# Saturn's rings in visible light and radio

- By: NASA / JPL / Space Science Institute
- Date: Visible light image taken 2004-12-12; radio data acquired 2005-05-03; combined image released 2005-05-23
- Classification: Photograph
- Credit line: http://photojournal.jpl.nasa.gov/catalog/PIA07874
- Museum: [Wikimedia Commons](https://commons.wikimedia.org/wiki/File:Saturn%27s_rings_in_visible_light_and_radio.jpg)
- Rights: Public domain
- Picture: https://invisiblenetwork.ai/thumbs/commons/thumb/1/1f/Saturn%27s_rings_in_visible_light_and_radio.jpg/1920px-Saturn%27s_rings_in_visible_light_and_radio.jpg
- Who can see it: Teens profiles and older (museums give no ratings; placed by Invisible Network from the museum's own words)

Cassini instruments provide complementary information about the structure of Saturn's rings. Narrow and wide angle cameras provide images in the visible region of the electromagnetic spectrum much like a digital camera does. The images have information about how the ring structure differs both with distance from the planet and with position around the equatorial circle. However, resolution is usually limited to few kilometers at best.

Radio and stellar occultations of the rings also provide important information about ring structure, but only along a one-dimensional track through the rings. The radial resolution can be as fine as 50 meters (164 feet). An "image" is then constructed by assuming circular symmetry over the ring region of interest. Color is usually added to encode other information related to the observed structure.

This image compares structure of Saturn's rings observed by these two approaches. The upper half is a natural color mosaic of images of the illuminated side of the rings by the Cassini narrow-angle camera (see PIA06175). The bottom simulated image is constructed from a radio occultation observation conducted on May 3, 2005. For another view created…