The DOI matches its Crossref record; 45 of the 46 references it cites were found in a registry or an index.
Ancient oceans, ice sheets and the hydrological cycle on Mars
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“Geomorphic evidence for the latter includes mottled plains, shorelines, terraced slopes, and layered sediments”
From A chemical model for evaporites on early Mars: Possible sedimentary tracers of the early climate and implications for exploration (1999) · cites this paper as Baker et al., 1991
In the citing paper
“The evidence for punctuated, impact-driven interaction between rocks and fluids supports scenarios such as those of Segura et al. (2002), where large impacts created temporary hydrous environments, as opposed to those including largescale, long-term hydrologic systems including oceans (Baker et al. 1991; Clifford and Parker 2001).”
From Multi-generational carbonate assemblages in martian meteorite Allan Hills 84001: Implications for nucleation, growth, and alteration (2004) · cites this paper as Baker et al. 1991
Citations
Cites
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Research works printed but not linked: 12
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Items 201–300 of 715
Tharsis recharge: A source of groundwater for Martian outflow channels
Harrison, K. P., & Grimm, R. E. (2004) · Geophysical Research Letters · doi:10.1029/2004gl020502 · Cited by 63
“We propose that recharge at the Tharsis rise, which was largely in place by the late Noachian [Phillips et al., 2001], provides a high elevation source of discharge to the outflow channels and further constrains postulated hydrologic links to the circum-Chryse outflow channels [ Baker et al., 2001 ].”
BackgroundMethane bursts as a trigger for intermittent lake-forming climates on post-Noachian Mars
Kite, E. S., Gao, P., Goldblatt, C., Mischna, M. A., Mayer, D. P., & Yung, Y. L. (2017) · Nature Geoscience · doi:10.1038/ngeo3033 · Cited by 63
Early hydrous melting and degassing of the Martian interior
Médard, É., & Grove, T. L. (2006) · Journal of Geophysical Research Atmospheres · doi:10.1029/2006je002742 · Cited by 62
“The evidence from surface geology of recurrent fluvial processes on the surface of the planet [Baker et al., 1991], extensive alteration of the Martian surface [Haskin et al., 2005] and abundant sulfate deposits [Squyres and Knoll, 2005] indicates that H 2 O was incorporated into Mars and has…”
Bishop, J. L., Banin, A., Mancinelli, R. L., & Klovstad, M. R. (2002) · Planetary and Space Science · doi:10.1016/s0032-0633(01)00077-0 · Cited by 62
Volcano-Ice Interaction as a Microbial Habitat on Earth and Mars
Cousins, C. R., & Crawford, I. (2011) · Astrobiology · doi:10.1089/ast.2010.0550 · Cited by 61
Rice, J. W., & Edgett, K. S. (1997) · Journal of Geophysical Research Atmospheres · doi:10.1029/96je02824 · Cited by 62
An ESA study for the search for life on Mars
Westall, F., Brack, A., Hofmann, B. A., Horneck, G., Kurat, G., Maxwell, J. R., Ori, G. G., Pillinger, C. T., Raulin, F., Thomas, N., et al. (2000) · Planetary and Space Science · doi:10.1016/s0032-0633(99)00090-2 · Cited by 62
Geological Processes and Evolution
Head, J. W., III, Greeley, R., Golombek, M. P., HARTMANN, W. K., Hauber, E., Jaumann, R., Masson, P. L., Neukum, G., Nyquist, L. E., & Carr, M. H. (2001) · Space Science Reviews · doi:10.1023/a:1011953424736 · Cited by 62
Fluvial Valley Networks on Mars
Irwin, R. P., Howard, A. D., & Craddock, R. A. (2008) · Wiley eBooks · doi:10.1002/9780470760383.ch19 · Cited by 63
Evidence for remnants of ancient ice‐rich deposits: Mangala Valles outflow channel, Mars
Levy, J. S., & Head, J. W., III (2005) · Terra Nova · doi:10.1111/j.1365-3121.2005.00642.x · Cited by 61
“Baker et al., 1991; Carr, 1996; Kreslavsky and Head, 2002).”
BackgroundSulfur in the early martian atmosphere revisited: Experiments with a 3-D Global Climate Model
Kerber, L., Forget, F., & Wordsworth, R. (2015) · Icarus · doi:10.1016/j.icarus.2015.08.011 · Cited by 61
Howard, A. D., & Moore, J. M. (2011) · Journal of Geophysical Research Atmospheres · doi:10.1029/2010je003782 · Cited by 60
“Water delivered to the northern lowlands by the outflow channels, therefore, may have been recycled as snow and ice deposits within the Martian midlatitudes as suggested by Baker et al. [1991] and Moore et al. [1995].”
BackgroundSeybold, H., Kite, E. S., & Kirchner, J. W. (2018) · Science Advances · doi:10.1126/sciadv.aar6692 · Cited by 64
Morphogenesis of Antarctic Paleosols: Martian Analogue
Mahaney, W. M. (2001) · Icarus · doi:10.1006/icar.2001.6667 · Cited by 60
The role of Raman spectroscopy as an astrobiological tool in the exploration of Mars
Ellery, A., Wynn-Williams, D., Parnell, J., Edwards, H., & Dickensheets, D. (2004) · Journal of Raman Spectroscopy · doi:10.1002/jrs.1189 · Cited by 61
Evidence for marine sedimentary rocks in Utopia Planitia: Zhurong rover observations
Xiao, L., Huang, J., Kusky, T., Head, J. W., III, Zhao, J., Wang, J., Wang, L., Yu, W., Shi, Y., Wu, B., et al. (2023) · National Science Review · doi:10.1093/nsr/nwad137 · Cited by 60
On the origin of the Vastitas Borealis Formation in Chryse and Acidalia Planitiae, Mars
Salvatore, M. R., & Christensen, P. R. (2014) · Journal of Geophysical Research Planets · doi:10.1002/2014je004682 · Cited by 63
“…et al., 2003, 2005; Fairén et al., 2003; Parker et al., 1989, 1993, 2010; Mellon et al., 2004, 2008; Mustard et al., 2001; Milliken et al., 2003; Baker et al., 1991; Costard and Kargel, 1995; Kreslavsky and Head, 2002; McGowan, 2009; Oehler and Allen, 2012a, 2014; Clifford et al., 2013;…”
Microbial Ecology: Caves as an Extreme Habitat
Gabriel, C. R., & Northup, D. (2013) · SpringerBriefs in microbiology · doi:10.1007/978-1-4614-5206-5_5 · Cited by 58
Martian hydrogeology sustained by thermally insulating gas and salt hydrates
Kargel, J. S., Furfaro, R., Prieto‐Ballesteros, O., Rodriguez, J. A. P., Montgomery, D. R., Gillespie, A. R., Marion, G. M., & Wood, S. E. (2007) · Geology · doi:10.1130/g23783a.1 · Cited by 59
Self-citationScenarios for the evolution of life on Mars
Schulze‐Makuch, D., Irwin, L. N., Lipps, J. H., LeMone, D. V., Dohm, J. M., & Fairén, A. G. (2005) · Journal of Geophysical Research Atmospheres · doi:10.1029/2005je002430 · Cited by 59
“…at least into the Middle Noachian followed by persisting dry and cold periods interrupted mainly by shortduration pulses (perhaps 103 to 104 years [Baker et al., 1991]) of endogenic-driven activity, especially at Tharsis and the surrounding regions [Dohm et al., 2001a; Anderson et al., 2001].”
BackgroundLeask, H. J., Wilson, L., & Mitchell, K. L. (2006) · Journal of Geophysical Research Atmospheres · doi:10.1029/2005je002550 · Cited by 58
“The combination of these factors causes fracturing of the cryosphere, thus allowing pressurized water to rise into the fractures [Masursky et al., 1977; Theilig and Greeley, 1979; Baker et al., 1991; Chapman and Tanaka, 2002; Leask, 2005].”
Brack, A. (1999) · Advances in Space Research · doi:10.1016/s0273-1177(99)00457-3 · Cited by 56
“However, the presence of extensive coastlines at the border of the northern lowlands where the (( Valles 1) flow supports the presence of a large ocean in the Northern Hemisphere (Baker et al., 1991).”
BackgroundMoore, J. M., Clow, G. D., Davis, W. L., Gulick, V. C., Janke, D. R., McKay, C. P., Stoker, C. R., & Zent, A. P. (1995) · Journal of Geophysical Research Atmospheres · doi:10.1029/94je02805 · Cited by 58
Self-citationFishbaugh, K. E., & Head, J. W., III (2000) · Journal of Geophysical Research Atmospheres · doi:10.1029/1999je001230 · Cited by 58
de Pablo, M. A., Michael, G. G., & Centeno, J. D. (2013) · Icarus · doi:10.1016/j.icarus.2013.05.012 · Cited by 57
Martian outflow channels: How did their source aquifers form and why did they drain so rapidly?
Rodriguez, J. A. P., Kargel, J. S., Baker, V. R., Gulick, V. C., Berman, D. C., Fairén, A. G., Linares, R., Zarroca, M., Yan, J., Miyamoto, H., et al. (2015) · Scientific Reports · doi:10.1038/srep13404 · Cited by 57
Self-citationFormation and mantling ages of lobate debris aprons on Mars: Insights from categorized crater counts
Berman, D. C., Crown, D. A., & Joseph, E. C. S. (2015) · Planetary and Space Science · doi:10.1016/j.pss.2015.03.013 · Cited by 57
Comparison of small lunar landslides and martian gullies
Bart, G. D. (2006) · Icarus · doi:10.1016/j.icarus.2006.11.004 · Cited by 57
Numerical modeling for target water depth estimation of marine‐target impact craters
Ormö, J., Shuvalov, V. V., & Lindström, M. (2002) · Journal of Geophysical Research Atmospheres · doi:10.1029/2002je001865 · Cited by 57
The Medusae Fossae Formation as the single largest source of dust on Mars
Ojha, L., Lewis, K. W., Karunatillake, S., & Schmidt, M. E. (2018) · Nature Communications · doi:10.1038/s41467-018-05291-5 · Cited by 56
Glaciovolcanic hydrothermal environments in Iceland and implications for their detection on Mars
Cousins, C. R., Crawford, I., Carrivick, J. L., Gunn, M. D., Harris, J. K., Kee, T. P., Karlsson, M., Carmody, L., Cockell, C. S., Herschy, B., et al. (2013) · Journal of Volcanology and Geothermal Research · doi:10.1016/j.jvolgeores.2013.02.009 · Cited by 60
“Aqueous floods have certainly played a major role in Mars surface processes (e.g. Warner et al., 2009), although the origin of these floods is often contested or uncertain (Baker et al., 1991; Baker, 2001).”
Background3D modelling of the climatic impact of outflow channel formation events on early Mars
Turbet, M., Forget, F., Head, J. W., III, & Wordsworth, R. (2017) · Icarus · doi:10.1016/j.icarus.2017.01.024 · Cited by 58
Fractionated martian atmosphere in the nakhlites?
DRAKE, M. J., Swindle, T. D., Owen, T., & Musselwhite, D. S. (1994) · Meteoritics · doi:10.1111/j.1945-5100.1994.tb01099.x · Cited by 55
Moscardelli, L. G., & Wood, L. J. (2011) · Geology · doi:10.1130/g31949.1 · Cited by 54
Volcanism and Ice Interactions on Earth and Mars
Chapman, M. G., Allen, C. C., Guðmundsson, M. T., Gulick, V. C., Jakobsson, S. P., LUCCHITTA, B. K., Skilling, I. P., & Waitt, R. B. (2000) · Springer eBooks · doi:10.1007/978-1-4615-4151-6_3 · Cited by 54
Self-citationDávila, A. F., Fairén, A. G., Gago-Duport, L., Stoker, C. R., Amils, R., Bonaccorsi, R., Zavaleta, J., Lim, D. S. S., Schulze‐Makuch, D., & McKay, C. P. (2008) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2008.05.015 · Cited by 54
Geomorphologic Evidence for Liquid Water
Masson, P. L., Carr, M. H., Costard, F., Greeley, R., Hauber, E., & Ralf Jaumann, E. (2001) · Space Science Reviews · doi:10.1023/a:1011913809715 · Cited by 55
Ivanov, M. A., Erkeling, G., Hiesinger, H., Bernhardt, H., & Reiss, D. (2017) · Planetary and Space Science · doi:10.1016/j.pss.2017.05.012 · Cited by 53
“…existed, the ocean-sized body of water thousands of kilometers wide may have seriously influenced the climate/atmospheric conditions on Mars (e.g., Baker et al., 1991; Villanueva et al., 2015) and leaved recognizable evidence of its presence in the geological record of the planet (Parker et al.,…”
BackgroundPersistent or repeated surface habitability on Mars during the late Hesperian ‐ Amazonian
Kite, E. S., Sneed, J., Mayer, D. P., & Wilson, S. A. (2017) · Geophysical Research Letters · doi:10.1002/2017gl072660 · Cited by 53
Wharton, R. A., Crosby, J. M., McKay, C. P., & Rice, J. W. (1995) · Journal of Paleolimnology · doi:10.1007/bf00682769 · Cited by 50
CORRIGAN, C. M., & HARVEY, R. P. (2004) · Meteoritics & Planetary Science · doi:10.1111/j.1945-5100.2004.tb00047.x · Cited by 50
On the role of widespread subsurface convection in bringing liquid water close to Mars' surface
Travis, B. J., Rosenberg, N. D., & Cuzzi, J. N. (2003) · Journal of Geophysical Research Atmospheres · doi:10.1029/2002je001877 · Cited by 52
Geomorphological Evidence for Water on Mars
Baker, V. R. (2006) · Elements · doi:10.2113/gselements.2.3.139 · Cited by 52
Self-citationWater soluble ions in the Nakhla martian meteorite
Sawyer, D. J., McGehee, M. D., Canepa, J., & Moore, C. (2000) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.2000.tb01458.x · Cited by 56
Gas Hydrates in Convergent Margins: Formation, Occurrence, Geochemistry, and Global Significance
Kastner, M. (2011) · Geophysical monograph · doi:10.1029/gm124p0067 · Cited by 51
Flow rates and duration within Kasei Valles, Mars: Implications for the formation of a Martian Ocean
Williams, R. M. E., Phillips, R. J., & Malin, M. C. (2000) · Geophysical Research Letters · doi:10.1029/1999gl010957 · Cited by 51
“This ocean may have formed episodically [Baker et al., 1991] and several contact/shoreline boundaries have been identified [e.g., Parker et al., 1993].”
BackgroundDegradation of mid-latitude craters on Mars
Berman, D. C., Crown, D. A., & Bleamaster, L. F. (2008) · Icarus · doi:10.1016/j.icarus.2008.10.026 · Cited by 51
Where is the nitrogen on Mars?
Mancinelli, R. L., & Banin, A. (2003) · International Journal of Astrobiology · doi:10.1017/s1473550403001599 · Cited by 51
Barlow, N. G., Koroshetz, J., & Dohm, J. M. (2001) · Geophysical Research Letters · doi:10.1029/2000gl012804 · Cited by 50
Traits and Evolution of the Tharsis Superplume, Mars
Dohm, J. M., Baker, V. R., Maruyama, S., & Anderson, R. C. (2007) · Springer eBooks · doi:10.1007/978-1-4020-5750-2_17 · Cited by 49
Self-citationElevations of water‐worn features on Mars: Implications for circulation of groundwater
Carr, M. H. (2002) · Journal of Geophysical Research Atmospheres · doi:10.1029/2002je001845 · Cited by 50
Formation and disruption of aquifers in southwestern Chryse Planitia, Mars
Rodriguez, J. A. P., Tanaka, K. L., Kargel, J. S., Dohm, J. M., Kuzmin, R. O., Fairén, A. G., Sasaki, S., Komatsu, G., Schulze‐Makuch, D., & Jianguo, Y. (2007) · Icarus · doi:10.1016/j.icarus.2007.05.021 · Cited by 48
Self-citationEvidence for late Hesperian lacustrine activity in Shalbatana Vallis, Mars
Achille, G. D., Ori, G. G., & Reiss, D. (2007) · Journal of Geophysical Research Atmospheres · doi:10.1029/2006je002858 · Cited by 48
“5.3. Age Dating and Stratigraphic Implications [37] Although it is thought that main Martian hydrological activity occurred in the late Noachian [e.g., Carr, 1996; Irwin et al., 2005; Bibring et al., 2006], several authors have suggested that valley reactivations and some new valley developments could have occurred du…”
BackgroundInfluentialRock glaciers on Mars: Earth-based clues to Mars’ recent paleoclimatic history
Mahaney, W. C., Miyamoto, H., Dohm, J. M., Baker, V. R., Cabrol, N. A., Grin, E. A., & Berman, D. C. (2006) · Planetary and Space Science · doi:10.1016/j.pss.2006.04.016 · Cited by 48
Self-citationErkeling, G., Reiss, D., Hiesinger, H., Poulet, F., Carter, J., Ivanov, M. A., Hauber, E., & Ralf Jaumann, E. (2012) · Icarus · doi:10.1016/j.icarus.2012.03.012 · Cited by 48
Williams, R. M. E., & Weitz, C. M. (2014) · Icarus · doi:10.1016/j.icarus.2014.06.030 · Cited by 46
Schulze‐Makuch, D., Dohm, J. M., Fairén, A. G., Baker, V. R., Fink, W., & STROM, R. G. (2005) · Astrobiology · doi:10.1089/ast.2005.5.778 · Cited by 47
Self-citationSearching for Biosignatures Using Electron Paramagnetic Resonance (EPR) Analysis of Manganese Oxides
Kim, S. S., Bargar, J., Nealson, K. H., Flood, B. E., Kirschvink, J. L., Raub, T. D., Tebo, B. M., & Villalobos, M. (2011) · Astrobiology · doi:10.1089/ast.2011.0619 · Cited by 47
Amagmatic hydrothermal systems on Mars from radiogenic heat
Ojha, L., Karunatillake, S., Karimi, S., & Buffo, J. (2021) · Nature Communications · doi:10.1038/s41467-021-21762-8 · Cited by 49
Formation of Aromatum Chaos, Mars: Morphological development as a result of volcano‐ice interactions
Leask, H. J., Wilson, L., & Mitchell, K. L. (2006) · Journal of Geophysical Research Atmospheres · doi:10.1029/2005je002549 · Cited by 47
“Aromatum Chaos and elsewhere, is the discharge of pressurized water from beneath the cryosphere, which results in the collapse of overlying terrain [Masursky et al., 1977; Baker and Kochel, 1979; Carr, 1979; Theilig and Greeley, 1979; Baker et al., 1991; Lucchitta et al., 1994; Cabrol et al., 1997; Coleman, 2003; Chap…”
BackgroundHypsometric analysis of Margaritifer Sinus and origin of valley networks
Luo, W. (2002) · Journal of Geophysical Research Atmospheres · doi:10.1029/2001je001500 · Cited by 46
Leask, H. J., Wilson, L., & Mitchell, K. L. (2007) · Journal of Geophysical Research Atmospheres · doi:10.1029/2006je002851 · Cited by 47
Schulze‐Makuch, D., Fairén, A. G., & Dávila, A. F. (2008) · International Journal of Astrobiology · doi:10.1017/s1473550408004175 · Cited by 49
Canyon formation constraints on the discharge of catastrophic outburst floods of Earth and Mars
Lapôtre, M. G. A., Lamb, M. P., & Williams, R. M. E. (2016) · Journal of Geophysical Research Planets · doi:10.1002/2016je005061 · Cited by 46
Warner, N. H., Gupta, S., Kim, J., Lin, S., & Müller, J. (2010) · Geology · doi:10.1130/g30579.1 · Cited by 46
Karunatillake, S., SQUYRES, S. W., Taylor, G. J., Keller, J. M., Gasnault, O., Evans, L. G., Reedy, R. C., Starr, R. D., Boynton, W. V., Janes, D. M., et al. (2006) · Journal of Geophysical Research Atmospheres · doi:10.1029/2006je002675 · Cited by 46
“Such mixing may be due in part to late-stage, Tharsis (and to a lesser extent, Elysium [Tanaka et al., 2003]) -related flood inundations [ Baker et al., 1991; Dohm et al., 2001a, 2001b], which Faire´n et al. [2003] hypothesized to be transient, be laden with sediments, and postdate a more extensive Noachian-era ocean.”
BackgroundRift zone volcanism and associated cinder cone field in Utopia Planitia, Mars
Lanz, J. K., Wagner, R., Wolf, U., Kröchert, J., & Neukum, G. (2010) · Journal of Geophysical Research Atmospheres · doi:10.1029/2010je003578 · Cited by 49
Komatsu, G., Kumar, P. S., Goto, K., Sekine, Y., Giri, C., & Matsui, T. (2013) · Planetary and Space Science · doi:10.1016/j.pss.2013.05.011 · Cited by 45
“However, it has been hypothesized that Mars has experienced periods drastically different from today, sometimes involving even liquid water on a global scale because of climate change (Baker et al., 1991; Craddock and Maxwell, 1993) or at localized areas due to magmatic, tectonic processes, or impact cratering (Braken…”
Self-citationSánchez, F. J., Mateo‐Martí, E., Raggio, J., Meeßen, J., Martínez‐Frías, J., Sancho, L. G., Ott, S., & de la Torre, R. (2012) · Planetary and Space Science · doi:10.1016/j.pss.2012.08.005 · Cited by 44
Fastook, J. L., Head, J. W., III, Forget, F., Madeleine, J., & Marchant, D. R. (2011) · Icarus · doi:10.1016/j.icarus.2011.07.018 · Cited by 45
“He cited: (1) the fact that the glacial hypotheses requires major climate change late in Mars history (e.g., Baker et al., 1991) for which he found little supporting evidence and (2) that the low erosion rates in the Amazonian argues against any major climate excursions accompanied by…”
BackgroundImage resolution and evaluation of genetic hypotheses for planetary landscapes
Zimbelman, J. R. (2001) · Geomorphology · doi:10.1016/s0169-555x(00)00082-9 · Cited by 45
Marine‐target craters on Mars? An assessment study
Ormö, J., Dohm, J. M., Ferris, J. C., Lepinette, A., & Fairén, A. G. (2004) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.2004.tb00344.x · Cited by 46
“The MEGAOUTFLO hypothesis (Baker et al. 2000) first proposed by Baker et al. (1991) genetically links episodic magmatic-driven activity with floods that pond in the northern lowlands to form oceans and associated relatively short-lived climatic perturbations (duration of tens of thousands of years).”
BackgroundMethodInfluentialOxygen isotopic record of silicate alteration in the Shergotty—Nakhla—Chassigny meteorite Lafayette
Romanek, C. S., Perry, E. C., Treiman, A. H., Socki, R. A., JONES, J. H., & Gibson, E. K. (1998) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.1998.tb01683.x · Cited by 45
Low‐frequency electromagnetic exploration for groundwater on Mars
Grimm, R. E. (2002) · Journal of Geophysical Research Atmospheres · doi:10.1029/2001je001504 · Cited by 45
Circumpolar ocean stability on Mars 3 Gy ago
Schmidt, F., Way, M. J., Costard, F., Bouley, S., Séjourné, A., & Aleinov, I. (2022) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.2112930118 · Cited by 51
“At the same time that Life spread on Earth (3 Gy ago), the Red Planet was possibly more similar to our Blue Planet.”
BackgroundInfluentialIsotopic and petrographic evidence for young Martian basalts
Walton, E. L., Kelley, S. P., & Herd, C. D. K. (2008) · Geochimica et Cosmochimica Acta · doi:10.1016/j.gca.2008.09.005 · Cited by 45
Formation of Hrad Vallis (Mars) by low viscosity lava flows
Hopper, J. P., & Leverington, D. W. (2013) · Geomorphology · doi:10.1016/j.geomorph.2013.10.029 · Cited by 44
Banks, M. E., McEwen, A. S., Kargel, J. S., Baker, V. R., STROM, R. G., Mellon, M. T., Gulick, V. C., Keszthelyi, L. P., Herkenhoff, K. E., Pelletier, J. D., et al. (2008) · Journal of Geophysical Research Atmospheres · doi:10.1029/2007je002994 · Cited by 44
“This in turn implies that there was a substantial source for the moisture and that appropriate climatic conditions existed in which the moisture could be released from the reservoir and, if necessary, transported to the midlatitudes [e.g., Baker et al., 1991].”
BackgroundSelf-citationNewsom, H., & Hagerty, J. (1997) · Journal of Geophysical Research Atmospheres · doi:10.1029/97je01687 · Cited by 36
Bishop, J., Lougear, A., Newton, J., Doran, P., Froeschl, H., Trautwein, A., Körner, W., & Koeberl, C. (2001) · Geochimica et Cosmochimica Acta · doi:10.1016/s0016-7037(01)00651-2 · Cited by 42
“Paleolakes and lacustrine features on Mars have also been studied to explain the surface processes on Mars (Baker et al., 1991; Goldspiel and Squyres, 1991; Scott et al., 1991, 1992, 1995; Rice, 1992).”
BackgroundMars: a small terrestrial planet
Mangold, N., Baratoux, D., Witasse, O. G., Encrenaz, T. A., & Sotin, C. (2016) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-016-0099-5 · Cited by 49
Did the martian outflow channels mostly form during the Amazonian Period?
Rodriguez, J. A. P., Platz, T., Gulick, V. C., Baker, V. R., Fairén, A. G., Kargel, J. S., Yan, J., Miyamoto, H., & Glines, N. H. (2015) · Icarus · doi:10.1016/j.icarus.2015.04.024 · Cited by 42
Self-citationPutative shorelines in northern Arabia Terra, Mars
Webb, V. E. (2004) · Journal of Geophysical Research Atmospheres · doi:10.1029/2003je002205 · Cited by 42
“[3] The validity of these proposed shorelines on Mars has since been part of an ongoing controversy regarding the hydrologic and geomorphic development of the northern plains [e.g., Baker et al., 1991, 2002; Jo¨ns, 1991; Edgett and Parker, 1997; Malin and Edgett, 1999; Withers and Neumann, 2001; Buczkowski and McGill,…”
BackgroundOri, G. G., & Mosangini, C. (1998) · Journal of Geophysical Research Atmospheres · doi:10.1029/98je01969 · Cited by 42
Séjourné, A., Costard, F., Swirad, Z., Łosiak, A., Bouley, S., Smith, I. B., Balme, M. R., Orgel, C., Ramsdale, J., Hauber, E., et al. (2018) · Journal of Geophysical Research Planets · doi:10.1029/2018je005665 · Cited by 43
“During the Hesperian, these lowlands may have been the location of accumulation and later freezing of sediments from multiple episodes of outflow channel discharge and perhaps even from a large ocean (e.g., Baker et al., 1991; Carr & Head, 2003; Clifford & Parker, 2001; Parker et al., 1993).”
BackgroundRussell, P. S., & Head, J. W., III (2006) · Planetary and Space Science · doi:10.1016/j.pss.2006.03.010 · Cited by 41
Mars chronology: assessing techniques for quantifying surficial processes
Doran, P. T. (2004) · Earth-Science Reviews · doi:10.1016/j.earscirev.2004.04.001 · Cited by 41
Exobiological implications of potential sedimentary deposits on Mars
Komatsu, G., & Ori, G. (2000) · Planetary and Space Science · doi:10.1016/s0032-0633(00)00078-7 · Cited by 45
Self-citationA terrestrial model for an alkaline martian hydrosphere
Kempe, S., & Kaźmierczak, J. (1997) · Planetary and Space Science · doi:10.1016/s0032-0633(97)00116-5 · Cited by 41
Meresse, S., Costard, F., Mangold, N., Baratoux, D., & Boyce, J. M. (2006) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.2006.tb00442.x · Cited by 39
“The existence of large bodies of water during different periods of time on these plains has been previously proposed (McGill 1985; Lucchitta et al. 1986; Parker et al. 1989; Baker et al. 1991; Kreslavsky and Head 2002b; Boyce et al. 2005).”
BackgroundBalme, M. R., Gallagher, C. J., & Hauber, E. (2013) · Progress in Physical Geography Earth and Environment · doi:10.1177/0309133313477123 · Cited by 39
“…2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 For Peer Review excursions in the past by releasing large amounts of volatiles into the atmosphere (e.g., 81 Baker et al., 1991).”
Miyamoto, H., Ito, K., Komatsu, G., Baker, V. R., Dohm, J. M., Tosaka, H., & Sasaki, S. (2005) · Geomorphology · doi:10.1016/j.geomorph.2005.11.002 · Cited by 39
Self-citationTectonic histories between Alba Patera and Syria Planum, Mars
Anderson, R. C., Dohm, J. M., Haldemann, A. F. C., Hare, T. M., & Baker, V. R. (2004) · Icarus · doi:10.1016/j.icarus.2004.04.018 · Cited by 39
“Along with the magmatic activity, the formation of Tharsis is considered to have triggered gigantic floods that ponded in the northern plains to form oceans and/or lakes, causing short-term hydrological cycles and relatively short-lived (tens of thousands of years) climatic perturbations from a common cold and dry Mar…”
BackgroundMethodSelf-citationNew evidence for a magmatic influence on the origin of Valles Marineris, Mars
Dohm, J. M., Williams, J. P., Anderson, R. C., Ruíz, J., McGuire, P. C., Komatsu, G., Dávila, A. F., Ferris, J. C., Schulze‐Makuch, D., Baker, V. R., et al. (2008) · Journal of Volcanology and Geothermal Research · doi:10.1016/j.jvolgeores.2008.11.029 · Cited by 39
Self-citationDelta Deposits on Mars: A Global Perspective
Toffoli, B. D., Plesa, A., Hauber, E., & Breuer, D. (2021) · Geophysical Research Letters · doi:10.1029/2021gl094271 · Cited by 40
Gómez, F., Aguilera, Á., & Amils, R. (2007) · Icarus · doi:10.1016/j.icarus.2007.04.008 · Cited by 38
Phosphates and carbon on Mars: Exobiological implications and sample return considerations
Mojzsis, S., & Arrhenius, G. (1998) · Journal of Geophysical Research Atmospheres · doi:10.1029/98je02141 · Cited by 33
Terraforming Mars: A review of current research
Fogg, M. J. (1998) · Advances in Space Research · doi:10.1016/s0273-1177(98)00166-5 · Cited by 38
Warner, N. H., & Farmer, J. D. (2010) · Astrobiology · doi:10.1089/ast.2009.0425 · Cited by 41
Constraints on the origin and evolution of Iani Chaos, Mars
Warner, N. H., Gupta, S., Kim, J., Müller, J., Corre, L. L., Morley, J. G., Lin, S., & McGonigle, C. (2011) · Journal of Geophysical Research Atmospheres · doi:10.1029/2010je003787 · Cited by 38
Metadata
- Authors
- Baker, V. R., Strom, R. G., Gulick, V. C., Kargel, J. S., Komatsu, G., & Kale, V. S.
- Affiliations
- University of Arizona (US)
- Savitribai Phule Pune University (IN)
- Venue
- Nature
- Published
- 1991-08
- Volume
- 352
- Issue
- 6336
- Pages
- 589-594
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W2019919661
- Cited by
- 714
- References
- 46
- Citations by year
- 2026: 16 · 2025: 13 · 2024: 24 · 2023: 22 · 2022: 28 · 2021: 21 · 2020: 22 · 2019: 21 · 2018: 24 · 2017: 16 · 2016: 13 · 2015: 22 · 2014: 25 · 2013: 19 · 2012: 21
- FWCI
- 21.03
- Type
- journal article
- Language
- en
- Update notices
- correction (1991-11-07)
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature (publishedVersion)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Earth-Surface Processes › Geological formations and processes
- Keywords
- Mars, ancient oceans, ice sheets, water cycle, valley networks, Tharsis volcanism, glaciation, Northern Plains, Southern Highlands, Martian paleoclimate
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