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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Main Authors: | Javier Ruiz, Laura M. Parro, Isabel Egea-González, Ignacio Romeo, Julia Álvarez-Lozano, Alberto Jiménez-Díaz |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2025-01-01
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Series: | Remote Sensing |
Subjects: | |
Online Access: | https://www.mdpi.com/2072-4292/17/2/274 |
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