{"title":"月球上的极地帽","authors":"Jan Kostelecký, Jaroslav Klokočník, Aleš Bezděk","doi":"10.1007/s10509-025-04457-0","DOIUrl":null,"url":null,"abstract":"<div><p>The Moon very likely has polar caps, but not as conspicuous as the Earth or Mars; the Moon’s caps must be hidden under the surface. The southern polar cap is probably more aquiferous than the northern one. Our indication of ground water at the poles has been obtained by a remote sensing method. We use the gravity aspects, namely the combed strike angles, derived from a global gravity field model of the Moon (now providing the ground resolution ∼10 km already sufficient for this purpose). We cannot estimate the absolute amount of the lunar water, only the contrast between the polar areas and the other regions; the contrast is high, statistically significant – to 8 times more groundwater at the poles. For the southern polar zone, we confirm the results achieved by others, and we do it in a completely independent way. The lunar water is necessary for future permanent human missions on the Moon, like Artemis; they will start near the southern pole. Thus, our findings would have immediate applications. <i>Observe and download</i>: https://www.asu.cas.cz/~jklokocn/MOON25_supplements/</p></div>","PeriodicalId":8644,"journal":{"name":"Astrophysics and Space Science","volume":"370 7","pages":""},"PeriodicalIF":1.8000,"publicationDate":"2025-07-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s10509-025-04457-0.pdf","citationCount":"0","resultStr":"{\"title\":\"Polar caps on the Moon\",\"authors\":\"Jan Kostelecký, Jaroslav Klokočník, Aleš Bezděk\",\"doi\":\"10.1007/s10509-025-04457-0\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>The Moon very likely has polar caps, but not as conspicuous as the Earth or Mars; the Moon’s caps must be hidden under the surface. The southern polar cap is probably more aquiferous than the northern one. Our indication of ground water at the poles has been obtained by a remote sensing method. We use the gravity aspects, namely the combed strike angles, derived from a global gravity field model of the Moon (now providing the ground resolution ∼10 km already sufficient for this purpose). We cannot estimate the absolute amount of the lunar water, only the contrast between the polar areas and the other regions; the contrast is high, statistically significant – to 8 times more groundwater at the poles. For the southern polar zone, we confirm the results achieved by others, and we do it in a completely independent way. The lunar water is necessary for future permanent human missions on the Moon, like Artemis; they will start near the southern pole. Thus, our findings would have immediate applications. <i>Observe and download</i>: https://www.asu.cas.cz/~jklokocn/MOON25_supplements/</p></div>\",\"PeriodicalId\":8644,\"journal\":{\"name\":\"Astrophysics and Space Science\",\"volume\":\"370 7\",\"pages\":\"\"},\"PeriodicalIF\":1.8000,\"publicationDate\":\"2025-07-04\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://link.springer.com/content/pdf/10.1007/s10509-025-04457-0.pdf\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astrophysics and Space Science\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1007/s10509-025-04457-0\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astrophysics and Space Science","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10509-025-04457-0","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
The Moon very likely has polar caps, but not as conspicuous as the Earth or Mars; the Moon’s caps must be hidden under the surface. The southern polar cap is probably more aquiferous than the northern one. Our indication of ground water at the poles has been obtained by a remote sensing method. We use the gravity aspects, namely the combed strike angles, derived from a global gravity field model of the Moon (now providing the ground resolution ∼10 km already sufficient for this purpose). We cannot estimate the absolute amount of the lunar water, only the contrast between the polar areas and the other regions; the contrast is high, statistically significant – to 8 times more groundwater at the poles. For the southern polar zone, we confirm the results achieved by others, and we do it in a completely independent way. The lunar water is necessary for future permanent human missions on the Moon, like Artemis; they will start near the southern pole. Thus, our findings would have immediate applications. Observe and download: https://www.asu.cas.cz/~jklokocn/MOON25_supplements/
期刊介绍:
Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered.
The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing.
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