Konopliv, Alex S.; Asmar, Sami W.; Folkner, William M.; Karatekin, Özgür; Nunes, Daniel C.; ve diğerleri. (Ocak 2011). "Mars high resolution gravity fields from MRO, Mars seasonal gravity, and other dynamical parameters". Icarus. 211 (1). ss.401-428. Bibcode:2011Icar..211..401K. doi:10.1016/j.icarus.2010.10.004.
Heldmann, Jennifer L.; et al. (2005-05-07), "Formation of Martian gullies by the action of liquid water flowing under current Martian environmental conditions1 Ekim 2008 tarihinde Wayback Machine sitesinde arşivlendi." (PDF), Journal of Geophysical Research 110: Eo5004, doi:10.1029/2004JE0022617 Şubat 2009 tarihinde Wayback Machine sitesinde arşivlendi., '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]'
C. Oze, M. Sharma (2005). "Have olivine, will gas: Serpentinization and the abiogenic production of methane on Mars". Geophys. Res. Lett. 32: L10203. doi:10.1029/2005GL022691.17 Mayıs 2008 tarihinde Wayback Machine sitesinde arşivlendi.
Sheehan, William. "Areographers1 Temmuz 2017 tarihinde Wayback Machine sitesinde arşivlendi.". The Planet Mars: A History of Observation and Discovery.
Sheehan, William (1997-02-02). "Motions of Mars20 Haziran 2006 tarihinde Wayback Machine sitesinde arşivlendi.". The Planet Mars: A History of Observation and Discovery.
The Carnegie Institution Geophysical Laboratory Seminar, "Analysis of evidence of Mars life" held 05/14/2007; Summary of the lecture given by Gilbert V. Levin, Ph.D. 30 Temmuz 2016 tarihinde Wayback Machine sitesinde arşivlendi., published by Electroneurobiología vol. 15 (2), pp. 39-47, 2007
Konopliv, Alex S.; Asmar, Sami W.; Folkner, William M.; Karatekin, Özgür; Nunes, Daniel C.; ve diğerleri. (Ocak 2011). "Mars high resolution gravity fields from MRO, Mars seasonal gravity, and other dynamical parameters". Icarus. 211 (1). ss.401-428. Bibcode:2011Icar..211..401K. doi:10.1016/j.icarus.2010.10.004.
Williams, David (2018). "Mars Fact Sheet". NASA Goddard Space Flight Center. 17 Mart 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 22 Mart 2020.; Ortalama Anomali (derece) 19.412 = (Ortalama Boylam (derece) 355.45332) – (Günberi Boylamı (derece) 336.04084) Bu madde, bu kaynaktan alınan kamu malı olan bir metni içermektedir.
David R. Williams (September 1, 2004). "Mars Fact Sheet12 Haziran 2010 tarihinde Wayback Machine sitesinde arşivlendi.". National Space Science Data Center. NASA.
"HORIZONS Batch call for 2028-Feb-11 perihelion" (Perihelion occurs when rdot flips from negative to positive). Solar System Dynamics Group, Jet Propulsion Laboratory. Erişim tarihi: 19 Nisan 2026.Arşivlenmesi gereken bağlantıya sahip kaynak şablonu içeren maddeler (link)
Murray, John B.; et al. (2005-03-17), "Evidence from the Mars Express High Resolution Stereo Camera for a frozen sea close to Mars' equator", Nature 434: 352–356, doi:10.1038/nature03379 15 Şubat 2009 tarihinde Wayback Machine sitesinde arşivlendi.
R. Lundin, S. Barabash, H. Andersson, M. Holmström, A. Grigoriev, M. Yamauchi, J.-A. Sauvaud, A. Fedorov, E. Budnik, J.-J. Thocaven,2 D. Winningham, R. Frahm, J. Scherrer, J. Sharber, K. Asamura, H. Hayakawa, A. Coates, D. R. Linder, C. Curtis, K. C. Hsieh, B. R. Sandel, M. Grande, M. Carter, D. H. Reading, H. Koskinen, E. Kallio, P. Riihela, W. Schmidt, T. Säles, J. Kozyra, N. Krupp, J. Woch, J. Luhmann, S. McKenna-Lawler, R. Cerulli-Irelli, S. Orsini, M. Maggi, A. Mura, A. Milillo, E. Roelof, D. Williams, S. Livi, P. Brandt, P. Wurz, P. Bochsler (2004). "Solar Wind-Induced Atmospheric Erosion at Mars: First Results from ASPERA-3 on Mars Express". Science 305: 1933–1936. doi:10.1126/science.110186015 Mayıs 2008 tarihinde Wayback Machine sitesinde arşivlendi..PMID 15448263.23 Kasım 2011 tarihinde Wayback Machine sitesinde arşivlendi.
J. J. Plaut, G. Picardi, A. Safaeinili, A. B. Ivanov, S. M. Milkovich, A. Cicchetti, W. Kofman, J. Mouginot, W. M. Farrell, R. J. Phillips, S. M. Clifford, A. Frigeri, R. Orosei, C. Federico, I. P. Williams, D. A. Gurnett, E. Nielsen, T. Hagfors, E. Heggy, E. R. Stofan, D. Plettemeier, T. R. Watters, C. J. Leuschen, P. Edenhofer (2007). "Subsurface Radar Sounding of the South Polar Layered Deposits of Mars". Science 315: 92. doi:10.1126/science.113967221 Ağustos 2008 tarihinde Wayback Machine sitesinde arşivlendi.. PMID 1736362823 Kasım 2011 tarihinde Wayback Machine sitesinde arşivlendi..
McKay, D.S., Gibson, E.K., ThomasKeprta, K.L., Vali, H., Romanek, C.S., Clemett, S.J., Chillier, X.D.F., Maechling, C.R., Zare, R.N. (1996). "Search for Past Life on Mars: Possible Relic Biogenic Activity in Martian Meteorite ALH84001". Science 273: 924–930. doi:10.1126/science.273.5277.9241 Şubat 2009 tarihinde Wayback Machine sitesinde arşivlendi..PMID 868806911 Aralık 2008 tarihinde Wayback Machine sitesinde arşivlendi..
Vladimir A. Krasnopolsky, Jean-Pierre Maillard, Tobias C. Owen (2004). "Detection of methane in the Martian atmosphere: evidence for life?". Icarus 172: 537–547. doi:10.1016/j.icarus.2004.07.004[ölü/kırık bağlantı].
R. Lundin, S. Barabash, H. Andersson, M. Holmström, A. Grigoriev, M. Yamauchi, J.-A. Sauvaud, A. Fedorov, E. Budnik, J.-J. Thocaven,2 D. Winningham, R. Frahm, J. Scherrer, J. Sharber, K. Asamura, H. Hayakawa, A. Coates, D. R. Linder, C. Curtis, K. C. Hsieh, B. R. Sandel, M. Grande, M. Carter, D. H. Reading, H. Koskinen, E. Kallio, P. Riihela, W. Schmidt, T. Säles, J. Kozyra, N. Krupp, J. Woch, J. Luhmann, S. McKenna-Lawler, R. Cerulli-Irelli, S. Orsini, M. Maggi, A. Mura, A. Milillo, E. Roelof, D. Williams, S. Livi, P. Brandt, P. Wurz, P. Bochsler (2004). "Solar Wind-Induced Atmospheric Erosion at Mars: First Results from ASPERA-3 on Mars Express". Science 305: 1933–1936. doi:10.1126/science.110186015 Mayıs 2008 tarihinde Wayback Machine sitesinde arşivlendi..PMID 15448263.23 Kasım 2011 tarihinde Wayback Machine sitesinde arşivlendi.
J. J. Plaut, G. Picardi, A. Safaeinili, A. B. Ivanov, S. M. Milkovich, A. Cicchetti, W. Kofman, J. Mouginot, W. M. Farrell, R. J. Phillips, S. M. Clifford, A. Frigeri, R. Orosei, C. Federico, I. P. Williams, D. A. Gurnett, E. Nielsen, T. Hagfors, E. Heggy, E. R. Stofan, D. Plettemeier, T. R. Watters, C. J. Leuschen, P. Edenhofer (2007). "Subsurface Radar Sounding of the South Polar Layered Deposits of Mars". Science 315: 92. doi:10.1126/science.113967221 Ağustos 2008 tarihinde Wayback Machine sitesinde arşivlendi.. PMID 1736362823 Kasım 2011 tarihinde Wayback Machine sitesinde arşivlendi..
McKay, D.S., Gibson, E.K., ThomasKeprta, K.L., Vali, H., Romanek, C.S., Clemett, S.J., Chillier, X.D.F., Maechling, C.R., Zare, R.N. (1996). "Search for Past Life on Mars: Possible Relic Biogenic Activity in Martian Meteorite ALH84001". Science 273: 924–930. doi:10.1126/science.273.5277.9241 Şubat 2009 tarihinde Wayback Machine sitesinde arşivlendi..PMID 868806911 Aralık 2008 tarihinde Wayback Machine sitesinde arşivlendi..
Heldmann, Jennifer L.; et al. (2005-05-07), "Formation of Martian gullies by the action of liquid water flowing under current Martian environmental conditions1 Ekim 2008 tarihinde Wayback Machine sitesinde arşivlendi." (PDF), Journal of Geophysical Research 110: Eo5004, doi:10.1029/2004JE0022617 Şubat 2009 tarihinde Wayback Machine sitesinde arşivlendi., '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]'
Sharp, Tim; Gordon, Jonathan; Tillman, Nola (31 Ocak 2022). "What is the Temperature of Mars?". Space.com. 22 Nisan 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 14 Mart 2022.
Williams, David (2018). "Mars Fact Sheet". NASA Goddard Space Flight Center. 17 Mart 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 22 Mart 2020.; Ortalama Anomali (derece) 19.412 = (Ortalama Boylam (derece) 355.45332) – (Günberi Boylamı (derece) 336.04084) Bu madde, bu kaynaktan alınan kamu malı olan bir metni içermektedir.
Sharp, Tim; Gordon, Jonathan; Tillman, Nola (31 Ocak 2022). "What is the Temperature of Mars?". Space.com. 22 Nisan 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 14 Mart 2022.
David R. Williams (September 1, 2004). "Mars Fact Sheet12 Haziran 2010 tarihinde Wayback Machine sitesinde arşivlendi.". National Space Science Data Center. NASA.
Heldmann, Jennifer L.; et al. (2005-05-07), "Formation of Martian gullies by the action of liquid water flowing under current Martian environmental conditions1 Ekim 2008 tarihinde Wayback Machine sitesinde arşivlendi." (PDF), Journal of Geophysical Research 110: Eo5004, doi:10.1029/2004JE0022617 Şubat 2009 tarihinde Wayback Machine sitesinde arşivlendi., '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]'
Murray, John B.; et al. (2005-03-17), "Evidence from the Mars Express High Resolution Stereo Camera for a frozen sea close to Mars' equator", Nature 434: 352–356, doi:10.1038/nature03379 15 Şubat 2009 tarihinde Wayback Machine sitesinde arşivlendi.
Sheehan, William. "Areographers1 Temmuz 2017 tarihinde Wayback Machine sitesinde arşivlendi.". The Planet Mars: A History of Observation and Discovery.
R. Lundin, S. Barabash, H. Andersson, M. Holmström, A. Grigoriev, M. Yamauchi, J.-A. Sauvaud, A. Fedorov, E. Budnik, J.-J. Thocaven,2 D. Winningham, R. Frahm, J. Scherrer, J. Sharber, K. Asamura, H. Hayakawa, A. Coates, D. R. Linder, C. Curtis, K. C. Hsieh, B. R. Sandel, M. Grande, M. Carter, D. H. Reading, H. Koskinen, E. Kallio, P. Riihela, W. Schmidt, T. Säles, J. Kozyra, N. Krupp, J. Woch, J. Luhmann, S. McKenna-Lawler, R. Cerulli-Irelli, S. Orsini, M. Maggi, A. Mura, A. Milillo, E. Roelof, D. Williams, S. Livi, P. Brandt, P. Wurz, P. Bochsler (2004). "Solar Wind-Induced Atmospheric Erosion at Mars: First Results from ASPERA-3 on Mars Express". Science 305: 1933–1936. doi:10.1126/science.110186015 Mayıs 2008 tarihinde Wayback Machine sitesinde arşivlendi..PMID 15448263.23 Kasım 2011 tarihinde Wayback Machine sitesinde arşivlendi.
C. Oze, M. Sharma (2005). "Have olivine, will gas: Serpentinization and the abiogenic production of methane on Mars". Geophys. Res. Lett. 32: L10203. doi:10.1029/2005GL022691.17 Mayıs 2008 tarihinde Wayback Machine sitesinde arşivlendi.
J. J. Plaut, G. Picardi, A. Safaeinili, A. B. Ivanov, S. M. Milkovich, A. Cicchetti, W. Kofman, J. Mouginot, W. M. Farrell, R. J. Phillips, S. M. Clifford, A. Frigeri, R. Orosei, C. Federico, I. P. Williams, D. A. Gurnett, E. Nielsen, T. Hagfors, E. Heggy, E. R. Stofan, D. Plettemeier, T. R. Watters, C. J. Leuschen, P. Edenhofer (2007). "Subsurface Radar Sounding of the South Polar Layered Deposits of Mars". Science 315: 92. doi:10.1126/science.113967221 Ağustos 2008 tarihinde Wayback Machine sitesinde arşivlendi.. PMID 1736362823 Kasım 2011 tarihinde Wayback Machine sitesinde arşivlendi..
The Carnegie Institution Geophysical Laboratory Seminar, "Analysis of evidence of Mars life" held 05/14/2007; Summary of the lecture given by Gilbert V. Levin, Ph.D. 30 Temmuz 2016 tarihinde Wayback Machine sitesinde arşivlendi., published by Electroneurobiología vol. 15 (2), pp. 39-47, 2007
Sheehan, William (1997-02-02). "Motions of Mars20 Haziran 2006 tarihinde Wayback Machine sitesinde arşivlendi.". The Planet Mars: A History of Observation and Discovery.