For my April 2025 diary, go here.

Diary — May 2025

John Baez

May 9, 2025

Did you see this? It's an artist's conception of how gravity from the tiny moon Daphnis creates ripples in Saturn's rings — created by Kevin Gill of NASA.

This image has been pretty popular on social media — but people often don't come out and say from the start that it's not a photo. The actual photos are less glamorous but... hey, they're real! And the ripples look different in the photos. Let's take a look.

This 2005 photo, taken by the Cassini probe, was the first time anyone actually saw Saturn's moon Daphnis! It's only 8 kilometers across. This gap in Saturn's A ring was first discovered by Voyager, and it was named the Keeler Gap. It's 35 kilometers wide. I guess this gap in the A ring let people guess the existence of a moon, and later the ripples in the let people guess where the moon must be. I don't really know the history here.

There's a larger gap in the A ring called the Encke Gap, created by a larger moon called Pan, which you can see clearly here.

To the left you see the smaller Keeler Gap. If you look very closely you can see the ripples near the Keeler gap... and if you look very closely you can see Daphnis!

Pan is closer to Saturn, so it orbits faster, and it overtakes Daphnis every 19 days.

Now here is a really great actual photo of Daphnis and the ripples it creates in Saturn's rings! It was taken by the Cassini probe and released in February 2017. It was taken in visible light using Cassini’s narrow-angle camera. Cassini was 28,000 kilometers away from Daphnis, and the image scale is 168 meters per pixel.

Above is a nice photo of Daphnis and the Keeler gap in real color. It was taken by Cassini on July 5, 2010 — taken in red, green, and blue and then recombined.

And here's an excellent image of Daphnis taken by the Cassini spacecraft on one of its ring-grazing passes on January 16, 2017 — the closest to Daphnis it's gotten so far, I believe!

NASA says:

Material on the inner edge of the gap orbits faster than the moon, so the waves there lead the moon in its orbit. Material on the outer edge moves slower than the moon, so waves there trail the moon. The waves Daphnis causes cast shadows on Saturn during its equinox when the sun is in line with the plane of the rings.

For my June 2025 diary, go here.


© 2024 John Baez
baez@math.removethis.ucr.andthis.edu

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