Observation from Earth of an atypical cloud system in the upper Martian atmosphere

Author:

Lilensten J.,Dauvergne J. L.,Pellier C.,Delcroix M.,Beaudoin E.,Vincendon M.,Kraaikamp E.,Bertrand G.,Foster C.,Go C.,Kardasis E.,Pace A.,Peach D.,Wesley A.,Samara E.,Poedts S.,Colas F.

Abstract

Context. The atmosphere of Mars is characterised by a complex seasonal cycle of cloud formation related to the condensation of CO2 and H2O, and to the lifting of surface dust. Several decades of spacecraft observations have provided an impressive amount of data to constrain cloud properties. However, observations of a given cloud obtained from Mars orbit are typically limited in time sampling and spatial coverage. As a complement to this existing dataset, Earth-based telescopic observations have the potential to provide a global and dynamic view of some large-scale Mars clouds. Aims. On 17 November 2020, Mars and Earth were close to opposition. We took advantage of this configuration to attempt observing large-scale high-altitude atmospheric phenomena from Earth with a high time sampling, over several hours. Methods. Ten amateur astronomers were coordinated along with professional astronomers to observe Mars. Results. We observed the occurrence of a large-scale high-altitude cloud system, extending over thousands of kilometres from the equator to 50°S. Over 3 h, it emerged from the night side at 92−16+30 km and dissipated on the dayside. It occurred at a solar longitude of 316° (southern summer) concomitantly to a regional dust storm and west of the magnetic anomaly. Despite its high altitude, it was composed of relatively large particles (effective radius in the 1–2 µm range). While dust appears an unlikely candidate, possible composition by CO2 or H2O are both conceivable, although the whole properties of the cloud makes it atypical compared to previously reported clouds. We discuss the possible connections with the dust storm, along with the hypothetical role of nucleation from cosmic particle precipitation. Conclusions. We continuously followed a high-altitude huge cloud system on Mars from Earth, emerging from the Martian night, from its appearance at the terminator until its complete dissipation. It is either a large-grained water ice cloud system or an extended mid-summer dawn CO2 cloud system.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Dynamics and clouds in planetary atmospheres from telescopic observations;The Astronomy and Astrophysics Review;2023-12

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3