{"title":"Magnetic Barriers Might Explain Mysterious Hot Jupiters","authors":"Jonathan O’Callaghan","doi":"10.1029/2024eo240238","DOIUrl":null,"url":null,"abstract":"Hot Jupiters might end up very close to stars because a magnetic field halts their progress—and future observations could confirm the idea.","PeriodicalId":52431,"journal":{"name":"Eos","volume":"29 27","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-06-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Eos","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1029/2024eo240238","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Earth and Planetary Sciences","Score":null,"Total":0}
引用次数: 0
Abstract
Hot Jupiters might end up very close to stars because a magnetic field halts their progress—and future observations could confirm the idea.