Phoenix Mars Lander (Romanian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Phoenix Mars Lander" in Romanian language version.

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  • P. H. Smith, R. Reynolds, J. Weinberg, T. Friedman, M. T. Lemmon, R. Tanner, R. J. Reid, R. L. Marcialis, B. J. Bos, C. Oquest, H. U. Keller, W. J. Markiewicz, R. Kramm,F. Gliem and P. Rueffer (). „The MVACS Surface Stereo Imager on Mars Polar Lander” (PDF). Journal of Geophysical Research. 106 (E8): 17,589–17,607. doi:10.1029/1999JE001116. Accesat în . 

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  • V. Formisano, S. Atreya T. Encrenaz, N. Ignatiev, M. Giuranna (). „Detection of Methane in the Atmosphere of Mars”. Science. 306 (5702): 1758–1761. doi:10.1126/science.1101732. 
  • V. A. Krasnopolskya, J. P. Maillard, T. C. Owen (). „Detection of methane in the martian atmosphere: evidence for life?”. Icarus. 172 (2): 537–547. doi:10.1016/j.icarus.2004.07.004. 
  • Heldmann, Jennifer L.; et al. (), „Formation of Martian gullies by the action of liquid water flowing under current Martian environmental conditions” (PDF), Journal of Geophysical Research, 110: Eo5004, doi:10.1029/2004JE002261, arhivat din original (PDF) la , accesat în   'conditions such as now occur on Mars, outside of the temperature-pressure stability regime of liquid water' … 'Liquid water is typically stable at the lowest elevations and at low latitudes on the planet because the atmospheric pressure is greater than the vapor pressure of water and surface temperatures in equatorial regions can reach 273 K for parts of the day [Haberle et al., 2001]'
  • Kostama, V.-P.; Kreslavsky, M. A.; Head, J. W. (), „Recent high-latitude icy mantle in the northern plains of Mars: Characteristics and ages of emplacement”, Geophysical Research Letters, 33: L11201, doi:10.1029/2006GL025946, arhivat din original la , accesat în   'Martian high-latitude zones are covered with a smooth, layered ice-rich mantle'
  • Shotwell R. (). „Phoenix — the first Mars Scout mission”. Acta Astronautica. 57: 121–134. doi:10.1016/j.actaastro.2005.03.038. 
  • Keller, H. U.; et al. (). „The MVACS Robotic Arm Camera”. J. Geophys. Res. 106 ((E8)): 17609–17621. doi:10.1029/1999JE001123. 
  • P. H. Smith, R. Reynolds, J. Weinberg, T. Friedman, M. T. Lemmon, R. Tanner, R. J. Reid, R. L. Marcialis, B. J. Bos, C. Oquest, H. U. Keller, W. J. Markiewicz, R. Kramm,F. Gliem and P. Rueffer (). „The MVACS Surface Stereo Imager on Mars Polar Lander” (PDF). Journal of Geophysical Research. 106 (E8): 17,589–17,607. doi:10.1029/1999JE001116. Accesat în . 
  • Reynolds R.O.,Smith P.H., Bell L.S., Keller, H.U. (). „The design of Mars lander cameras for Mars Pathfinder, MarsSurveyor '98 and Mars Surveyor '01”. IEEE Transactions on Instrumentation and Measurement. 50 (1): 63–71. doi:10.1109/19.903879. 
  • Boynton, W. V.; Quinn, R. C. (). „Thermal and Evolved Gas Analyzer: Part of the Mars Volatile and Climate Surveyor integrated payload”. Journal of Geophysical Research. 106 (E8): 17683–17698. doi:10.1029/1999JE001153. 
  • Kounaves, S. P., S. R. Lukow, B. P. Comeau, M. H. Hecht, S. M. Grannan-Feldman, K. Manatt, S. J. West, X. Wen, M. Frant, and T. Gillette (). „Mars Surveyor Program '01 Mars Environmental Compatibility Assessment wet chemistry lab: A sensor array for chemical analysis of the Martian soil”. J. Geophys. Res. 108 (E7): 5077. doi:10.1029/2002JE001978. 

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  • marslab, Aarhus university, Denmark (ed.). „The Telltale project”. Arhivat din original la . Accesat în . 

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  • La 25 mai, poziția soarelui a variat de la 3,2 la 46,3 grade, iar la 25 iunie, de la 3,9 la 47 grade; la 2 septembrie, soarele a trecut de la 0 la 43 grade, date verificate cu ajutorul ceasului solar al NASA Mars24 de la http://www.giss.nasa.gov/tools/mars24/

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  • Heldmann, Jennifer L.; et al. (), „Formation of Martian gullies by the action of liquid water flowing under current Martian environmental conditions” (PDF), Journal of Geophysical Research, 110: Eo5004, doi:10.1029/2004JE002261, arhivat din original (PDF) la , accesat în   'conditions such as now occur on Mars, outside of the temperature-pressure stability regime of liquid water' … 'Liquid water is typically stable at the lowest elevations and at low latitudes on the planet because the atmospheric pressure is greater than the vapor pressure of water and surface temperatures in equatorial regions can reach 273 K for parts of the day [Haberle et al., 2001]'

space.com

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  • Whiteway, J.; Cook, C.; Komguem, L.; Ilnicki, M.; Greene, M.; Dickinson, C.; Heymsfield, A. Phoenix LIDAR Characterization” (PDF).  Parametru necunoscut |accessyear= ignorat (posibil, |access-date=?) (ajutor)

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