Search Publications

Insights into surface runoff on early Mars from paleolake basin morphology and stratigraphy
DOI: 10.1130/G37734.1 Bibcode: 2016Geo....44..419G

Mustard, John F.; Goudge, Timothy A.; Head, James W. +2 more

2016 Geology
MEx 70
Preserved glass-rich impactites on Mars
DOI: 10.1130/G36953.1 Bibcode: 2015Geo....43..635C

Mustard, J. F.; Cannon, K. M.

2015 Geology
MEx 40
Retreat of a giant cataract in a long-lived (3.7-2.6 Ga) martian outflow channel
DOI: 10.1130/G31268.1 Bibcode: 2010Geo....38..791W

Warner, N. H.; Gupta, S.; Muller, J. -P. +2 more

2010 Geology
MEx 25
Unique chronostratigraphic marker in depositional fan stratigraphy on Mars: Evidence for ca. 1.25 Ma gully activity and surficial meltwater origin
DOI: 10.1130/G25398A.1 Bibcode: 2009Geo....37..207S

Head, J. W.; Fassett, C. I.; Schon, S. C.

2009 Geology
MEx 98
Salt tectonics and collapse of Hebes Chasma, Valles Marineris, Mars
DOI: 10.1130/G30024A.1 Bibcode: 2009Geo....37..691A

Combe, J. -P.; Adams, J. B.; Gillespie, A. R. +4 more

2009 Geology
MEx 26
Late Amazonian glaciation at the dichotomy boundary on Mars: Evidence for glacial thickness maxima and multiple glacial phases
DOI: 10.1130/G24382A.1 Bibcode: 2008Geo....36..411D

Head, James W.; Marchant, David R.; Dickson, James L.

Lineated valley fill (LVF) in fretted valleys at the dichotomyboundary has been interpreted as glacial in origin. Unknownare (1) the original thickness of the glacier ice, (2) the amountof ice-surface lowering, through sublimation and retreat, toits presently observed level, and (3) whether there were multipleperiods of glaciation. We address thes…

2008 Geology
MEx 108
The Huygens-Hellas giant dike system on Mars: Implications for Late Noachian Early Hesperian volcanic resurfacing and climatic evolution
DOI: 10.1130/G22163.1 Bibcode: 2006Geo....34..285H

Head, J. W.; Neukum, G.; Wilson, L. +1 more

Two narrow, broadly arcuate, low ridges extend for 600 700 km in western Terra Tyrrhena, Mars, crosscut ancient Noachian terrain, and are associated with Early Hesperian plains, which cover ∼30% of Mars. Geological relationships suggest that the ridges represent near-surface erosional remnants of subsurface dikes, solidified magma-filled cracks th…

2006 Geology
MEx 67