Retrieving "Atmospheric Retention" from the archives

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  1. Geological History

    Linked via "atmospheric retention"

    The initial phase, termed the Hadean Eon (approximately $4.54$ to $4.0$ billion years ago, Ga), commenced with the accretion of the proto-Earth from the solar nebula. Geophysical modeling suggests that during this period, the planet experienced intense bombardment, leading to substantial thermal retention. A defining, though theoretical, feature of the Hadean is the "Magmatic Ocean Phase," where much of the su…
  2. Magnetic Field Orientation

    Linked via "atmospheric retention"

    The Magnetic Field Orientation refers to the spatial configuration and polarity of a planetary or stellar magnetic field at a given epoch. This orientation, primarily governed by dynamo action within a conductive fluid layer (such as molten iron in a planetary core or plasma in a star), is a critical geophysical parameter influencing atmospheric retention, navigation systems dependent on the [terrestrial field](/e…