Your notebook

A thought worth keeping.

Your observations, saved in this browser.

Browse Cassini observations

Your notebook holds your own drafts and saved views. Open any observation below to start exploring.

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Room for discovery

Every observation starts
with a little curiosity.

Explore the rings, notice a detail, and save the view.
Your questions and notes will be waiting here.

Explore data
MIT PRIMES 2026 · Saturn’s ringsBuilt for curiosity.

Sources & credits

Follow the source.

Cassini sent radio signals through Saturn’s rings toward Earth. Changes in those signals reveal structure across the rings.

Explore six archived observations here, compare exact samples, and keep a record of what you notice.

MIT PRIMES 2026

New Methods toward High-Resolution Reconstruction of Saturn’s Rings

Dell Li · Maiya Qiu · Yutong Zhao
Mentored by Dr. Ryan Maguire

What am I looking at?

These are Cassini RSS diffraction-limited ring profiles from NASA’s Planetary Data System. The three measured variables are normal optical depth, normalized signal power, and phase shift.

Wide views are reduced overviews. Narrow windows load the exact converted source records and verify their hashes. Optical depth is not a direct measure of ring mass; a pattern alone does not establish its physical cause. Missing and negative values are preserved.

Explore the team’s project research

Project research presents methods and reported results from the team’s working manuscript. The explorer displays archived observations; the method benchmarks are separate synthetic and scalar-model experiments. The full manuscript and scientific solver are not hosted here.

Background: an artistic rendering of Saturn.