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Cited by 307

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Ancient lowlands on Mars

Frey, Herbert V., Roark, James H., Shockey, Kelly M., Frey, Erin L., Sakimoto, Susan E. H.·2002·Geophysical Research Letters

Abstract

Mars Orbiter Laser Altimeter (MOLA) data provide compelling evidence that the martian lowlands, below the smooth and sparsely cratered northern plains, are extremely old, far older than the plains which cover them. The evidence is in the form of a very large population of “Quasi‐Circular Depressions” (QCDs), many of which are very evident in the MOLA elevation data but generally not visible in available imagery. We interpret these “invisible” QCDs to be buried impact basins. Cumulative number versus diameter curves for lowland QCDs suggests the buried lowland surface is older than the visible highland surface and that the lowland plains are a relatively thin (1–2 km) veneer overlying this much older surface. We conclude that the martian lowlands have been low and stable for nearly all of martian history.

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Metadata

Authors
Frey, H. V., Roark, J. H., Shockey, K. M., Frey, E. L., & Sakimoto, S. E. H.
Venue
Geophysical Research Letters
Published
2002-05-15
Volume
29
Issue
10
ISSN
  • 0094-8276 (ISSN-L)
  • 1944-8007
OpenAlex
W1614526441
Cited by
307
References
0
FWCI
10.79
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Ancient lowlands on Mars. https://app.cochat.ai/papers/10.1029/2001gl013832
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Frey, H. V., Roark, J. H., Shockey, K. M., Frey, E. L., & Sakimoto, S. E. H. (2002). Ancient lowlands on Mars. Geophysical Research Letters. https://doi.org/10.1029/2001gl013832

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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