Lunar Hydration at the South Pole observed by Deep Impact [version 1.0]
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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| Format: | Dataset |
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2022
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| Online Access: | https://doi.org/10.4231/T3B9-QK78 |
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ftpurdueunivpurr:https://doi.org/10.4231/T3B9-QK78 |
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openpolar |
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ftpurdueunivpurr:https://doi.org/10.4231/T3B9-QK78 2023-11-12T04:26:17+01:00 Lunar Hydration at the South Pole observed by Deep Impact [version 1.0] Kris Laferriere 2022-05-05T05:28:26Z https://doi.org/10.4231/T3B9-QK78 unknown https://doi.org/10.4231/0643-AM58 https://doi.org/10.4231/T3B9-QK78 EAPS hydration hydroxyl Lunar Water publications:dataset 2022 ftpurdueunivpurr https://doi.org/10.4231/T3B9-QK7810.4231/0643-AM58 2023-10-30T09:32:34Z 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 South Pole |
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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 Lunar Water |
| spellingShingle |
EAPS hydration hydroxyl Lunar Water Kris Laferriere Lunar Hydration at the South Pole observed by Deep Impact [version 1.0] |
| topic_facet |
EAPS hydration hydroxyl Lunar 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 1.0] |
| title_short |
Lunar Hydration at the South Pole observed by Deep Impact [version 1.0] |
| title_full |
Lunar Hydration at the South Pole observed by Deep Impact [version 1.0] |
| title_fullStr |
Lunar Hydration at the South Pole observed by Deep Impact [version 1.0] |
| title_full_unstemmed |
Lunar Hydration at the South Pole observed by Deep Impact [version 1.0] |
| title_sort |
lunar hydration at the south pole observed by deep impact [version 1.0] |
| publishDate |
2022 |
| url |
https://doi.org/10.4231/T3B9-QK78 |
| geographic |
South Pole |
| geographic_facet |
South Pole |
| genre |
South pole |
| genre_facet |
South pole |
| op_relation |
https://doi.org/10.4231/0643-AM58 https://doi.org/10.4231/T3B9-QK78 |
| op_doi |
https://doi.org/10.4231/T3B9-QK7810.4231/0643-AM58 |
| _version_ |
1782340330186604544 |