Planetary Atmospheres: From Solar System to Exoplanets (2nd Edition)

A special issue of Atmosphere (ISSN 2073-4433). This special issue belongs to the section "Planetary Atmospheres".

Deadline for manuscript submissions: 30 April 2025 | Viewed by 96

Special Issue Editor


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Guest Editor
Insitute of Astrophysics and Space Sciences, Porto Rua das Estrelas, 4150-762 Porto, Portugal
Interests: atmospheres; atmosphere dynamics; spectroscopy; cloud-tracking; atmospheric composition; exoplanets; astrobiology; ARIEL space mission
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Special Issue Information

Dear Colleagues,

This Special Issue is the second edition of a series of publications dedicated to “Planetary Atmospheres: From Solar System to Exoplanets”: https://www.mdpi.com/journal/atmosphere/special_issues/solar_exoplanets.

There is currently a considerable effort from the science community to study the planetary atmospheres, within and beyond our Solar System. Nevertheless, the knowledge of all mechanisms at work on Solar System planet atmospheres is still limited. An understanding of the dominant factors and mechanisms controlling the atmospheric general circulation and its chemical composition is a prerequisite to our understanding of planets' climate variability and evolution. In this context, Solar System's gas giant planets, as well as telluric planets, are natural comparative laboratories to investigate the diversity of circulation regimes and the composition of planetary systems' atmospheres.

Planetary atmospheres' temporal and spatial variability of winds, the role of waves, and the mechanisms that allow topography to influence the upper cloud motions need to be addressed. There are still several open questions related with Solar System planets' atmospheres as is the case of the Venusian volcanism and its atmospheric impact, the source of the Venus atmosphere's super rotation, the origin of the methane detected on Mars, and how the "red planet" lost most of its water. Regarding the gas giants, there are also several mysteries that need to be addressed in order that we learn from our backyard's planets to better undergo a new quest in planetary systems research that relies on the characterization of exoplanets' atmospheres.

Dr. Pedro MacHado
Guest Editor

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Atmosphere is an international peer-reviewed open access monthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 2400 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

Keywords

  • atmospheres
  • rocky planets
  • atmosphere dynamics
  • atmospheric waves
  • atmosphere’s modeling

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Published Papers

This special issue is now open for submission.
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