Sub-Neptunes occupy an intriguing region of planetary mass-radius space, where theoretical models of interior structure predict that they could be water-rich, where water is in steam and supercritical state.
Water/Hycean Worlds & Oceanography
The First Billion Years: Habitability
The physical processes active during the first billion years (FBY) of Earth’s history, such as accretion, differentiation, and impact cratering, provide constraints on the initial conditions that were conducive to […]
Ocean World Exploration Tech: MBARI’s Advanced Technology
MBARI’s Environmental Sample Processor (ESP) enables scientists and resource managers to monitor the health of remote aquatic environments. Equipped with advanced biological sensors and a wireless data connection, this “lab […]
Illuminating The Mysteries Of Icy Ocean Worlds
As NASA’s Europa Clipper embarks on its historic journey to Jupiter’s icy moon, Europa, Dr. Matt Powell-Palm, a faculty member at Texas A&M University’s J. Mike Walker ‘66 Department of […]
Towards the Habitable Worlds Observatory: Visionary Science and Transformational Technology
We are pleased to announce the inaugural open community conference for NASA’s Habitable Worlds Observatory, to be held at the Johns Hopkins Bloomberg Center in Washington, DC, from July 28‐31, […]
Study Reveals Origins Of Lunar Water And Its Connection To Earth’s Early History
The team analyzed water in nine samples from the Apollo lunar mission, using a high-precision triple oxygen isotope technique. This method, developed by Dr. Morgan Nunn Martinez of the University […]
Earth’s Northernmost Seafloor Hydrothermal System Shows Even More Variety In Vent Styles Than Expected
A new study about Earth’s northernmost seafloor hydrothermal system shows even more variety in vent styles than previously thought. This has important implications for understanding the origin of these vents […]
New Evidence For Hidden Water Reservoirs And Rare Magmas On Ancient Mars
A new study explores how variations in Mars’ crustal thickness during its ancient history may have influenced the planet’s magmatic evolution and hydrological systems. The research, published in Earth and […]
Solving Meteorological Mysteries On Mars
A groundbreaking achievement by scientists at the University of Houston is changing our understanding of climate and weather on Mars and providing critical insights into Earth’s atmospheric processes as well.
Experimental Heating of Complex Organic Matter at Titan’s Interior Conditions Supports Contributions to Atmospheric N2 and CH4
Titan’s abundant atmospheric N2 and CH4 gases are notable characteristics of the moon that may help constrain its origins and evolution. Previous work suggests that atmospheric CH4 is lost on […]
