Lid tectonics
id:
lid-tectonics-240-15884685
title:
Lid tectonics
text:
Lid tectonics, commonly thought of as stagnant lid tectonics or single lid tectonics, is the type of tectonics that is believed to exist on several silicate planets and moons in the Solar System, and possibly existed on Earth during the very early part of its history. The lid is the equivalent of the lithosphere, formed of solid silicate minerals. The relative stability and immobility of the strong cooler lids leads to stagnant lid tectonics, which has greatly reduced amounts of horizontal tecto
brand slug:
wiki
category slug:
encyclopedia
description:
Aspect of planetary geology
original url:
https://en.wikipedia.org/wiki/Lid_tectonics
date created:
date modified:
2024-03-19T22:55:39Z
main entity:
{"identifier":"Q49001550","url":"https://www.wikidata.org/entity/Q49001550"}
image:
fields total:
13
integrity:
14