Recent low-latitude freeze–thaw on Mars

Page, David P.

doi:10.1016/j.icarus.2007.01.005

Cited by 61 publications

(40 citation statements)

References 117 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…1) and across the wider Cerberus Plains region (Page, 2007). A periglacial origin has been proposed for this assemblage of landforms on morphologic , and stratigraphic (Page, 2008;Page and Murray, 2006) grounds, with the catastrophic floods that carved the channels thought to have also supplied the Fig.…”

Section: Introductionmentioning

confidence: 87%

“…Stable, low-latitude, low-elevation ground ice is not predicted by models, yet low-latitude, low-elevation, decameter-scale, patterned grounds, ring-mound landforms, and shallow "thermokarstlike" pits do, in fact, exist Jaeger et al, 2007;Lanagan et al, 2001;Page, 2007;Page and Murray, 2006), especially within the outflow channel Athabasca Vallis, the downstream basins and channels in the Elysium Planitia region that it supplies ( Fig. 1) and across the wider Cerberus Plains region (Page, 2007).…”

Section: Introductionmentioning

confidence: 99%

See 1 more Smart Citation

Sorted stone circles in Elysium Planitia, Mars: Implications for recent martian climate

Balme

Gallagher

Page

et al. 2009

Icarus

View full text Add to dashboard Cite

Section: Introductionmentioning

confidence: 87%

Section: Introductionmentioning

confidence: 99%

Sorted stone circles in Elysium Planitia, Mars: Implications for recent martian climate

Balme

Gallagher

Page

et al. 2009

Icarus

View full text Add to dashboard Cite

“…We have demonstrated that the RMLs and polygonal terrain central to this interpretation are both postdepositional in origin [cf. (9,10)]. …”

mentioning

confidence: 99%

Comment on "Athabasca Valles, Mars: A Lava-Draped Channel System"

Page

2008

Science

Self Cite

View full text Add to dashboard Cite

show abstract

“…pingos: e.g. Burr et al 2005;Page 2007) and mud volcanism (Farrand et al 2005). Recent detailed surveys have shown that small cone groups in Tartarus Colles (Hamilton et al 2011), and in Athabasca Valles and Cerberus Palus (Keszthelyi et al 2010), probably formed by rootless eruptions.…”

Section: Volcanic Landformsmentioning

confidence: 99%

Volcanism and tectonism across the inner solar system: an overview

Platz

Byrne

Massironi

et al. 2014

View full text Add to dashboard Cite

Volcanism and tectonism are the dominant endogenic means by which planetary surfaces change. This book, in general, and this overview, in particular, aim to encompass the broad range in character of volcanism, tectonism, faulting and associated interactions observed on planetary bodies across the inner solar system -a region that includes Mercury, Venus, Earth, the Moon, Mars and asteroids. The diversity and breadth of landforms produced by volcanic and tectonic processes are enormous, and vary across the inventory of inner solar system bodies. As a result, the selection of prevailing landforms and their underlying formational processes that are described and highlighted in this review are but a primer to the expansive field of planetary volcanism and tectonism. In addition to this extended introductory contribution, this Special Publication features 21 dedicated research articles about volcanic and tectonic processes manifest across the inner solar system. Those articles are summarized at the end of this review.

show abstract

Recent low-latitude freeze–thaw on Mars

Cited by 61 publications

References 117 publications

Sorted stone circles in Elysium Planitia, Mars: Implications for recent martian climate

Sorted stone circles in Elysium Planitia, Mars: Implications for recent martian climate

Comment on "Athabasca Valles, Mars: A Lava-Draped Channel System"

Volcanism and tectonism across the inner solar system: an overview

Contact Info

Product

Resources

About