Stephen Kane

@exocytherean.bsky.social

Planetary Astrophysicist at the University of California, Riverside. I like Venus. A lot. Exoplanets are also kinda cool.

I'm very excited for the ESA PLATO mission, for several reasons. One reason in particular: it will be a mean, lean Venus-analog finding machine that will greatly increase our ability to explore the Venus/Earth divergence. Read more in my new paper here: arxiv.org/abs/2607.14225

The Expected Yield of Venus Zone Terrestrial Planets from PLATO

The characterization of terrestrial exoplanets and the conditions that lead to divergent climate outcomes is a primary goal of exoplanetary science. The Venus Zone (VZ) provides a framework for identi...

arxiv.org

Tonight’s fireworks has competition. Venus is blazing in the western sky, a steady planetary lantern above all that beautiful human thunder. A reminder that not all fireworks are made on Earth. Happy July 4th!

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Don't forget to watch for Jupiter and Venus together after sunset! On June 9 they'll be very close but even now it's good. Look west after sunset. If it's clear you can't miss them lowish to the horizon. Venus is very bright.

My new paper explores the dynamical stability and habitability of the nearby HD 20794 system. The outer planet follows a highly eccentric orbit through the habitable zone, raising exciting questions for climate, architecture, and future HWO observations. arxiv.org/abs/2605.26217

Dynamical Stability and Habitability in the HD 20794 System

The Keplerian orbit of a terrestrial planet can be a significant driver in the evolution of surface conditions, as well as influencing the overall dynamics of the system. The HD 20794 system harbors t...

arxiv.org

If you've had a long day, go outside after sunset and admire the view of our beautiful planetary companions Venus and Jupiter toward the west, along with the first quarter moon overhead. It's soothing for the soul!

Venus is blazing in the western evening sky right now, and every time I look at it I’m struck by the contrast. To the eye it is serene and beautiful, yet the surface is one of the most hostile known locations. That visual tension is one reason I find Venus is so interesting.

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Venus advocacy is also exoplanet advocacy. Every improvement in our understanding of Venusian climate history, atmospheric loss, surface–atmosphere coupling, and volcanism sharpens how we interpret terrestrial exoplanets.

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As we move toward direct imaging and better atmospheric characterization of rocky exoplanets, Venus becomes even more important. We are going to need robust spectral and physical intuition for worlds that are cloudy, hot, chemically complex, and not remotely Earth-like.

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A big reason I advocate so strongly for Venus missions is that Venus is not a niche topic. It sits right at the intersection of planetary interiors, atmospheres, climate evolution, and exoplanet interpretation. The Venus story improves a huge fraction of planetary science.

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Venus’s atmosphere is a time capsule under pressure. Noble gases, isotopes, and trace chemistry can tell us whether Venus followed a fundamentally different path from Earth, or whether it began more clement and then changed profoundly over time. DAVINCI will provide the answers!

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One of the many things I love about EnVision is the mindset: Venus is a connected system. Interior, surface, atmosphere, and climate evolve together. To understand why Venus and Earth diverged so dramatically, we have to study those links directly.

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VERITAS is exactly the kind of mission Venus needs: high-resolution radar, topography, and surface composition at global scale. That’s how we move from debating resurfacing and tectonics to actually testing them.

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Every serious step forward on Venus helps us interpret rocky exoplanets better. “Earth-size” does not automatically mean Earth-like, and Venus is the Solar System reminder that planetary evolution can take a very different turn.

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Alpha Regio is one of the most interesting places in the Solar System. Its tessera terrain may preserve clues to ancient crustal processes on Venus, and DAVINCI is designed to explore that story by descending through the atmosphere to the surface.

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Venus isn’t just our nearest planetary neighbor. It’s one of the best tests we have for how rocky worlds diverge. If we want to understand habitability, climate evolution, and Earth-size exoplanets, we need the full Venus story.

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