High‐obliquity simulations for the Archean Earth: Implications for climatic conditions on early Mars
- 25 December 2001
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 106 (E12) , 32903-32913
- https://doi.org/10.1029/2000je001427
Abstract
No abstract availableKeywords
This publication has 42 references indexed in Scilit:
- Global climate model high‐obliquity solutions to the ancient climate puzzles of the Faint‐Young Sun Paradox and low‐altitude Proterozoic glaciationJournal of Geophysical Research: Atmospheres, 2000
- Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth–Moon dynamics and palaeoclimateSedimentary Geology, 1998
- Habitable Planets with High ObliquitiesIcarus, 1997
- Climate and ice-sheet mass balance at the last glacial maximum from the GENESIS version 2 global climate modelQuaternary Science Reviews, 1997
- Paleomagnetic evidence for low-latitude glaciation during deposition of the Neoproterozoic Rapitan Group, Mackenzie Mountains, N.W.T., CanadaCanadian Journal of Earth Sciences, 1997
- Atmospheric carbon dioxide concentrations before 2.2 billion years agoNature, 1995
- History of the earth's obliquityEarth-Science Reviews, 1993
- The chaotic obliquity of the planetsNature, 1993
- Length of day and obliquity of the ecliptic 850 MA ago: Preliminary results of a stromatolite growth modelGeophysical Research Letters, 1982
- Precambrian Geologic HistoryScience, 1976