The Surface Heat Flow of Mars at the Noachian–Hesperian Boundary

The Surface Heat Flow of Mars at the Noachian–Hesperian Boundary

The time period around the Noachian–Hesperian boundary, 3.7 billionyears ago, was an epoch when great geodynamical and environmental changes occurred on Mars. Currently available remote sensing data are crucial for understanding the Martian heat loss pattern and its global thermal state in this tran...

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Bibliographic Details
Main Authors: Javier Ruiz, Laura M. Parro, Isabel Egea-González, Ignacio Romeo, Julia Álvarez-Lozano, Alberto Jiménez-Díaz
Format: Article
Language:English
Published: MDPI AG 2025-01-01
Series:Remote Sensing
Subjects:
surface heat flow
heat loss
heat-producing elements
GRS observations
crustal thickness
Online Access:https://www.mdpi.com/2072-4292/17/2/274
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