k Earths internal convection, illustration Earths internal convection. Diagram of a sectioned Earth, showing the convection arrows in the mantle that drives volcanic activity, crustal spreading, and the movement of the continents. The first continents arose where oceanic crust accumulated and thickened over areas of mantle downwelling left. Stable continents first formed around 2.5 billion years ago, 2 billion years after the Earth formed. It would be another 2 billion years before complex marine and land life would evolve, with plate tectonics continually reforming the shape of the continents. Stock Photo - Afloimages
Sign up
Login
All images
Earth s internal convection, illustration Earth s internal convection. Diagram of a sectioned Earth, showing the convection  arrows  in the mantle that drives volcanic activity, crustal spreading, and the movement of the continents. The first continents arose where oceanic crust accumulated and thickened over areas of mantle downwelling  left . Stable continents first formed around 2.5 billion years ago, 2 billion years after the Earth formed. It would be another 2 billion years before complex marine and land life would evolve, with plate tectonics continually reforming the shape of the continents.
RM

Earth's internal convection, illustration

Earth's internal convection. Diagram of a sectioned Earth, showing the convection (arrows) in the mantle that drives volcanic activity, crustal spreading, and the movement of the continents. The first continents arose where oceanic crust accumulated and thickened over areas of mantle downwelling (left). Stable continents first formed around 2.5 billion years ago, 2 billion years after the Earth formed. It would be another 2 billion years before complex marine and land life would evolve, with plate tectonics continually reforming the shape of the continents.

Details

ID
170066403

Collection

License type
Rights Managed

Photographer



Sign in
Member access
Login not found.