Atmosphere and frost cycle revealed by Pluto's dark side

Pluto's dark side has come into dreary view, thanks to the radiance of the dwarf planet's moon. At the point when NASA's New Horizons spacecraft went by Pluto in 2015, almost all the images of the dwarf planet's out of the blue complex surface were of the side illuminated by the...

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Main Author: Mathew
Format: Article in Journal/Newspaper
Language:unknown
Published: Zenodo 2022
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Online Access:https://doi.org/10.5281/zenodo.6903976
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spelling ftzenodo:oai:zenodo.org:6903976 2024-09-15T18:36:56+00:00 Atmosphere and frost cycle revealed by Pluto's dark side Mathew 2022-07-25 https://doi.org/10.5281/zenodo.6903976 unknown Zenodo https://doi.org/10.5281/zenodo.6903975 https://doi.org/10.5281/zenodo.6903976 oai:zenodo.org:6903976 info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode info:eu-repo/semantics/article 2022 ftzenodo https://doi.org/10.5281/zenodo.690397610.5281/zenodo.6903975 2024-07-27T03:45:06Z Pluto's dark side has come into dreary view, thanks to the radiance of the dwarf planet's moon. At the point when NASA's New Horizons spacecraft went by Pluto in 2015, almost all the images of the dwarf planet's out of the blue complex surface were of the side illuminated by the sun (SN: 7/15/15). Darkness covered the dwarf planet's other half of the globe. Some of it, similar to the area near the south pole, hadn't seen the sun for quite a long time. Presently, mission scientists have finally released a grainy perspective on the dwarf planet's dark side. The researchers describe the cycle to take the photo and what it enlightens them regarding how Pluto's nitrogen cycle affects its atmosphere October 20 in the Planetary Science Journal. Before New Horizons passed by Pluto, the team thought the dwarf planet's largest moon, Charon, might mirror sufficient light to illuminate the distant world's surface. So the researchers had the spacecraft turn back toward the sun to take a parting look at Pluto. From the beginning, the images just showed a ring of sunlight filtering through Pluto's hazy atmosphere (SN: 7/24/15). "It's extremely hard to see anything in that glare," says planetary researcher John Spencer of the Southwest Research Institute in Boulder, Colo. "It's like trying to read a road sign while you're driving toward the setting sun and you have a grimy windshield." Spencer and colleagues took a couple of moves toward make it conceivable to pull details of Pluto's dark side out of the glare. To begin with, the team had the spacecraft take 360 short snapshots of the backlit dwarf planet. Each was about 0.4 seconds long, to avoid overexposing the images. The team also took snapshots of the sun without Pluto in the frame so the sun could be subtracted out after the fact. Tod Lauer of the National Optical Astronomy Observatory in Tucson, Ariz., attempted to deal with the images when he got the data in 2016. At the time, the other data from New Horizons was still new and took up the vast majority of his ... Article in Journal/Newspaper South pole Zenodo
institution Open Polar
collection Zenodo
op_collection_id ftzenodo
language unknown
description Pluto's dark side has come into dreary view, thanks to the radiance of the dwarf planet's moon. At the point when NASA's New Horizons spacecraft went by Pluto in 2015, almost all the images of the dwarf planet's out of the blue complex surface were of the side illuminated by the sun (SN: 7/15/15). Darkness covered the dwarf planet's other half of the globe. Some of it, similar to the area near the south pole, hadn't seen the sun for quite a long time. Presently, mission scientists have finally released a grainy perspective on the dwarf planet's dark side. The researchers describe the cycle to take the photo and what it enlightens them regarding how Pluto's nitrogen cycle affects its atmosphere October 20 in the Planetary Science Journal. Before New Horizons passed by Pluto, the team thought the dwarf planet's largest moon, Charon, might mirror sufficient light to illuminate the distant world's surface. So the researchers had the spacecraft turn back toward the sun to take a parting look at Pluto. From the beginning, the images just showed a ring of sunlight filtering through Pluto's hazy atmosphere (SN: 7/24/15). "It's extremely hard to see anything in that glare," says planetary researcher John Spencer of the Southwest Research Institute in Boulder, Colo. "It's like trying to read a road sign while you're driving toward the setting sun and you have a grimy windshield." Spencer and colleagues took a couple of moves toward make it conceivable to pull details of Pluto's dark side out of the glare. To begin with, the team had the spacecraft take 360 short snapshots of the backlit dwarf planet. Each was about 0.4 seconds long, to avoid overexposing the images. The team also took snapshots of the sun without Pluto in the frame so the sun could be subtracted out after the fact. Tod Lauer of the National Optical Astronomy Observatory in Tucson, Ariz., attempted to deal with the images when he got the data in 2016. At the time, the other data from New Horizons was still new and took up the vast majority of his ...
format Article in Journal/Newspaper
author Mathew
spellingShingle Mathew
Atmosphere and frost cycle revealed by Pluto's dark side
author_facet Mathew
author_sort Mathew
title Atmosphere and frost cycle revealed by Pluto's dark side
title_short Atmosphere and frost cycle revealed by Pluto's dark side
title_full Atmosphere and frost cycle revealed by Pluto's dark side
title_fullStr Atmosphere and frost cycle revealed by Pluto's dark side
title_full_unstemmed Atmosphere and frost cycle revealed by Pluto's dark side
title_sort atmosphere and frost cycle revealed by pluto's dark side
publisher Zenodo
publishDate 2022
url https://doi.org/10.5281/zenodo.6903976
genre South pole
genre_facet South pole
op_relation https://doi.org/10.5281/zenodo.6903975
https://doi.org/10.5281/zenodo.6903976
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op_rights info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
op_doi https://doi.org/10.5281/zenodo.690397610.5281/zenodo.6903975
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