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Planetary Geologic Mapping and Remote Sensing (Third Edition)

A special issue of Remote Sensing (ISSN 2072-4292). This special issue belongs to the section "Satellite Missions for Earth and Planetary Exploration".

Deadline for manuscript submissions: 16 March 2026 | Viewed by 597

Special Issue Editors


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Guest Editor
Head, Imaging Group, Mullard Space Science Laboratory, Department of Space & Climate Physics, University College London (UCL), Holmbury St Mary, RH5 6NT, UK
Interests: deep learning for change detection on Mars; 3D imaging for Mars and the Moon; orbital-rover image fusion; subsurface mapping; super-resolution restoration; surface albedo; cloud heights and winds; globe imaging; VR.
Special Issues, Collections and Topics in MDPI journals

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Guest Editor
Institute of Geology and Geophysics Chinese Academy of Sciences, Beijing, China
Interests: planetary remote sensing; planetary impact craters; planetary surface dating

Special Issue Information

Dear Colleagues,

Planetary geologic maps are spatial and temporal representations of the materials, landforms, structures, and processes of planetary surfaces. Planetary geologic mapping is largely based on analyses of various remote sensing data acquired by space missions and is fundamental in understanding the formation and evolution of planetary surfaces and shallow subsurfaces. Planetary remote sensing techniques and the ever-increasing data have greatly supported geologic mapping, as well as other scientific studies of the Moon, Mars and other planetary bodies in the solar system.

This is the third edition of the Special Issue “Planetary Geologic Mapping and Remote Sensing”. The first edition and the second edition were a great success and attracted much attention in the scientific community. Therefore, we are pleased to announce this new volume in Remote Sensing.

We welcome new submissions on the recent advances in planetary geologic mapping and planetary remote sensing, including theory, methods, techniques, algorithms, data validation, mapping products, and applications. Review articles are also welcome. Articles may address, but are not limited to, the following topics:

  • Planetary geologic mapping;
  • Planetary geomorphologic mapping;
  • Photogrammetric remote sensing of planetary surfaces;
  • Spectroscopic remote sensing of planetary surfaces;
  • Remote sensing methods, data calibration and validation;
  • Planetary GIS for geologic mapping;
  • Recent and future planetary exploration missions;
  • Landing sites studies;
  • Analog studies.

Prof. Dr. Jan-Peter Muller
Prof. Dr. Zongyu Yue
Guest Editors

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 250 words) can be sent to the Editorial Office for assessment.

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. Remote Sensing is an international peer-reviewed open access semimonthly 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 2700 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

  • planetary geology
  • planetary topography and geomorphology
  • planetary chronology
  • planetary spectrum
  • planetary remote sensing
  • geologic structures
  • geologic mapping
  • planetary composition
  • planetary GIS
  • planetary exploration missions
  • landing sites

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Published Papers (1 paper)

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Research

19 pages, 5281 KB  
Article
Morphometric Analysis and Emplacement Dynamics of Folded Terrains at Avernus Colles, Mars
by Caitlin Ahrens and Rachel A. Slank
Remote Sens. 2025, 17(24), 3946; https://doi.org/10.3390/rs17243946 - 6 Dec 2025
Viewed by 469
Abstract
Folded, arcuate terrains on the surface of Mars provide insight into the volcanic properties of surface materials and emplacement dynamics. This research focused on the analysis of folded terrains in the chaotic-terrain Avernus Colles region, located near Elysium Planitia, using images from the [...] Read more.
Folded, arcuate terrains on the surface of Mars provide insight into the volcanic properties of surface materials and emplacement dynamics. This research focused on the analysis of folded terrains in the chaotic-terrain Avernus Colles region, located near Elysium Planitia, using images from the Mars Odyssey Orbiter and altimetry data from the Mars Orbiter Laser Altimeter (MOLA). The combined data revealed areas of deformation, which is inferred to be the result of compressions and possibly collapse from the late Amazonian period. We identified and measured 19 distinct folds, with morphometric wavelengths ranging from 0.7 to 1.75 km. These measurements were applied to a simple two-layer regolith model to better understand the folding patterns observed. The model suggests that these folds could have formed with an upper viscous boundary layer less than 0.55 km thick and strain rates approximately 10−7 s−1. These strain rates indicate that the deformation of the terrains likely occurred over a relatively short period of time, ranging from 16 to 38 days. By studying these deformation patterns, we can enhance our understanding of the volcanic history and surface processes on Mars, offering insight into the planet’s geologic evolution and material properties. Full article
(This article belongs to the Special Issue Planetary Geologic Mapping and Remote Sensing (Third Edition))
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