Categories: Saturn

Saturn With Cassini’s Blue Filter

Image credit: NASA/JPL
Bands and spots in Saturn’s atmosphere, including a dark band south of the equator with a scalloped border, are visible in this image from the Cassini-Huygens spacecraft.

The narrow-angle camera took the image in blue light on Feb. 29, 2004. The distance to Saturn was 59.9 million kilometers (37.2 million miles). The image scale is 359 kilometers (223 miles) per pixel.

Three of Saturn’s moons are seen in the image: Enceladus (499 kilometers, or 310 miles across) at left; Mimas (398 kilometers, or 247 miles across) left of Saturn’s south pole; and Rhea (1,528 kilometers, or 949 miles across) at lower right. The imaging team enhanced the brightness of the moons to aid visibility.

The BL1 broadband spectral filter (centered at 451 nanometers) allows Cassini to “see” light in a part of the spectrum visible as the color blue to human eyes. Scientist can combine images made with this filter with those taken with red and green filters to create full-color composites.

In this image, everything on the planet is a cloud, and the contrast between bright and dark features is determined by the different blue-light absorbing properties of the particles that comprise the clouds. White regions contain material reflecting in the blue; dark regions contain material absorbing in the blue. This reflecting/absorbing behavior is controlled by the composition of the cloud’s colored material, which is still a mystery — one which may be answered by Cassini. The differing concentrations of this material across the planet are responsible for its banded appearance in the visible region of the electromagnetic spectrum.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The imaging team is based at the Space Science Institute, Boulder, Colo.

For more information about the Cassini-Huygens mission visit, http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org .

Original Source: CICLOPS News Release

Fraser Cain

Fraser Cain is the publisher of Universe Today. He's also the co-host of Astronomy Cast with Dr. Pamela Gay. Here's a link to my Mastodon account.

Recent Posts

Supermassive Black Holes Got Started From Massive Cosmic Seeds

One longstanding mystery in astronomy is how supermassive black holes got so heavy so early.…

13 hours ago

If You’ve Never Seen An Aurora Before, This Might Be Your Chance!

Tonight and the rest of the weekend could be your best chance ever to see…

1 day ago

Lighting Up the Moon’s Permanently Shadowed Craters

The Moon's polar regions are home to permanently shadowed craters. In those craters is ancient…

1 day ago

Here’s Where China’s Sample Return Mission is Headed

Humanity got its first look at the other side of the Moon in 1959 when…

1 day ago

Why Hot Jupiters Spiral into Their Stars

Exoplanets are a fascinating astronomy topic, especially the so-called "Hot Jupiters". They're overheated massive worlds…

2 days ago

Does the Milky Way Have Too Many Satellite Galaxies?

The Large and Small Magellanic Clouds are well known satellite galaxies of the Milky Way…

2 days ago