Results 211 to 220 of about 13,340 (290)
Gravity and Magnetic Field Signatures in Hydrothermally Affected Regions on Mars
Abstract Multiple lines of evidence indicate that liquid water‐rock interactions occurred on ancient Mars, particularly within the crust, where hydrothermal systems have been hypothesized. Such hydrothermal circulation (HC) can significantly lower temperatures in the crust, thereby restricting the viscoelastic relaxation of impact craters. Craters with
Anna Mittelholz+3 more
wiley +1 more source
Abstract Mars may have had an ancient ocean filling its northern lowlands until around 3.5 billion years ago. The existence or lack of such a large body of water would have important implications on the ancient martian climate, landscapes, and habitability.
Zachary J. Baran, Benjamin T. Cardenas
wiley +1 more source
Perspectives on Mars Sample Return: A critical resource for planetary science and exploration. [PDF]
McSween HY, Hamilton VE, Farley KA.
europepmc +1 more source
Terrestrial and Habitable Planet Formation in Binary and Multi-star Systems
Nader Haghighipour+3 more
openalex +2 more sources
ON THE VALIDITY OF THE “HILL RADIUS CRITERION” FOR THE EJECTION OF PLANETS FROM STELLAR HABITABLE ZONES [PDF]
M. Cuntz, Katherine E. Yeager
openalex +1 more source
Heat Waves and Early Birth: Exploring Vulnerability by Individual‐ and Area‐Level Factors
Abstract Extreme heat has been linked to many health outcomes, including preterm and early term birth. We examine associations between acute heat wave exposure and risk of preterm (PTB) (28–36 weeks) or early term (ETB) (37–38 weeks) birth, stratified by individual‐level and area‐level factors.
A. Fitch+9 more
wiley +1 more source
The erosion of large primary atmospheres typically leaves behind substantial secondary atmospheres on temperate rocky planets. [PDF]
Krissansen-Totton J+3 more
europepmc +1 more source