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Lenghu on the Tibetan Plateau as an astronomical observing site
On Earth’s surface, there are only a handful of high-quality astronomical sites that meet the requirements for very large next-generation facilities. In the context of scientific opportunities in time-domain astronomy, a good site on the Tibetan Plateau will bridge the longitudinal gap between the k...
Autores principales: | , , , , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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Nature Publishing Group UK
2021
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8373612/ https://www.ncbi.nlm.nih.gov/pubmed/34408333 http://dx.doi.org/10.1038/s41586-021-03711-z |
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author | Deng, Licai Yang, Fan Chen, Xiaodian He, Fei Liu, Qili Zhang, Bo Zhang, Chunguang Wang, Kun Liu, Nian Ren, Anbing Luo, Zhiquan Yan, Zhengzhou Tian, Jianfeng Pan, Jun |
author_facet | Deng, Licai Yang, Fan Chen, Xiaodian He, Fei Liu, Qili Zhang, Bo Zhang, Chunguang Wang, Kun Liu, Nian Ren, Anbing Luo, Zhiquan Yan, Zhengzhou Tian, Jianfeng Pan, Jun |
author_sort | Deng, Licai |
collection | PubMed |
description | On Earth’s surface, there are only a handful of high-quality astronomical sites that meet the requirements for very large next-generation facilities. In the context of scientific opportunities in time-domain astronomy, a good site on the Tibetan Plateau will bridge the longitudinal gap between the known best sites(1,2) (all in the Western Hemisphere). The Tibetan Plateau is the highest plateau on Earth, with an average elevation of over 4,000 metres, and thus potentially provides very good opportunities for astronomy and particle astrophysics(3–5). Here we report the results of three years of monitoring of testing an area at a local summit on Saishiteng Mountain near Lenghu Town in Qinghai Province. The altitudes of the potential locations are between 4,200 and 4,500 metres. An area of over 100,000 square kilometres surrounding Lenghu Town has a lower altitude of below 3,000 metres, with an extremely arid climate and unusually clear local sky (day and night)(6). Of the nights at the site, 70 per cent have clear, photometric conditions, with a median seeing of 0.75 arcseconds. The median night temperature variation is only 2.4 degrees Celsius, indicating very stable local surface air. The precipitable water vapour is lower than 2 millimetres for 55 per cent of the night. |
format | Online Article Text |
id | pubmed-8373612 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2021 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-83736122021-09-02 Lenghu on the Tibetan Plateau as an astronomical observing site Deng, Licai Yang, Fan Chen, Xiaodian He, Fei Liu, Qili Zhang, Bo Zhang, Chunguang Wang, Kun Liu, Nian Ren, Anbing Luo, Zhiquan Yan, Zhengzhou Tian, Jianfeng Pan, Jun Nature Article On Earth’s surface, there are only a handful of high-quality astronomical sites that meet the requirements for very large next-generation facilities. In the context of scientific opportunities in time-domain astronomy, a good site on the Tibetan Plateau will bridge the longitudinal gap between the known best sites(1,2) (all in the Western Hemisphere). The Tibetan Plateau is the highest plateau on Earth, with an average elevation of over 4,000 metres, and thus potentially provides very good opportunities for astronomy and particle astrophysics(3–5). Here we report the results of three years of monitoring of testing an area at a local summit on Saishiteng Mountain near Lenghu Town in Qinghai Province. The altitudes of the potential locations are between 4,200 and 4,500 metres. An area of over 100,000 square kilometres surrounding Lenghu Town has a lower altitude of below 3,000 metres, with an extremely arid climate and unusually clear local sky (day and night)(6). Of the nights at the site, 70 per cent have clear, photometric conditions, with a median seeing of 0.75 arcseconds. The median night temperature variation is only 2.4 degrees Celsius, indicating very stable local surface air. The precipitable water vapour is lower than 2 millimetres for 55 per cent of the night. Nature Publishing Group UK 2021-08-18 2021 /pmc/articles/PMC8373612/ /pubmed/34408333 http://dx.doi.org/10.1038/s41586-021-03711-z Text en © The Author(s) 2021 https://creativecommons.org/licenses/by/4.0/Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Article Deng, Licai Yang, Fan Chen, Xiaodian He, Fei Liu, Qili Zhang, Bo Zhang, Chunguang Wang, Kun Liu, Nian Ren, Anbing Luo, Zhiquan Yan, Zhengzhou Tian, Jianfeng Pan, Jun Lenghu on the Tibetan Plateau as an astronomical observing site |
title | Lenghu on the Tibetan Plateau as an astronomical observing site |
title_full | Lenghu on the Tibetan Plateau as an astronomical observing site |
title_fullStr | Lenghu on the Tibetan Plateau as an astronomical observing site |
title_full_unstemmed | Lenghu on the Tibetan Plateau as an astronomical observing site |
title_short | Lenghu on the Tibetan Plateau as an astronomical observing site |
title_sort | lenghu on the tibetan plateau as an astronomical observing site |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8373612/ https://www.ncbi.nlm.nih.gov/pubmed/34408333 http://dx.doi.org/10.1038/s41586-021-03711-z |
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