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Mars' Lowest and Highest Points Revisited

Mars' Lowest and Highest Points Revisited

This is a Preprint and has not been peer reviewed. This is version 1 of this Preprint.

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Comment #259 Kamilla Dyreborg Hansen @ 2025-12-05 22:05

The manuscript uses numerical-only references in some places (e.g., in the introduction), author-year plus numerical references in others (e.g., Voelker et al. (2017) [6]), and institution-year citations elsewhere (e.g., USGS (2002) [9]). I'm not sure whether this hybrid style is intentional or simply evolved through revisions, so I thought I'd mention it in case you decide to harmonize citation style in a future revision. No need to change it, of course — I just wanted to check whether it reflects a conscious choice.

In Section 3.1.2: Adding the explicit reference to Figure 1 may tidy the flow when discussing points A and B (e.g., “as evident in Figure 1”). It reads clearly as it is, but this would remove any ambiguity.
Figures 1 and 2 are excellent — very clean and intuitive. But if they are reused outside the manuscript context (talks, slides, future papers), a slightly more descriptive caption would allow you to preserve your intended interpretation.

In the conclusion, “metres” appears in US English context — you might want to change this to “meters” for consistency.

If you’d like to add a future-perspective sentence, this method could be applied to other topographic anomalies, particularly where MOLA sampling gaps complicate local interpretation. For example, this may benefit landing-site analyses where accurate local topography is vital for mission safety.

Your paper is refreshingly concise — many Mars papers drown the reader in context; yours delivers a single clear objective with a single clear result.
Given the methodological clarity and real improvement over MOLA-only estimates, you might allow yourself to assert the significance a bit more confidently in your conclusion section.
I enjoyed reading this, and I thank you for your work.

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Authors

Jim Singh

Abstract

We present revised values for Mars’ extreme elevations using a blended digital elevation model (DEM) that combines altimetry collected from the Mars Orbiter Laser Altimeter (MOLA) on NASA’s Mars Global Surveyor with stereo imagery from the High Resolution Stereo Camera (HRSC) on ESA’s Mars Express. The widely cited minimum elevation is derived from an earlier MOLA-only DEM which lacks direct altimetry in the region of the true minimum, where interpolation omitted a pit. Using the blended DEM, we identify and measure this feature to produce a revised estimate of Mars’ lowest point. The same dataset also enables a reassessment of the position and elevation of the planet’s highest point on Olympus Mons.

DOI

https://doi.org/10.31223/X5HN10

Subjects

Physical Sciences and Mathematics, Planetary Geomorphology, Planetary Sciences

Keywords

Mars, Olympus Mons, Badwater crater, topographic extremes, highest elevation, lowest elevation, Mars surface features, MOLA, HRSC, DEM

Dates

Published: 2025-10-25 19:14

Last Updated: 2025-10-25 19:14

License

CC BY Attribution 4.0 International

Additional Metadata

Conflict of interest statement:
None

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Downloads: 269