อ้างอิง ของ น้ำบนดาวอังคาร

  1. ↑ Jakosky, B.M.; Haberle, R.M. (1992). "The Seasonal Behavior of Water on Mars". ใน Kieffer, H.H.; และคณะ (บ.ก.). Mars. Tucson, AZ: University of Arizona Press. pp. 969–1016.
  2. 1 2 Ojha, L.; Wilhelm, M. B.; Murchie, S. L.; McEwen, A. S.; Wray, J. J.; Hanley, J.; Massé, M.; Chojnacki, M. (2015). "Spectral evidence for hydrated salts in recurring slope lineae on Mars". Nature Geoscience. doi:10.1038/ngeo2546.
  3. ↑ Carr, M.H. (1996). Water on Mars. New York: Oxford University Press. p. 197.
  4. ↑ Bibring, J.-P.; Langevin, Yves; Poulet, François; Gendrin, Aline; Gondet, Brigitte; Berthé, Michel; Soufflot, Alain; Drossart, Pierre; Combes, Michel; Bellucci, Giancarlo; Moroz, Vassili; Mangold, Nicolas; Schmitt, Bernard; Omega Team, the; Erard, S.; Forni, O.; Manaud, N.; Poulleau, G.; Encrenaz, T.; Fouchet, T.; Melchiorri, R.; Altieri, F.; Formisano, V.; Bonello, G.; Fonti, S.; Capaccioni, F.; Cerroni, P.; Coradini, A.; Kottsov, V.; และคณะ (2004). "Perennial Water Ice Identified in the South Polar Cap of Mars". Nature. 428 (6983): 627–630. Bibcode:2004Natur.428..627B. doi:10.1038/nature02461. PMID 15024393.
  5. ↑ "Water at Martian south pole". European Space Agency (ESA). March 17, 2004.
  6. ↑ "Mars Odyssey: Newsroom". Mars.jpl.nasa.gov. May 28, 2002.
  7. ↑ Feldman, W.C.; และคณะ (2004). "Global Distribution of Near-Surface Hydrogen on Mars". J. Geophysical Research. 109. Bibcode:2004JGRE..10909006F. doi:10.1029/2003JE002160.
  8. ↑
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  10. ↑ Hecht, M.H. (2002). "Metastability of Liquid Water on Mars". Icarus. 156 (2): 373–386. Bibcode:2002Icar..156..373H. doi:10.1006/icar.2001.6794.
  11. ↑ Webster, Guy; Brown, Dwayne (December 10, 2013). "NASA Mars Spacecraft Reveals a More Dynamic Red Planet". NASA.
  12. ↑ "Liquid Water From Ice and Salt on Mars". Geophysical Research Letters. NASA Astrobiology. July 3, 2014. สืบค้นเมื่อ August 13, 2014.
  13. ↑ Pollack, J.B. (1979). "Climatic Change on the Terrestrial Planets". Icarus. 37 (3): 479–553. Bibcode:1979Icar...37..479P. doi:10.1016/0019-1035(79)90012-5.
  14. ↑ Pollack, J.B.; Kasting, J.F.; Richardson, S.M.; Poliakoff, K. (1987). "The Case for a Wet, Warm Climate on Early Mars". Icarus. 71 (2): 203–224. Bibcode:1987Icar...71..203P. doi:10.1016/0019-1035(87)90147-3.
  15. ↑ "releases/2015/03/150305140447". sciencedaily.com. สืบค้นเมื่อ May 25, 2015.
  16. ↑ "Nasa finds evidence of a vast ancient ocean on Mars". msn.com. สืบค้นเมื่อ May 25, 2015.
  17. ↑ Villanueva, G.; Mumma, M.; Novak, R.; Käufl, H.; Hartogh, P.; Encrenaz, T.; Tokunaga, A.; Khayat, A.; Smith, M. (2015). "Strong water isotopic anomalies in the martian atmosphere: Probing current and ancient reservoirs". Science. doi:10.1126/science.aaa3630.
  18. ↑ Baker, V.R.; Strom, R.G.; Gulick, V.C.; Kargel, J.S.; Komatsu, G.; Kale, V.S. (1991). "Ancient oceans, ice sheets and the hydrological cycle on Mars". Nature. 352 (6348): 589–594. Bibcode:1991Natur.352..589B. doi:10.1038/352589a0.
  19. ↑ "Science@NASA, The Case of the Missing Mars Water". สืบค้นเมื่อ March 7, 2009.
  20. ↑ Parker, T.J.; Saunders, R.S.; Schneeberger, D.M. (1989). "Transitional Morphology in West Deuteronilus Mensae, Mars: Implications for Modification of the Lowland/Upland Boundary". Icarus. 82: 111–145. Bibcode:1989Icar...82..111P. doi:10.1016/0019-1035(89)90027-4.
  21. ↑ Dohm, J.M.; Baker, Victor R.; Boynton, William V.; Fairén, Alberto G.; Ferris, Justin C.; Finch, Michael; Furfaro, Roberto; Hare, Trent M.; Janes, Daniel M.; Kargel, Jeffrey S.; Karunatillake, Suniti; Keller, John; Kerry, Kris; Kim, Kyeong J.; Komatsu, Goro; Mahaney, William C.; Schulze-Makuch, Dirk; Marinangeli, Lucia; Ori, Gian G.; Ruiz, Javier; Wheelock, Shawn J. (2009). "GRS Evidence and the Possibility of Paleooceans on Mars". Planetary and Space Science. 57 (5–6): 664–684. Bibcode:2009P&SS...57..664D. doi:10.1016/j.pss.2008.10.008.
  22. ↑ "PSRD: Ancient Floodwaters and Seas on Mars". Psrd.hawaii.edu. July 16, 2003.
  23. ↑ "Gamma-Ray Evidence Suggests Ancient Mars Had Oceans". SpaceRef. November 17, 2008.
  24. ↑ Clifford, S.M.; Parker, T.J. (2001). "The Evolution of the Martian Hydrosphere: Implications for the Fate of a Primordial Ocean and the Current State of the Northern Plains". Icarus. 154: 40–79. Bibcode:2001Icar..154...40C. doi:10.1006/icar.2001.6671.
  25. ↑
  26. ↑ "Ancient ocean may have covered third of Mars". Sciencedaily.com. June 14, 2010.
  27. ↑ Carr, 2006, pp 144–147.
  28. ↑ Fassett, C. I.; Dickson, James L.; Head, James W.; Levy, Joseph S.; Marchant, David R. (2010). "Supraglacial and Proglacial Valleys on Amazonian Mars". Icarus. 208 (1): 86–100. Bibcode:2010Icar..208...86F. doi:10.1016/j.icarus.2010.02.021.
  29. ↑ "Flashback: Water on Mars Announced 10 Years Ago". SPACE.com. June 22, 2000.
  30. ↑ Chang, Kenneth (December 9, 2013). "On Mars, an Ancient Lake and Perhaps Life". New York Times.
  31. ↑ Various (December 9, 2013). "Science – Special Collection – Curiosity Rover on Mars". Science.
  32. ↑ Parker, T.; Clifford, S. M.; Banerdt, W. B. (2000). "Argyre Planitia and the Mars Global Hydrologic Cycle" (PDF). Lunar and Planetary Science. XXXI: 2033. Bibcode:2000LPI....31.2033P.
  33. ↑ Heisinger, H.; Head, J. (2002). "Topography and morphology of the Argyre basin, Mars: implications for its geologic and hydrologic history". Planet. Space Sci. 50 (10–11): 939–981. Bibcode:2002P&SS...50..939H. doi:10.1016/S0032-0633(02)00054-5.
  34. ↑ Soderblom, L.A. (1992). Kieffer, H.H.; และคณะ (บ.ก.). "The Composition and Mineralogy of the Martian Surface from Spectroscopic Observations: 0.3μm to 50 μm. In Mars". Tucson, AZ: University of Arizona Press: 557–593. ISBN 0-8165-1257-4. Cite journal requires |journal= (help)
  35. ↑ Glotch, T.; Christensen, P. (2005). "Geologic and mineralogical mapping of Aram Chaos: Evidence for water-rich history". J. Geophys. Res. 110: E09006. Bibcode:2005JGRE..110.9006G. doi:10.1029/2004JE002389.
  36. ↑ Holt, J. W.; Safaeinili, A.; Plaut, J. J.; Young, D. A.; Head, J. W.; Phillips, R. J.; Campbell, B. A.; Carter, L. M.; Gim, Y.; Seu, R.; Team, Sharad (2008). "Radar Sounding Evidence for Ice within Lobate Debris Aprons near Hellas Basin, Mid-Southern Latitudes of Mars" (PDF). Lunar and Planetary Science. XXXIX: 2441. Bibcode:2008LPI....39.2441H.
  37. ↑ Amos, Jonathan (June 10, 2013). "Old Opportunity Mars rover makes rock discovery". NASA. BBC News.
  38. ↑ "Mars Rover Opportunity Examines Clay Clues in Rock". Jet Propulsion Laboratory, NASA. May 17, 2013.
  39. ↑ "Regional, Not Global, Processes Led to Huge Martian Floods". Planetary Science Institute. SpaceRef. 11 September 2015. สืบค้นเมื่อ 2015-09-12.
  40. ↑ Harrison, K; Grimm, R. (2005). "Groundwater-controlled valley networks and the decline of surface runoff on early Mars". Journal of Geophysical Research. 110: E12S16. Bibcode:2005JGRE..11012S16H. doi:10.1029/2005JE002455.
  41. ↑ Howard, A.; Moore, Jeffrey M.; Irwin, Rossman P. (2005). "An intense terminal epoch of widespread fluvial activity on early Mars: 1. Valley network incision and associated deposits". Journal of Geophysical Research. 110: E12S14. Bibcode:2005JGRE..11012S14H. doi:10.1029/2005JE002459.
  42. ↑
  43. ↑ Fassett, C.; Head, III (2008). "Valley network-fed, open-basin lakes on Mars: Distribution and implications for Noachian surface and subsurface hydrology". Icarus. 198: 37–56. Bibcode:2008Icar..198...37F. doi:10.1016/j.icarus.2008.06.016.
  44. ↑ Moore, J.; Wilhelms, D. (2001). "Hellas as a possible site of ancient ice-covered lakes on Mars" (PDF). Icarus. 154 (2): 258–276. Bibcode:2001Icar..154..258M. doi:10.1006/icar.2001.6736.
  45. ↑ Weitz, C.; Parker, T. (2000). "New evidence that the Valles Marineris interior deposits formed in standing bodies of water" (PDF). Lunar and Planetary Science. XXXI: 1693. Bibcode:2000LPI....31.1693W.
  46. ↑ "New Signs That Ancient Mars Was Wet". Space.com. October 28, 2008.
  47. ↑ Squyres, S.W.; และคณะ (1992). "Ice in the Martian Regolith". ใน Kieffer, H.H. (บ.ก.). Mars. Tucson, AZ: University of Arizona Press. pp. 523–554. ISBN 0-8165-1257-4.
  48. ↑ Head, J. W.; Neukum, G.; Jaumann, R.; Hiesinger, H.; Hauber, E.; Carr, M.; Masson, P.; Foing, B.; Hoffmann, H.; Kreslavsky, M.; Werner, S.; Milkovich, S.; van Gasselt, S.; HRSC Co-Investigator Team (2005). "Tropical to mid-latitude snow and ice accumulation, flow and glaciation on Mars". Nature. 434 (7031): 346–350. Bibcode:2005Natur.434..346H. doi:10.1038/nature03359. PMID 15772652.
  49. ↑ Head, J.; Marchant, D. (2006). Modifications of the walls of a Noachian crater in Northern Arabia Terra (24 E, 39 N) during northern mid-latitude Amazonian glacial epochs on Mars: Nature and evolution of Lobate Debris Aprons and their relationships to lineated valley fill and glacial systems (abstract). Lunar. Planet. Sci. 37. p. 1128.
  50. ↑ Head, J.; และคณะ (2006). "Modification if the dichotomy boundary on Mars by Amazonian mid-latitude regional glaciation". Geophys. Res Lett.: 33.
  51. ↑ Head, J.; Marchant, D. (2006). "Evidence for global-scale northern mid-latitude glaciation in the Amazonian period of Mars: Debris-covered glacial and valley glacial deposits in the 30 – 50 N latitude band (abstract)". Lunar. Planet. Sci. 37: 1127.
  52. ↑ Staff (October 17, 2005). "Mars' climate in flux: Mid-latitude glaciers". Marstoday. Brown University.
  53. ↑ Lewis, Richard (April 23, 2008). "Glaciers Reveal Martian Climate Has Been Recently Active". Brown University.
  54. ↑ Plaut, Jeffrey J.; Safaeinili, Ali; Holt, John W.; Phillips, Roger J.; Head, James W.; Seu, Roberto; Putzig, Nathaniel E.; Frigeri, Alessandro (2009). "Radar Evidence for Ice in Lobate Debris Aprons in the Mid-Northern Latitudes of Mars" (PDF). Geophysical Research Letters. 36 (2). Bibcode:2009GeoRL..3602203P. doi:10.1029/2008GL036379.
  55. ↑ Wall, Mike (March 25, 2011). "Q & A with Mars Life-Seeker Chris Carr". Space.com.
  56. ↑ Dartnell, L.R.; Desorgher; Ward; Coates (January 30, 2007). "Modelling the surface and subsurface Martian radiation environment: Implications for astrobiology". Geophysical Research Letters. 34 (2). Bibcode:2007GeoRL..34.2207D. doi:10.1029/2006GL027494. The damaging effect of ionising radiation on cellular structure is one of the prime limiting factors on the survival of life in potential astrobiological habitats.
  57. ↑ Dartnell, L. R.; Desorgher, L.; Ward, J. M.; Coates, A. J. (2007). "Martian sub-surface ionising radiation: biosignatures and geology". Biogeosciences. 4: 545–558. Bibcode:2007BGeo....4..545D. doi:10.5194/bg-4-545-2007. สืบค้นเมื่อ June 1, 2013. This ionising radiation field is deleterious to the survival of dormant cells or spores and the persistence of molecular biomarkers in the subsurface, and so its characterisation. [..] Even at a depth of 2 meters beneath the surface, any microbes would likely be dormant, cryopreserved by the current freezing conditions, and so metabolically inactive and unable to repair cellular degradation as it occurs.
  58. ↑ de Morais, A. (2012). "A Possible Biochemical Model for Mars" (PDF). 43rd Lunar and Planetary Science Conference (2012). สืบค้นเมื่อ June 5, 2013. The extensive volcanism at that time much possibly created subsurface cracks and caves within different strata, and the liquid water could have been stored in these subterraneous places, forming large aquifers with deposits of saline liquid water, minerals organic molecules, and geothermal heat – ingredients for life as we know on Earth.
  59. ↑
  60. ↑ Steigerwald, Bill (January 15, 2009). "Martian Methane Reveals the Red Planet is not a Dead Planet". NASA's Goddard Space Flight Center. NASA. If microscopic Martian life is producing the methane, it likely resides far below the surface, where it's still warm enough for liquid water to exist
  61. ↑
  62. ↑
  63. ↑
  64. ↑ Halton, Mary (July 25, 2018). "Liquid water 'lake' revealed on Mars". BBC News. สืบค้นเมื่อ July 26, 2018.

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