric hemispherical albedo of Cthulhu is 0.12 ± 0.01, and that of Sputnik Planitia is 0.80 ± 0.06, where uncertainties are estimates based on scatter from different photometric functional approximations. The bolometric Bond albedo (global energy balance albedo) of Cthulhu is 0.12 ± 0.01, and that of Sputnik Planitia is 0.80 ± 0.07. A map of Pluto’s incidence-angle-average bolometric hemispherical albedo is produced. The incidence-angle-average bolometric hemispherical albedo, spatially averaged over areas north of ≈30° S, is ≈0.54. Pluto has three general albedo categories: (1) very low albedo southern equatorial terrains, including Cthulhu; (2) high-albedo terrains, which constitute most of Pluto’s surface; and (3) very high albedo terrains, including Sputnik Planitia. Pluto’s extraordinary albedo variability with location is also spatially sharp at some places
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/psj/ace3ab

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Author
ORCID:
0000-0002-6517-3864
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Role:
Author
ORCID:
0000-0002-5901-4875
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ORCID:
0000-0003-4503-3335
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ORCID:
0000-0002-8847-8492
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Author
ORCID:
0000-0002-8296-6540


Publisher:
IOP Publishing
Journal:
The Planetary Science Journal More from this journal
Volume:
4
Issue:
7
Pages:
132-132
Publication date:
2023-07-27
DOI:
EISSN:
2632-3338
ISSN:
2632-3338


Language:
English
Keywords:
Pubs id:
1510156
Local pid:
pubs:1510156
Source identifiers:
W4385308554
Deposit date:
2026-05-12
ARK identifier:
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

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