FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4285012915> ?p ?o ?g. }

• W4285012915 endingPage "117699" @default.
• W4285012915 startingPage "117699" @default.
• W4285012915 abstract "Although the nature of the early Martian climate is a matter of considerable debate, the presence of valley networks (VN) provides unambiguous evidence for the presence of liquid water on Mars' surface. A subaerial fluvial origin of VN is at odds with the expected phase instability of near-surface water in the cold, dry Late Noachian climate. Furthermore, many geomorphic properties of VN (e.g., deep U-shaped valleys with constant widths; longitudinal profile reversals) are inconsistent with surface water flow. Conversely, subglacial channels exhibit many of these characteristics and could have persisted beneath ice sheets even in a cold climate. Here we model basal melting beneath a Late Noachian Icy Highlands ice sheet and map subglacial hydrological flow paths to investigate the distribution and geomorphometry of subglacial channels. We show that subglacial processes produce enough melt water to carve Mars' VN; that predicted channel distribution is consistent with observations; and corroborate reversed channel gradient measurements of VN consistent with subglacial formation mechanisms. We suggest that, given a sufficient historical global water inventory and Late Noachian geothermal heat flux, subglacial hydrology may have played a significant role in the surface modification of Mars. Plain language summary. Thousands of valley networks on Mars appear to have been carved by flowing water, and exhibit branching characteristics akin to river networks on Earth. Their origins, however, remain enigmatic for two primary reasons. First, ancient Mars was potentially cold, dry, and unable to support liquid water on its surface. Second, many physical characteristics of the valleys are inconsistent with features formed by precipitation and runoff. On Earth, water flowing beneath ice sheets produces channels with similar characteristics to Mars' valley networks. Here we model the deposition and evolution of Martian ice sheets and show that melting at the ice sheet base is likely even under cold and dry surface conditions. The volume, regional distribution, and flow patterns of melt are consistent with the volume and dynamics needed to carve the observed valley networks. A subglacial origin for Mars' valley networks accounts for their formation in a cold, dry climate and produces valley characteristics that match observations." @default.
• W4285012915 created "2022-07-12" @default.
• W4285012915 creator A5021653279 @default.
• W4285012915 creator A5042908854 @default.
• W4285012915 creator A5056282502 @default.
• W4285012915 creator A5078151990 @default.
• W4285012915 creator A5082936195 @default.
• W4285012915 date "2022-09-01" @default.
• W4285012915 modified "2023-09-28" @default.
• W4285012915 title "Revisiting subglacial hydrology as an origin for Mars' valley networks" @default.
• W4285012915 cites W1484710375 @default.
• W4285012915 cites W1492950700 @default.
• W4285012915 cites W1498786100 @default.
• W4285012915 cites W1520565385 @default.
• W4285012915 cites W1526636882 @default.
• W4285012915 cites W1612534022 @default.
• W4285012915 cites W1834351883 @default.
• W4285012915 cites W1875794043 @default.
• W4285012915 cites W1964386491 @default.
• W4285012915 cites W1966903975 @default.
• W4285012915 cites W1978674490 @default.
• W4285012915 cites W1981061458 @default.
• W4285012915 cites W1981285817 @default.
• W4285012915 cites W1982678971 @default.
• W4285012915 cites W1983571399 @default.
• W4285012915 cites W198461670 @default.
• W4285012915 cites W1986859129 @default.
• W4285012915 cites W1987169966 @default.
• W4285012915 cites W1988997534 @default.
• W4285012915 cites W1993611590 @default.
• W4285012915 cites W1994836202 @default.
• W4285012915 cites W2014607400 @default.
• W4285012915 cites W2016149291 @default.
• W4285012915 cites W2018800485 @default.
• W4285012915 cites W2022594017 @default.
• W4285012915 cites W2028134116 @default.
• W4285012915 cites W2032433525 @default.
• W4285012915 cites W2039319719 @default.
• W4285012915 cites W2050012108 @default.
• W4285012915 cites W2056505499 @default.
• W4285012915 cites W2064128523 @default.
• W4285012915 cites W2064679800 @default.
• W4285012915 cites W2079799239 @default.
• W4285012915 cites W2083483943 @default.
• W4285012915 cites W2085012469 @default.
• W4285012915 cites W2085982749 @default.
• W4285012915 cites W2089567445 @default.
• W4285012915 cites W2089939271 @default.
• W4285012915 cites W2093000948 @default.
• W4285012915 cites W2099887084 @default.
• W4285012915 cites W2105641585 @default.
• W4285012915 cites W2106111282 @default.
• W4285012915 cites W2109184821 @default.
• W4285012915 cites W2113162852 @default.
• W4285012915 cites W2113634331 @default.
• W4285012915 cites W2119534769 @default.
• W4285012915 cites W2120077698 @default.
• W4285012915 cites W2120449497 @default.
• W4285012915 cites W2121446820 @default.
• W4285012915 cites W2129829709 @default.
• W4285012915 cites W2133044191 @default.
• W4285012915 cites W2135955237 @default.
• W4285012915 cites W2139315028 @default.
• W4285012915 cites W2157738344 @default.
• W4285012915 cites W2289749624 @default.
• W4285012915 cites W2424964397 @default.
• W4285012915 cites W2555613453 @default.
• W4285012915 cites W2586433278 @default.
• W4285012915 cites W2605964051 @default.
• W4285012915 cites W2624196263 @default.
• W4285012915 cites W2769527114 @default.
• W4285012915 cites W2782467850 @default.
• W4285012915 cites W2794946512 @default.
• W4285012915 cites W2796812396 @default.
• W4285012915 cites W2800384049 @default.
• W4285012915 cites W2805049639 @default.
• W4285012915 cites W2811168270 @default.
• W4285012915 cites W2884720674 @default.
• W4285012915 cites W2885885535 @default.
• W4285012915 cites W2913306397 @default.
• W4285012915 cites W2963184437 @default.
• W4285012915 cites W2982993401 @default.
• W4285012915 cites W2983548508 @default.
• W4285012915 cites W3104628389 @default.
• W4285012915 cites W3106263859 @default.
• W4285012915 cites W3106689788 @default.
• W4285012915 cites W3124581147 @default.
• W4285012915 cites W4247077355 @default.
• W4285012915 doi "https://doi.org/10.1016/j.epsl.2022.117699" @default.
• W4285012915 hasPublicationYear "2022" @default.
• W4285012915 type Work @default.
• W4285012915 citedByCount "3" @default.
• W4285012915 countsByYear W42850129152022 @default.
• W4285012915 countsByYear W42850129152023 @default.
• W4285012915 crossrefType "journal-article" @default.
• W4285012915 hasAuthorship W4285012915A5021653279 @default.
• W4285012915 hasAuthorship W4285012915A5042908854 @default.
• W4285012915 hasAuthorship W4285012915A5056282502 @default.

• next