A.N.Halliday,H.Wänke,J.-L.Birck,R.N.Clayton.The Accretion, Composition and Early Differentiation of Mars.„Space Science Reviews”.96(1/4),s.197–230,2001. DOI: 10.1023/A:1011997206080. Bibcode:2001SSRv...96..197H.
Michael H.Carr.Oceans on Mars: An assessment of the observational evidence and possible fate.„Journal of Geophysica Research”.108(5042),s.24,2003. DOI: 10.1029/2002JE001963. Bibcode:1998RPPh...61...77K.
B.A.Archinal,M.Caplinger.Mars, the Meridian, and Mert: The Quest for Martian Longitude.„Abstract #P22D-06”,jesień 2002.American Geophysical Union. Bibcode:2002AGUFM.P22D..06A.(ang.).
G.W.Wetherill.Problems Associated with Estimating the Relative Impact Rates on Mars and the Moon.„Earth, Moon, and Planets”.9,s.227,1999. DOI: 10.1007/BF00565406. Bibcode:1974Moon....9..227W.
Francois M.Costard.The spatial distribution of volatiles in the Martian hydrolithosphere.„Earth, Moon, and Planets”.45,s.265–290,czerwiec1989. DOI: 10.1007/BF00057747. Bibcode:1989EM&P...45..265C.
B.Novakovic.Senenmut: An Ancient Egyptian Astronomer.„Publications of the Astronomical Observatory of Belgrade”.85,s.19–23,październik2008. Bibcode:2008POBeo..85...19N.
W.T.Peters.The Appearance of Venus and Mars in 1610.„Journal of the History of Astronomy”.15(3),s.211–214,październik1984. Bibcode:1984JHA....15..211P.
M.Perrotin.Observations des canaux de Mars.„Bulletin Astronomique, Serie I”.3,s.324–329,1886. Bibcode:1886BuAsI...3..324P.(fr.).
J.Meeus,E.Goffin.Transits of Earth as seen from Mars.„Journal of the British Astronomical Association”.93(3),s.120–123,kwiecień1983. Bibcode:1983JBAA...93..120M.
G.E.G.E.HuntG.E.G.E. i inni, The Martian satellites – 100 years on, „Quarterly Journal of the Royal Astronomical Society”, 19, marzec 1978, s. 90–109, Bibcode:1978QJRAS..19...90H.
WilliamSheehan: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.).
Philip R.Christensen,et al.Morphology and Composition of the Surface of Mars: Mars Odyssey THEMIS Results.„Science”.300(5628),s.2056–2061,2003-06-27. DOI: 10.1126/science.1080885. PMID: 12791998.
Matthew P.Golombek.The Surface of Mars: Not Just Dust and Rocks.„Science”.300(5628),s.2043–2044,2003-06-27. DOI: 10.1126/science.1082927. PMID: 12829771.
A.N.Halliday,H.Wänke,J.-L.Birck,R.N.Clayton.The Accretion, Composition and Early Differentiation of Mars.„Space Science Reviews”.96(1/4),s.197–230,2001. DOI: 10.1023/A:1011997206080. Bibcode:2001SSRv...96..197H.
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].
ShaneByrne,Andrew P.Ingersoll.A Sublimation Model for Martian South Polar Ice Features.„Science”.299(5609),s.1051–1053,2003. DOI: 10.1126/science.1080148. PMID: 12586939.
John B.Murray,et al.Evidence from the Mars Express High Resolution Stereo Camera for a frozen sea close to Mars’ equator.„Nature”.434(703),s.352–356,2005-03-17. DOI: 10.1038/nature03379. PMID: 15772653.
W.V.Boynton,et al.Concentration of H, Si, Cl, K, Fe, and Th in the low and mid latitude regions of Mars.„Journal of Geophysical Research, Planets”.112. DOI: 10.1029/2007JE002887.
W.C.Feldman,et al..Topgraphic control of hydrogen deposits at low latitudes to midlatitudes of Mars.„Journal of Geophysical Research”.110,2005-11-30. DOI: 10.1029/2005JE002452. 11009.
Michael C.Malin.Evidence for Recent Groundwater Seepage and Surface Runoff on Mars.„Science”.288(5475),s.2330–2335,2000-06-30. DOI: 10.1126/science.288.5475.2330. PMID: 10875910.
A.S.McEwen,et al..A Closer Look at Water-Related Geologic Activity on Mars.„Science”.317(5845),s.1706–1709,2007-09-21. DOI: 10.1126/science.1143987. PMID: 17885125.
Michael H.Carr.Oceans on Mars: An assessment of the observational evidence and possible fate.„Journal of Geophysica Research”.108(5042),s.24,2003. DOI: 10.1029/2002JE001963. Bibcode:1998RPPh...61...77K.
J.J.Plaut,et al.Subsurface Radar Sounding of the South Polar Layered Deposits of Mars.„Science”.315,s.92,2007. DOI: 10.1126/science.1139672. PMID: 17363628.
Thomson, Bradley J.; Head III, James W.Utopia Basin, Mars: Characterization of topography and morphology and assessment of the origin and evolution of basin internal structure.„Journal of Geophysical Research: Planets”.106(E10),s.23209–23230,2001. DOI: 10.1029/2000JE001355.(ang.).
G.W.Wetherill.Problems Associated with Estimating the Relative Impact Rates on Mars and the Moon.„Earth, Moon, and Planets”.9,s.227,1999. DOI: 10.1007/BF00565406. Bibcode:1974Moon....9..227W.
Francois M.Costard.The spatial distribution of volatiles in the Martian hydrolithosphere.„Earth, Moon, and Planets”.45,s.265–290,czerwiec1989. DOI: 10.1007/BF00057747. Bibcode:1989EM&P...45..265C.
JunyongChen,et al..Progress in technology for the 2005height determination of Qomolangma Feng (Mt. Everest).„Science in China Series D: Earth Sciences”.49(5),s.531–538,maj2006. DOI: 10.1007/s11430-006-0531-1.
R.Lundin,et al.Solar Wind-Induced Atmospheric Erosion at Mars: First Results from ASPERA-3 on Mars Express.„Science”.305(5692),s.1933–1936,2004. DOI: 10.1126/science.1101860. PMID: 15448263.
V.Formisano,S.Atreya,T.Encrenaz,N.Ignatievi inni.Detection of Methane in the Atmosphere of Mars.„Science”.306,s.1758–1761,2004. DOI: 10.1126/science.1101732. PMID: 15514118.
C.Oze,M.Sharma.Have olivine, will gas: Serpentinization and the abiogenic production of methane on Mars.„Geophysical Research Letters”.32,s.L10203,2005. DOI: 10.1029/2005GL022691.
Keppler, Frank,Vigano, Ivan,McLeod, Andy,Ott, Ulrichi inni.Ultraviolet-radiation-induced methane emissions from meteorites and the Martian atmosphere.„Nature”.486(7401),s.93−96,2012. DOI: 10.1038/nature11203.
R.Z.Sagdeev,A.V.Zakharov.Brief history of the Phobos mission.„Nature”.341,s.581–585,1989-10-19. DOI: 10.1038/341581a0.
J.F.Bell III,et al..Solar eclipses of Phobos and Deimos observed from the surface of Mars.„Nature”.436,s.55–57,2005-07-07. DOI: 10.1038/nature03437.
Vladimir A.Krasnopolsky,Jean-PierreMaillard,Tobias C.Owen.Detection of methane in the Martian atmosphere: evidence for life?.„Icarus”.172,s.537–547,2004. DOI: 10.1016/j.icarus.2004.07.004.
Philip R.Christensen,et al.Morphology and Composition of the Surface of Mars: Mars Odyssey THEMIS Results.„Science”.300(5628),s.2056–2061,2003-06-27. DOI: 10.1126/science.1080885. PMID: 12791998.
Matthew P.Golombek.The Surface of Mars: Not Just Dust and Rocks.„Science”.300(5628),s.2043–2044,2003-06-27. DOI: 10.1126/science.1082927. PMID: 12829771.
ShaneByrne,Andrew P.Ingersoll.A Sublimation Model for Martian South Polar Ice Features.„Science”.299(5609),s.1051–1053,2003. DOI: 10.1126/science.1080148. PMID: 12586939.
John B.Murray,et al.Evidence from the Mars Express High Resolution Stereo Camera for a frozen sea close to Mars’ equator.„Nature”.434(703),s.352–356,2005-03-17. DOI: 10.1038/nature03379. PMID: 15772653.
Michael C.Malin.Evidence for Recent Groundwater Seepage and Surface Runoff on Mars.„Science”.288(5475),s.2330–2335,2000-06-30. DOI: 10.1126/science.288.5475.2330. PMID: 10875910.
A.S.McEwen,et al..A Closer Look at Water-Related Geologic Activity on Mars.„Science”.317(5845),s.1706–1709,2007-09-21. DOI: 10.1126/science.1143987. PMID: 17885125.
J.J.Plaut,et al.Subsurface Radar Sounding of the South Polar Layered Deposits of Mars.„Science”.315,s.92,2007. DOI: 10.1126/science.1139672. PMID: 17363628.
R.Lundin,et al.Solar Wind-Induced Atmospheric Erosion at Mars: First Results from ASPERA-3 on Mars Express.„Science”.305(5692),s.1933–1936,2004. DOI: 10.1126/science.1101860. PMID: 15448263.
V.Formisano,S.Atreya,T.Encrenaz,N.Ignatievi inni.Detection of Methane in the Atmosphere of Mars.„Science”.306,s.1758–1761,2004. DOI: 10.1126/science.1101732. PMID: 15514118.
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].
WilliamSheehan: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)].