The DOI matches its Crossref record; 17 of the 17 references it cites were found in a registry or an index.
Ancient Geodynamics and Global-Scale Hydrology on Mars
Abstract
Loading of the lithosphere of Mars by the Tharsis rise explains much of the global shape and long-wavelength gravity field of the planet, including a ring of negative gravity anomalies and a topographic trough around Tharsis, as well as gravity anomaly and topographic highs centered in Arabia Terra and extending northward toward Utopia. The Tharsis-induced trough and antipodal high were largely in place by the end of the Noachian Epoch and exerted control on the location and orientation of valley networks. The release of carbon dioxide and water accompanying the emplacement of ∼3 × 10 8 cubic kilometers of Tharsis magmas may have sustained a warmer climate than at present, enabling the formation of ancient valley networks and fluvial landscape denudation in and adjacent to the large-scale trough.
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Zuber, M. T., Solomon, S. C., Phillips, R. J., Smith, D. E., Tyler, G. L., Aharonson, O., Balmino, G., Banerdt, W. B., Head, J. W., Johnson, C. L., et al. (2000) · Science · doi:10.1126/science.287.5459.1788 · Cited by 586
Self-citationCarr, M. H. (1996) · doi:10.1093/oso/9780195099386.001.0001 · Cited by 551
Warming Early Mars with Carbon Dioxide Clouds That Scatter Infrared Radiation
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Interior Structure and Seasonal Mass Redistribution of Mars from Radio Tracking of Mars Pathfinder
Folkner, W. M., Yoder, C. F., Yuan, D. N., Standish, E. M., & Preston, R. A. (1997) · Science · doi:10.1126/science.278.5344.1749 · Cited by 311
The Martian drainage system and the origin of valley networks and fretted channels
Carr, M. H. (1995) · Journal of Geophysical Research: Planets · doi:10.1029/95je00260 · Cited by 269
Voluminous volcanism on early Mars revealed in Valles Marineris
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Role of membrane stresses in the support of planetary topography
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Geochemical evidence for magmatic water within Mars from pyroxenes in the Shergotty meteorite
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Cited by
Global Mineralogical and Aqueous Mars History Derived from OMEGA/Mars Express Data
Bibring, J.-P., Langevin, Y., Mustard, J. F., Poulet, F., Arvidson, R., Gendrin, A., Gondet, B., Mangold, N., Pinet, P., Forget, F., et al. (2006) · Science · doi:10.1126/science.1122659 · Cited by 1,667
Subsurface water and clay mineral formation during the early history of Mars
Ehlmann, B. L., Mustard, J. F., Murchie, S. L., Bibring, J.-P., Meunier, A., Fraeman, A. A., & Langevin, Y. (2011) · Nature · doi:10.1038/nature10582 · Cited by 868
Carr, M. H., & Head, J. W. (2010) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2009.06.042 · Cited by 734
Water and the martian landscape
Baker, V. R. (2001) · Nature · doi:10.1038/35084172 · Cited by 608
Updated global map of Martian valley networks and implications for climate and hydrologic processes
Hynek, B. M., Beach, M., & Hoke, M. R. T. (2010) · Journal of Geophysical Research: Planets · doi:10.1029/2009je003548 · Cited by 505
Self-citation
Metadata
- Authors
- Phillips, R. J., Zuber, M. T., Solomon, S. C., Golombek, M. P., Jakosky, B. M., Banerdt, W. B., Smith, D. E., Williams, R. M. E., Hynek, B. M., Aharonson, O., & Hauck II, S. A.
- Venue
- Science
- Published
- 2001-03-30
- Volume
- 291
- Issue
- 5513
- Pages
- 2587-2591
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2096724893
- Cited by
- 506
- References
- 17
- FWCI
- 14.87
- Type
- journal article
- Language
- en
- Open access
- closed
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- Phillips, R. J., Zuber, M. T., Solomon, S. C., Golombek, M. P., Jakosky, B. M., Banerdt, W. B., Smith, D. E., Williams, R. M. E., Hynek, B. M., Aharonson, O., & Hauck II, S. A. (2001). Ancient Geodynamics and Global-Scale Hydrology on Mars. Science. https://doi.org/10.1126/science.1058701
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
