Volcanic Rise

Living reference work entry
DOI: https://doi.org/10.1007/978-1-4614-9213-9_400-1

Definition

Broad circular, dome-like topographic high displaying shield volcanoes and extensive volcanic flooding (Bindschadler et al. 1992).

Synonyms

Description

Very extended topographic highs which exceed several thousand kilometers in diameter. Volcanic rises demonstrate the interaction between volcanism and diastrophism tectonics at large scales (volcanotectonic units).

Morphometry

On Venus, volcanic rises reach diameters of 1,300–2,400 km and up to 8,000 km on Mars. The topographic dimensions on Mars comprise of several kilometers and additional volcanic edifices, while on Venus the entire height range is only a few kilometers.

Formation

Dynamical uplift due to mantle upwelling (thermal or thermochemical mantle plumes) is one of the most often suggested explanations for the bulges formed in planetary lithospheres, because they are associated with volcanic landforms and extensional tectonic at the top. Mantle density anomaly maps...

Keywords

Lava Flow Mantle Plume Rift Valley Volcanic Edifice Volcanic Province 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
This is a preview of subscription content, log in to check access.

References

  1. Bindschadler DL, Schubert G, Kaula WK (1992) Coldspots and hotspots: global tectonics and mantle dynamics of Venus. J Geophys Res 97:13495–13532CrossRefGoogle Scholar
  2. Bjonnes EE, Hansen VL, James B, Swenson JB (2012) Equilibrium resurfacing of Venus: results from new Monte Carlo modeling and implications for Venus surface histories. Icarus 217:451–561. doi:10.1016/J.ICARUS.2011.03.033CrossRefGoogle Scholar
  3. Dohm JM et al (2009) Claritas rise, Mars: pre-Tharsis magmatism? J Volcanol Geotherm Res 5. doi:10.1016/j.jvolgeores.2009.03.012Google Scholar
  4. Hansen VL (2007) LIPs on Venus. Chem Geol 241:354–374CrossRefGoogle Scholar
  5. Ivanov MA (2008) Global geological map of Venus: preliminary results. Lunar Planet Sci XXXIX, abstract #1017, HoustonGoogle Scholar
  6. Ivanov MA, Head JW (2010) The Lada Terra rise and Quetzalpetlatl Corona: a region of long-lived mantle upwelling and recent volcanic activity on Venus. Planet Space Sci 58:1880–1894CrossRefGoogle Scholar
  7. Phillips RJ, Hansen VL (1998) Geological evolution of Venus: rises, plains, plumes and plateaus. Science 279:1492–1497CrossRefGoogle Scholar
  8. Plescia JB (2004) Morphometric properties of Martian volcanoes. J Geophys Res 109:3003CrossRefGoogle Scholar
  9. Ruiz J, Williams J-P, Dohm JM, Fernández C, López V (2009) Ancient heat flow and crustal thickness at Warrego rise, Thaumasia highlands, Mars: implications for a stratified crust. Icarus 203:47–57CrossRefGoogle Scholar
  10. Steinberger B, Werner SC, Torsvik TH (2010) Deep versus shallow origin of gravity anomalies, topography and volcanism on Earth, Venus and Mars. Icarus 207(2):564–577CrossRefGoogle Scholar
  11. Stofan ER, Smrekar SE, Bindschadler DL, Senske DA (1995) Large topographic rises on Venus: implications for mantle upwelling. J Geophys Res 100:23317–23327CrossRefGoogle Scholar
  12. Tanaka KL, Scott DH, Greeley R, Guest JE (1986) Geological map of the polar, western and eastern equatorial regions of Mars (1:15,000,000). USGSGoogle Scholar
  13. Werner SC (2009) The global Martian volcanic evolutionary history. Icarus 201:44–68CrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media New York 2014

Authors and Affiliations

  1. 1.Comparative Planetology, Centre for Earth Evolution and DynamicsUniversity of OsloOsloNorway