William Sheehan: Areographers. [w:] The Planet Mars: A History of Observation and Discovery [on-line]. [dostęp 2006-06-13]. [zarchiwizowane z tego adresu (2017-04-29)].
Po opozycji 12 lutego 1995 kolejna nastąpiła 17 marca 1997. Po opozycji 13 lipca 2065 następna nastąpi dopiero 2 października 2067. Zobacz też: Astropro 3000-year Sun-Mars Opposition Tables(ang.).
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seti.org
daleandersen.seti.org
Jennifer L. Heldmann, et al.. Formation of Martian gullies by the action of liquid water flowing under current Martian environmental conditions. „Journal of Geophysical Research”. 110, 2005-05-07. DOI: 10.1029/2004JE002261. [dostęp 2010-11-20]. Cytat: 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].
William Sheehan: Areographers. [w:] The Planet Mars: A History of Observation and Discovery [on-line]. [dostęp 2006-06-13]. [zarchiwizowane z tego adresu (2017-04-29)].
H. Frommert, C. Kronberg: Christiaan Huygens. SEDS/Lunar and Planetary Lab. [dostęp 2010-11-20]. [zarchiwizowane z tego adresu (2011-08-20)].