Lunar Hydration at the South Pole observed by Deep Impact [version 2.0]
The dataset contains the information used to investigate the variability of the 3 micron hydration absorption feature on the southern hemisphere of the Moon as observed by the Deep Impact spacecraft during the lunar flybys in 2009. We used this data to determine the dependencies (temperature, latitu...
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2023
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| Online Access: | https://doi.org/10.4231/0643-AM58 |
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ftpurdueunivpurr:https://doi.org/10.4231/0643-AM58 |
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ftpurdueunivpurr:https://doi.org/10.4231/0643-AM58 2023-11-12T04:26:17+01:00 Lunar Hydration at the South Pole observed by Deep Impact [version 2.0] Kris Laferriere 2023-08-11T02:48:01Z https://doi.org/10.4231/0643-AM58 unknown https://doi.org/10.4231/T3B9-QK78 https://doi.org/10.4231/0643-AM58 EAPS hydration hydroxyl Moon Water publications:dataset 2023 ftpurdueunivpurr https://doi.org/10.4231/0643-AM5810.4231/T3B9-QK78 2023-10-30T09:32:39Z The dataset contains the information used to investigate the variability of the 3 micron hydration absorption feature on the southern hemisphere of the Moon as observed by the Deep Impact spacecraft during the lunar flybys in 2009. We used this data to determine the dependencies (temperature, latitude, time of day) for the strength of the 3 micron feature, to understand what processes lead to the formation and loss of OH/H2O on the lunar surface. Dataset South pole Purdue University Research Repository |
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Open Polar |
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Purdue University Research Repository |
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ftpurdueunivpurr |
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unknown |
| topic |
EAPS hydration hydroxyl Moon Water |
| spellingShingle |
EAPS hydration hydroxyl Moon Water Kris Laferriere Lunar Hydration at the South Pole observed by Deep Impact [version 2.0] |
| topic_facet |
EAPS hydration hydroxyl Moon Water |
| description |
The dataset contains the information used to investigate the variability of the 3 micron hydration absorption feature on the southern hemisphere of the Moon as observed by the Deep Impact spacecraft during the lunar flybys in 2009. We used this data to determine the dependencies (temperature, latitude, time of day) for the strength of the 3 micron feature, to understand what processes lead to the formation and loss of OH/H2O on the lunar surface. |
| format |
Dataset |
| author |
Kris Laferriere |
| author_facet |
Kris Laferriere |
| author_sort |
Kris Laferriere |
| title |
Lunar Hydration at the South Pole observed by Deep Impact [version 2.0] |
| title_short |
Lunar Hydration at the South Pole observed by Deep Impact [version 2.0] |
| title_full |
Lunar Hydration at the South Pole observed by Deep Impact [version 2.0] |
| title_fullStr |
Lunar Hydration at the South Pole observed by Deep Impact [version 2.0] |
| title_full_unstemmed |
Lunar Hydration at the South Pole observed by Deep Impact [version 2.0] |
| title_sort |
lunar hydration at the south pole observed by deep impact [version 2.0] |
| publishDate |
2023 |
| url |
https://doi.org/10.4231/0643-AM58 |
| genre |
South pole |
| genre_facet |
South pole |
| op_relation |
https://doi.org/10.4231/T3B9-QK78 https://doi.org/10.4231/0643-AM58 |
| op_doi |
https://doi.org/10.4231/0643-AM5810.4231/T3B9-QK78 |
| _version_ |
1782340330379542528 |