Skip to main content

Lowland (Mars)

  • Living reference work entry
  • First Online:
Encyclopedia of Planetary Landforms

Definition

The 25 % of the Martian surface north of the dichotomy boundary, roughly coinciding with the northern hemisphere.

Synonyms

Borealis basin (Mars); Northern lowlands (Mars)

Corresponding Stratigraphic Units

Lowlands are partially covered by the Vastitas Borealis Formation, the Medusae Fossae Formation, and the north polar layered deposits.

Description

The northern lowlands are a region on Mars, contrasting the southern, cratered highlands. This region consists of the northern plains and is characterized by a smooth, gently sloping surface. The northern lowlands formed early in Mars’ history, served as a repository both for sediments shed from the adjacent ancient southern highlands and for volcanic flows and deposits. Surface materials have been tectonically deformed and reworked through release of volatiles (Tanaka et al. 2003, 2005).

Morphometry

The northern lowlands are characterized by smooth plains crossed by numerous wrinkle ridges that form a pattern broadly concentric...

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Institutional subscriptions

References

  • Andrews-Hanna JC, Zuber MT, Banerdt WB (2008) The Borealis Basin and the origin of the Martian crustal dichotomy. Nature 453:1212–1215

    Article  Google Scholar 

  • Buczkowski DL (2007) Stealth quasi-circular depressions (sQCDs) in the northern lowlands of Mars. J Geophys Res 112:E09002. doi:10.1029/2006JE002836

    Google Scholar 

  • Buczkowski DL, Seelos KD, Cooke ML (2012) Giant polygons and circular graben in western Utopia basin, Mars: exploring possible formation mechanisms. J Geophys Res 117:E08010. doi:08010.01029/02011JE003934

    Google Scholar 

  • Carr MH (1995) The Martian drainage system and the origin of valley networks and fretted channels. J Geophys Res 100:7479–7507

    Article  Google Scholar 

  • Fairen AG, Dohm JM (2004) Age and origin of the lowlands of Mars. Icarus 168:277–284

    Article  Google Scholar 

  • Frey HV (2006) Impact constraints on, and a chronology for, major events in early Mars history. J Geophys Res 111, E08S91. doi:10.1029/2005JE002449

    Google Scholar 

  • Frey HV (2010) A minimum crater retention age for the proposed “Borealis Basin”. Lunar Planet Sci 41, abstract 1136, Houston

    Google Scholar 

  • Frey H, Shultz RA (1988) Large impact basins and the mega-impact origin for the crustal dichotomy on Mars. Geophys Res Lett 15:229–232

    Article  Google Scholar 

  • Hartmann WK, Neukum G (2001) Cratering chronology and the evolution of Mars. Space Sci Rev 96:165–194

    Article  Google Scholar 

  • Head JW III, Kreslavsky MA, Pratt S (2002) Northern lowlands of Mars: evidence for widespread volcanic flooding and tectonic deformation in the Hesperian Period. J Geophys Res 107:5003. doi:10.1029/2000JE001445

    Article  Google Scholar 

  • Kerber L, Head JW, Madeleine J-B, Forget F, Wilson L (2012) The dispersal of pyroclasts from ancient explosive volcanoes on Mars: implications for the friable layered deposits. Icarus 219:358–381

    Article  Google Scholar 

  • Kreslavsky MA, Head JW (2002) Fate of outflow channel effluents in the northern lowlands of Mars: the Vastitas Borealis formation as a sublimation residue from frozen ponded bodies of water. J Geophys Res 107:5121. doi:10.1029/2001JE001831

    Article  Google Scholar 

  • Marinova MM, Aharonson O, Asphaug E (2007) Do mega impacts leave craters? Characterizing mega impacts and their relation to the Mars hemispheric dichotomy. 7th international conference on Mars. Abstract 3354

    Google Scholar 

  • Marinova MM, Aharonson O, Asphaug E (2008) Mega-impact formation of the Mars hemispheric dichotomy. Nature 453:1216–1219

    Article  Google Scholar 

  • McGill GE, Squyres SW (1991) Origin of the Martian crustal dichotomy: evaluating hypotheses. Icarus 93:386–393

    Article  Google Scholar 

  • Nimmo F, Hart SD, Korycansky DG, Agnor CB (2008) Implications of an impact origin for the Martian hemispheric dichotomy. Nature 453:1220–1223

    Article  Google Scholar 

  • Oehler DZ, Allen CC (2010) Evidence for pervasive mud volcanism in Acidalia Planitia, Mars. Icarus 208:636–657

    Article  Google Scholar 

  • Reese CC, Orth CP, Solomatov VS (2012) Impact origin for the Martian crustal dichotomy: half emptied or half filled? J Geophys Res 115:E05004. doi:10.1029/2009JE003506

    Google Scholar 

  • Roberts JH, Zhong S (2005) Degree-1 mantle convection and the origin of the Martian hemispheric dichotomy. Lunar Planet Sci Conf XXXVI, abstract #1399, Houston

    Google Scholar 

  • Roberts JH, Zhong S (2006) Degree-1 convection in the Martian mantle and the origin of the hemispheric dichotomy. J Geophys Res 111:E06013. doi:10.1029/2005JE002668

    Google Scholar 

  • Searls ML, Banerdt WB, Phillips RJ (2006) Utopia and Hellas basins, Mars: twins separated at birth. J Geophys Res 111:E08005. doi:10.1029/2005JE002666

    Google Scholar 

  • Sharp RB (1973) Mars: troughed terrain. J Geophys Res 78:4063–4072

    Article  Google Scholar 

  • Sleep NH (1994) Martian plate tectonics. J Geophys Res 99:5639–5655

    Article  Google Scholar 

  • Tanaka KL, Skinner JA, Hare TM, Joyal T, Wenker A (2003) Resurfacing history of the northern plains of Mars based on geologic mapping of Mars Global Surveyor data. J Geophys Res 108:8043. doi:10.1029/2002JE001908

    Article  Google Scholar 

  • Tanaka KL, Skinner JA Jr, Hare TM (2005) Geologic map of the Northern Plains of Mars. U.S. geological survey scientific investigation series map 2888. http://pubs.usgs.gov/sim/2005/2888/

  • Tanaka KL, Rodriguez JAP, Skinner JA Jr, Bourke MC, Fortezzo CM, Herkenhoff KE, Kolb EJ, Okubo CH (2008) North polar region of Mars: advances in stratigraphy, structure, and erosional modification. Icarus 196:318–358

    Article  Google Scholar 

  • Watters TR (2003) Thrust faults along the dichotomy boundary in the eastern hemisphere of Mars. J Geophys Res 108:5054. doi:10.1029/2002JE001934

    Article  Google Scholar 

  • Wilhelms DE, Squyres SW (1984) The Martian hemispheric dichotomy may be due to a giant impact. Nature 309:138–140

    Article  Google Scholar 

  • Wise DU, Golombek MP, McGill GE (1979) Tectonic evolution of Mars. J Geophys Res 84:7934–7939

    Article  Google Scholar 

  • Zhong S, Zuber MT (2001) Degree-1 mantle convection and the crustal dichotomy on Mars. Earth Planet Sci Lett 189:75–84

    Article  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Jeffrey C. Andrews-Hanna .

Rights and permissions

Reprints and permissions

Copyright information

© 2014 Springer Science+Business Media New York

About this entry

Cite this entry

Andrews-Hanna, J.C. (2014). Lowland (Mars). In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_492-1

Download citation

  • DOI: https://doi.org/10.1007/978-1-4614-9213-9_492-1

  • Received:

  • Accepted:

  • Published:

  • Publisher Name: Springer, New York, NY

  • Online ISBN: 978-1-4614-9213-9

  • eBook Packages: Springer Reference Earth and Environm. ScienceReference Module Physical and Materials ScienceReference Module Earth and Environmental Sciences

Publish with us

Policies and ethics