{"title":"利用WSO-UV任务对彗星和系外行星进行光谱研究的潜力","authors":"E. Kanev, S. Sichevsky, V. Shmagin, M. Sachkov","doi":"10.31577/caosp.2021.51.3.221","DOIUrl":null,"url":null,"abstract":"In this article we consider the prospects of research on comets and exoplanets using instruments onboard the WSO-UV mission. Ultraviolet spectroscopy at 115-310 nm is a powerful tool for studying comets, since this range of the electromagnetic spectrum contains most of the resonance lines of atoms, molecules and ions. The spectrographs on board the WSO-UV spacecraft will become one of the most important instruments for spectral studies of comets and exoplanets after 2025.","PeriodicalId":50617,"journal":{"name":"Contributions of the Astronomical Observatory Skalnate Pleso","volume":" ","pages":""},"PeriodicalIF":0.4000,"publicationDate":"2021-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Potentials of spectroscopic studies of comets and exoplanets with WSO-UV mission\",\"authors\":\"E. Kanev, S. Sichevsky, V. Shmagin, M. Sachkov\",\"doi\":\"10.31577/caosp.2021.51.3.221\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In this article we consider the prospects of research on comets and exoplanets using instruments onboard the WSO-UV mission. Ultraviolet spectroscopy at 115-310 nm is a powerful tool for studying comets, since this range of the electromagnetic spectrum contains most of the resonance lines of atoms, molecules and ions. The spectrographs on board the WSO-UV spacecraft will become one of the most important instruments for spectral studies of comets and exoplanets after 2025.\",\"PeriodicalId\":50617,\"journal\":{\"name\":\"Contributions of the Astronomical Observatory Skalnate Pleso\",\"volume\":\" \",\"pages\":\"\"},\"PeriodicalIF\":0.4000,\"publicationDate\":\"2021-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Contributions of the Astronomical Observatory Skalnate Pleso\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.31577/caosp.2021.51.3.221\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Contributions of the Astronomical Observatory Skalnate Pleso","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.31577/caosp.2021.51.3.221","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Potentials of spectroscopic studies of comets and exoplanets with WSO-UV mission
In this article we consider the prospects of research on comets and exoplanets using instruments onboard the WSO-UV mission. Ultraviolet spectroscopy at 115-310 nm is a powerful tool for studying comets, since this range of the electromagnetic spectrum contains most of the resonance lines of atoms, molecules and ions. The spectrographs on board the WSO-UV spacecraft will become one of the most important instruments for spectral studies of comets and exoplanets after 2025.
期刊介绍：
Contributions of the Astronomical Observatory Skalnate Pleso" (CAOSP) is published by the Astronomical Institute of the Slovak Academy of Sciences (SAS). The journal publishes new results of astronomical and astrophysical research, preferentially covering the fields of Interplanetary Matter, Stellar Astrophysics and Solar Physics. We publish regular papers, expert comments and review contributions.
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