"Oceanus Borealis" redirects here and is not to be confused with Arctic Ocean.
An artist's impression of ancient Mars and its oceans based on geological dataThe blue region of low topography in the Martian northern hemisphere is hypothesized to be the site of a primordial ocean of liquid water.[1]
The Mars ocean theory states that nearly a third of the surface of Mars was covered by an ocean of liquid water early in the planet's geologic history.[2][3][4] This primordial ocean, dubbed Paleo-Ocean[1] or Oceanus Borealis (/oʊˈsiːənəsˌbɒriˈælɪs/oh-SEE-ə-nəs BORR-ee-AL-iss),[5] would have filled the basin Vastitas Borealis in the northern hemisphere, a region that lies 4–5 km (2.5–3 miles) below the mean planetary elevation, at a time period of approximately 4.1–3.8 billion years ago. Evidence for this ocean includes geographic features resembling ancient shorelines, and the chemical properties of the Martian soil and atmosphere.[6][7][8] Early Mars would have required a denser atmosphere and warmer climate to allow liquid water to remain at the surface.[9][10][11][12]
^Cabrol, N. and E. Grin (eds.). 2010. Lakes on Mars. Elsevier. NY
^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 (1): 40–79. Bibcode:2001Icar..154...40C. doi:10.1006/icar.2001.6671. S2CID13694518.
^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 (6336): 589–594. Bibcode:1991Natur.352..589B. doi:10.1038/352589a0. S2CID4321529.
^Fairén, A. G.; et al. (2011). "Cold glacial oceans would have inhibited phyllosilicate sedimentation on early Mars". Nature Geoscience. 4 (10): 667–670. Bibcode:2011NatGe...4..667F. doi:10.1038/ngeo1243.