Help Shape the Future of Space Exploration

Join The Planetary Society Now Join Now!

Join our eNewsletter for updates & action alerts

   Please leave this field empty
Blogs

Headshot of Emily Lakdawalla

Cassini eyes the eyeball

Posted by Emily Lakdawalla

16-02-2010 14:11 CST

Topics:

On Saturday, Cassini flew within 9,500 kilometers of Mimas, the innermost of the medium-sized icy moons of Saturn. Here's a view taken late in the flyby as Cassini was receding, showing the moon and its emblematic crater Herschel. Look at Mimas' shape -- it's clear in this view that Mimas is fatter across the middle than from pole to pole. This color version was assembled by Adam Hurcewicz, who has just started posting his image processing work to unmannedspaceflight.com. It's great to see more and more people getting in to the fun of playing with space image data!

Mimas in color

NASA / JPL / SSI / Adam Hurcewicz

Mimas in color
Cassini was about 71,500 kilometers from Mimas on February 13, 2010 when it captured the images for this false-color composite. Images taken through infrared, blue, and ultraviolet filters produce a view of the moon that emphasizes the interesting bluish color splotch on its leading hemisphere, centered on the giant crater herschel. The alignment of the color frames is not perfect because when it is as close to Saturn as Mimas' orbit, Cassini is moving very rapidly, so Mimas appeared to rotate from color frame to color frame. The background is not perfectly dark because Mimas was poised in front of Saturn at the time that these photos were taken. (Here is a simulated view from JPL's Solar System Simulator.)
This is Cassini's best encounter with Mimas to date, and it comes nearly six years into Cassini's mission. Why did it take Cassini so long to have a good flyby of Mimas?

Icy satellite scientist Paul Schenk explained the reasons in his blog, which I'll paraphrase here. Mimas orbits close to the outer edge of Saturn's ring system -- its average orbital distance is about 186,000 kilometers, while the F and G rings are found at about 140,000 and 170,000 kilometers, respectively. In order to photograph Mimas up close, Cassini has to approach as close to Saturn as Mimas' orbit.

For much of the mission, Cassini's orbit has not ventured as close to Saturn as Mimas; Cassini's orbit periapsis has been farther away from the planet. The biggest exception to this statement, interestingly, was the periapsis on "orbit 0," that is, Cassini's orbit insertion, when the spacecraft actually passed between the F and G rings. At other times, Cassini has had periapses around 160,000 kilometers, but I guess Mimas just wasn't in the neighborhood at the time. The science team didn't seem to see particular reason to expend precious fuel to set up a close flyby with a moon that looks like a battered rock that's been passively accepting the incessant banging of impactors without mustering much internal geologic activity, unlike its much more flamboyant neighbor, Enceladus.

Clearly Paul, at least, was looking forward to a closer look. He wrote:

It would be a mistake to disregard Mimas as a cold cratered lump of ice, however. All of Saturn's other icy moons have betrayed some level of geologic activity in their past. The largest crater Herschel, about 130-140 kilometers across and 11-12 kilometers deep, is one of the deepest in the Solar System. It may also be relatively young, providing an opportunity to study how craters on these icy worlds form and what they might tell us about the interior. Voyager mappers, myself included, saw sets of linear grooves that are most likely extension fractures crosing the globe. Whether these fractures formed when Mimas cooled and expanded or when Herschel knocked Mimas for a loop remains to be determined. Herschel was potentially large enough to have fractured Mimas throughout.

Diminutive Mimas, named after a giant (!) of Greek mythology, is only 400 kilometers across. It is also distinctly non-spherical as its polar axis is 10% shorter than the longer equatorial axes. The degree of sphericity could be used to tell whether Mimas has a small rocky core or not (it is otherwise mostly made of ices). Plus there is something very new (to us at least). I reported on this in one of my October blogs. It is a lens-shaped deposit of "bluish" "stuff" along the equator of Mimas' leading (forward-facing) hemisphere. This material appears to coat the cratered surface. We now have an explanation for this feature, and a similar one on Tethys. Unfortunately I can't tell you the exact answer right now, as this paper has been submitted for review and we should wait until it is approved. I will post all the details on this phenomenon in a few weeks!

So what did Cassini see in this rare close look? Cassini was moving so fast during the flyby (that's what happens during periapsis) that the number of images was somewhat limited compared to similarly close encounters of other moons, but the details were pretty cool. The first thing I do when I sit down to look at a set of Cassini encounter images is to just lay them all out like cards on a table to see how they all fit together. I also rotate them all to put north up, which makes it easier to get oriented as I try to match features to Mimas' map. In this effort I was greatly helped by Jason Perry's Looking Ahead article, which explained how the images were organized: there were two seven-frame mosaics of Mimas' disk, one six-frame "ride-along" observation where the camera scanned Mimas disk, and a final multispectral view of Mimas filling one frame (a color version of which is at the top of this post).
Cassini's February 13 flyby of Mimas

NASA / JPL / SSI / montage by Emily Lakdawalla

Cassini's February 13 flyby of Mimas
On February 13, 2010, Cassini flew within 9,500 kilometers of Mimas, the closest encounter yet with the smallest of Saturn's round satellites. Cassini approached from the night side and retreated with a nearly full-phase view of Mimas' leading hemisphere including the giant crater Herschel. The highest resolution view (the bottom center frame of the first mosaic) shows Herschel from a distance of about 15,000 kilometers away. Two multispectral mosaics covered most of the visible disk around the crater Herschel. A few last images were caught as the camera "rode along" with an observation by one of the other optical instruments, and a last full-globe, multispectral shot of Mimas caught it completely filling the frame with the limb of Saturn as a backdrop.
Since the big story on this flyby was the closeness of the approach, I thought I'd put together a mosaic of the closest approach images. There are two frames that catch the southeast portion of Herschel and an area to its east. Here's what they look like assembled:
Closeup on Herschel

NASA / JPL / SSI / mosaic by Emily Lakdawalla

Closeup on Herschel
Cassini's two highest-resolution views from its February 13, 2010 flyby of Mimas caught the southern half of the crater Herschel and an area to its east. This view is composed of two clear-filter images taken from the raw JPEG website. They were rotated to put north up and their levels adjusted to make the coloration fairly continuous. Level adjustment is not perfect because of the automatic contrast stretch applied to the raw JPEG images.
One of the notable things about this view is the relative lack of craters within Herschel and on the striated ejecta radial to Herschel. Since surfaces accumulate craters as they age, lack of craters implies a relatively young age. We knew this about Herschel before, but it's still kind of neat to see it confirmed in detail. Across the solar system, there are lots of places that have giant craters, but usually those giant craters are very old; they've been modified a great deal by later impacts. Studying Herschel up close should provide a clearer view of what happens to an icy moon when something big hits it.

There's something else that I find kind of exciting in the image, and that's the dark jaggedy stripe along the southern wall of Herschel. Here's a closeup view on that:

Herschel's southern wall

NASA / JPL / SSI

Herschel's southern wall
My first instinct when I see a stripe in a crater wall is "layers." But I think it's pretty clear that this stripe is not evidence for internal layering within Mimas. It doesn't follow topography the way that it would do if it were a horizontal layer cut into by the impact crater. Instead, it looks for all the world like the edge of a spill or splash, like the line left on a beach after waves have washed up it. It has that kind of lobate shape. This is a big impact crater into an icy moon; could this dark line have something to do with impact melt? I don't know -- that's just my wild guess. Also, I wonder if that's a relatively fresh crater near the left side of the detail image, the dark- and bright-rayed splotch.

Nearly six years into its mission, Cassini continues to deliver cool pictures!

 
See other posts from February 2010

 

Or read more blog entries about:

Comments:

Leave a Comment:

You must be logged in to submit a comment. Log in now.
Facebook Twitter Email RSS AddThis

Blog Search

JOIN THE
PLANETARY SOCIETY

Our Curiosity Knows No Bounds!

Become a member of The Planetary Society and together we will create the future of space exploration.

Join Us

Featured Images

Lunokhod 2 panorama

Lunokhod 2 traverse overview
LROC NAC view of Lunokhod 2 tracks
Lunokhod 2 panorama of the Fossa Recta
More Images

Fly to an Asteroid!

Travel to Bennu on the OSIRIS-REx spacecraft!

Send your name

Join the New Millennium Committee

Let’s invent the future together!

Become a Member

Connect With Us

Facebook! Twitter! Google+ and more…
Continue the conversation with our online community!