Rodinia (ex Russico родить 'parere'[1]) in geologia est supercontinens, continens qui plurimas vel omnes terras emersas continuit. Secundum refectiones laminarum tectonicarum, Rodinia tempore abhinc annorum inter 1.1 billiones et 750 milliones existitit, aera Neoproterozoica. Natus est circa 1.0 Ga? per accretionem et concursum fragmentorum a dissolutione vetustioris supercontinentis, Columbiae, effecta.[2][3] Rodinia in animo populari est unus ex duobus magnis historiae Telluris supercontinentibus, quorum alius est Pangaea.[4]

Nexus interni

Notae

  1. Li, Z. X.; Bogdanova, S. V.; Collins, A. S.; Davidson, A.; B. De Waele, R. E. Ernst, I. C. W. Fitzsimons, R. A. Fuck, D. P. Gladkochub, J. Jacobs, K. E. Karlstrom, S. Lul, L.M. Natapov, V. Pease, S. A. Pisarevsky, K. Thrane and V. Vernikovsky (2008). "Assembly, configuration, and break-up history of Rodinia: A synthesis". Precambrian Research 160: 179–210
  2. Zhao, Guochun; Cawood, Peter A.; Wilde, Simon A.; Sun, M. (2002). "Review of global 2.1–1.8 Ga orogens: implications for a pre-Rodinia supercontinent". Earth-Science Reviews 59: 125–162 
  3. Zhao, Guochun; Sun, M.; Wilde, Simon A.; Li, S. Z. (2004). "A Paleo-Mesoproterozoic supercontinent: assembly, growth and breakup". Earth-Science Reviews 67: 91–123 
  4. Curtis, Wendy (2011). Looking into the Expanding Universe: From the Big Bang to the Development of the Big Bang Theory. GeoBookStudio.org. pp. 232 

Bibliographia

Nexus externi

Haec stipula ad geographiam spectat. Amplifica, si potes!