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Stephen R. Kane

Stephen R. Kane

Astrophysicist and professorWikipedia

Search complete. 12 mentions across 5 episodes found for "Stephen R. Kane".

Sep 27, 2026

speaker_5HOST
34:07
We assume that because our moon is a beneficial companion, an exomoon must be a safe harbor.
speaker_5HOST
34:12
Stephen Kane's research shatters that assumption entirely.
speaker_4HOST
34:15
He explicitly points out that while a moon might offer benefits, it is not strictly required for a planet to be habitable.
speaker_4HOST
34:21
But what is absolutely required is that the planet doesn't drag its own moon out of the sky and drop it on its own biosphere.
Stuart GaryHOST
10:22
And that's where this new study comes in.
Stuart GaryHOST
10:24
The lead author, Stephen Kane from the University of California Riverside, says Venus didn't require a catastrophe to arrive at what we see today.
Stuart GaryHOST
10:32
He says it turns out the gravity of the planet itself, combined with the rate at which it spins, naturally caused any forming moon to collapse onto the surface.
Stuart GaryHOST
10:42
Scientists can precisely measure the exact distance between the Earth and the Moon because of NASA's Apollo 11 mission, which left laser retroreflective mirrors there.
Stuart GaryHOST
15:15
An astronomical unit is 150 million kilometers, the average distance between the Earth and the Sun.
Stuart GaryHOST
15:21
The new observations, reported in the journal Astronomy & Astrophysics, are based on studies by the Mid-Infrared Spectrograph aboard NASA's Webb Space Telescope.
Stuart GaryHOST
15:30
The study's lead author, Florian Pfitzker from the University of Cologne, says what makes the star so special is its enormous envelope, which has a radius of around 10,000 astronomical units.
Stuart GaryHOST
15:41
But sure, stars often show large envelopes.
Fred WatsonGUEST
7:56
Anyway, um, so yes, so Venus may have had the same experience.
Fred WatsonGUEST
8:01
Uh, what, uh, would have happened, though, if, uh, Venus had had a moon? Why isn't it there now? And so this is the, uh, thesis of a, a group of scientists, um, led by, um, Stephen Kane, who's at the University of California Riverside.
Fred WatsonGUEST
8:19
Uh, he, uh, and his colleagues have looked to see, you know, what might have happened had Venus had a moon.
Fred WatsonGUEST
8:30
So it's all done by modeling, of course.
Fred WatsonGUEST
10:36
Um, so it would break up.
Fred WatsonGUEST
10:39
Um, and, uh, the f- y- you know, even a, even a big moon, uh, would not necessarily survive.
Fred WatsonGUEST
10:47
Uh, in fact, one of the comments that Stephen Kane makes is an interesting aspect is that a heavier moon is destroyed faster since a massive moon would drain Venus's spin so efficiently that it hastens its destruction.
Fred WatsonGUEST
11:02
Uh, and so, um, that is the basic outcome of this work.
Andrew DunkleyHOST
13:02
Yeah.
Fred WatsonGUEST
13:02
Uh, let me, um, quote again, uh, Stephen Kane.
Fred WatsonGUEST
13:06
Uh, "Finding direct observational evidence is pretty tough.
Fred WatsonGUEST
13:10
A moon lost billions of years ago would leave little to no direct trace we can point a telescope at today."
Fred WatsonGUEST
13:20
However, there are indirect avenues.
Fred WatsonGUEST
13:22
For example, if a moon was destroyed and its debris rained down on Venus, it could have left a chemical fingerprint in the planet, planet's surface or atmosphere, and upcoming missions to Venus, including NASA's DAVINCI, uh, will measure the atmospheric composition in detail." So it is possible, uh, that we might eventually, um, find something.
Fred WatsonGUEST
13:46
Uh, one other comment from Stephen Kane is, "There's a broader test beyond our solar system because our results predict that slowly rotating Venus-like planets around other stars should generically lack large moons.
Fred WatsonGUEST
13:59
So as astronomers begin searching for moons around exoplanets, that's a prediction that can eventually be checked against real data."
speaker_2HOST
5:22
And that's exactly what researchers have done.
speaker_2HOST
5:25
A team led by astrophysicist Stephen R. Kane actually approached this exact problem by utilizing what we call N-body integrations.
speaker_4HOST
5:34
Okay, break that down for us.
speaker_2HOST
5:35
Sure.

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