A defining characteristic of the planet Venus is its thick, CO2-dominated atmosphere. Despite over fifty years of robotic exploration, including thirteen successful atmosphere probes and landers, our knowledge of N2, […]
Venus
Solar XUV And ENA-driven Water Loss From Early Venus' Steam Atmosphere
The influence of the hydrogen hydrodynamic upper atmosphere escape, driven by the solar soft X-ray and extreme ultraviolet radiation (XUV) flux, on an expected magma ocean outgassed steam atmosphere of […]
Was Venus Once Warm And Wet? New Study of Lava Flow Suggests Not
A new study of the Ovda Fluctus lava flow on Venus indicates that it is made of basaltic lava. This discovery weakens the notion that Venus might once have been […]
Predicting The Yield of Potential Venus Analogs From TESS And Their Potential for Atmospheric Characterization
The transit method is biased toward short orbital period planets that are interior to their host star’s Habitable Zone (HZ). These planets are particularly interesting from the perspective of exploring […]
Venus As A Laboratory For Exoplanetary Science
The current goals of the astrobiology community are focused on developing a framework for the detection of biosignatures, or evidence thereof, on objects inside and outside of our solar system. […]
Consequences Of Tidal Dissipation In A Putative Venusian Ocean
The solar tide in an ancient Venusian ocean is simulated using a dedicated numerical tidal model. Simulations with varying ocean depth and rotational periods ranging from -243 to 64 sidereal […]
Venus As An Analog for Hot Earths
Here, we evaluate our nearest planetary neighbor, Venus, as an exemplar of the runaway greenhouse state that bounds the inner edge of the habitable zone. Despite its current hellish surface […]
Is There Life Adrift in the Clouds of Venus?
Mars has geological features that suggest it once had — and still has — subsurface liquid water, an almost sure prerequisite for life. Scientists have also eyed Saturn’s moons Titan […]
Modeling Venus-Like Worlds Through Time
We explore the atmospheric and surface history of a hypothetical paleo-Venus climate using a 3-D General Circulation Model. We constrain our model with the in-situ and remote sensing Venus data […]
Venus: The Making of an Uninhabitable World
The goals of the astrobiology community are focussed on developing a framework for the detection of biosignatures, or evidence thereof, on objects inside and outside of our solar system. A […]
