M.D. Paton , P.M. Grindrod , T. Bertrand , J.M. Davis , A.-M. Harri , H. Savijärvi , C. Segonne
{"title":"Inferred wind and surface conditions during the descent and landing of Beagle 2 on Mars","authors":"M.D. Paton , P.M. Grindrod , T. Bertrand , J.M. Davis , A.-M. Harri , H. Savijärvi , C. Segonne","doi":"10.1016/j.icarus.2025.116728","DOIUrl":null,"url":null,"abstract":"<div><div>Beagle 2 was a British-built lander sent to Isidis Planitia on Mars in 2003. It was part of ESA's Mars Express mission to conduct astrobiology investigations on the surface but failed to communicate after landing. The lander and its jettisoned hardware were eventually discovered on the surface in images taken from orbit. These items preserve information about the wind conditions during the descent and landing. Deciphering the location of these items allows us a glimpse into the atmospheric circulation on Mars and hence an opportunity to verify atmospheric models. In addition, the knowledge can help improve our understanding of the conditions during Beagle 2's descent and landing.</div><div>We found the winds during the initial part of the descent to be consistent with the expected large-scale circulation, especially in terms of wind direction, i.e., a complex interaction between Hadley circulation, stationary waves and the thermal tide. The mean wind speed and direction in the lower part of the descent were found to be consistent with a strong circulation in the basin, driven by slope winds on its rim. As well as the wind conditions we were able to provide some constraints on the surface properties. From modelling the bouncing trajectory of the airbags, there is some indication they were deflected to the side after impact perhaps by an uneven surface, e.g. impact with the Transverse Aeolian Ridges (TARs) as observed in the HiRISE images.</div><div>We have inferred wind speed and direction profiles for the descent and landing of Beagle 2. This study indicates that the wind conditions during the descent of Beagle 2 were likely in line with atmospheric model predictions. The study has been useful for verifying atmospheric models and constraining the range of conditions during the descent and landing of Beagle 2.</div></div>","PeriodicalId":13199,"journal":{"name":"Icarus","volume":"441 ","pages":"Article 116728"},"PeriodicalIF":3.0000,"publicationDate":"2025-07-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Icarus","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0019103525002763","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Beagle 2 was a British-built lander sent to Isidis Planitia on Mars in 2003. It was part of ESA's Mars Express mission to conduct astrobiology investigations on the surface but failed to communicate after landing. The lander and its jettisoned hardware were eventually discovered on the surface in images taken from orbit. These items preserve information about the wind conditions during the descent and landing. Deciphering the location of these items allows us a glimpse into the atmospheric circulation on Mars and hence an opportunity to verify atmospheric models. In addition, the knowledge can help improve our understanding of the conditions during Beagle 2's descent and landing.
We found the winds during the initial part of the descent to be consistent with the expected large-scale circulation, especially in terms of wind direction, i.e., a complex interaction between Hadley circulation, stationary waves and the thermal tide. The mean wind speed and direction in the lower part of the descent were found to be consistent with a strong circulation in the basin, driven by slope winds on its rim. As well as the wind conditions we were able to provide some constraints on the surface properties. From modelling the bouncing trajectory of the airbags, there is some indication they were deflected to the side after impact perhaps by an uneven surface, e.g. impact with the Transverse Aeolian Ridges (TARs) as observed in the HiRISE images.
We have inferred wind speed and direction profiles for the descent and landing of Beagle 2. This study indicates that the wind conditions during the descent of Beagle 2 were likely in line with atmospheric model predictions. The study has been useful for verifying atmospheric models and constraining the range of conditions during the descent and landing of Beagle 2.
期刊介绍:
Icarus is devoted to the publication of original contributions in the field of Solar System studies. Manuscripts reporting the results of new research - observational, experimental, or theoretical - concerning the astronomy, geology, meteorology, physics, chemistry, biology, and other scientific aspects of our Solar System or extrasolar systems are welcome. The journal generally does not publish papers devoted exclusively to the Sun, the Earth, celestial mechanics, meteoritics, or astrophysics. Icarus does not publish papers that provide "improved" versions of Bode''s law, or other numerical relations, without a sound physical basis. Icarus does not publish meeting announcements or general notices. Reviews, historical papers, and manuscripts describing spacecraft instrumentation may be considered, but only with prior approval of the editor. An entire issue of the journal is occasionally devoted to a single subject, usually arising from a conference on the same topic. The language of publication is English. American or British usage is accepted, but not a mixture of these.