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

New names for gaps in Saturn's rings

Posted by Emily Lakdawalla

09-02-2009 13:35 CST

Topics:

According to a bulletin today from the USGS, there are nine new formal names for many gaps in the Saturnian ring system: Bond, Dawes, Herschel, Russell, Jeffreys, Kuiper, Laplace, Bessel, and Barnard. Here's a table, again copied from the USGS, detailing the locations of rings and ring gaps. The new Bond and Dawes gaps are located within the C ring; all the others are located within the Cassini Division.

NameDistance
rom planet's
enter (km)
Width (km)
D67,000 - 74,4907,500
C74,490 - 91,98017,500
Colombo Gap77,800100
Maxwell Gap87,500270
Bond Gap88,690 - 88,72030
Dawes Gap90,200 - 90,22020
B91,980 - 117,50025,500
Cassini Division117,500 - 122,0504,700
Huygens Gap117,680285 - 440
Herschel Gap118,183 - 118,285102
Russell Gap118,597 - 118,63033
Jeffreys Gap118,931 - 118,96938
Kuiper Gap119,403 - 119,4063
Laplace Gap119,848 - 120,086238
Bessel Gap120,236 - 120,24610
Barnard Gap120,305 - 120,31813
A122,050 - 136,77014,600
Encke Gap133,570325
Keeler Gap136,53035
Roche Division136,770 - 139,3802600
F140,22430 - 500
G166,000 - 174,0008,000
E180,000 - 480,000300,000

For context, here's Cassini's marvelous panorama across the complete ring system, including the gaps that had names at the time that the images were taken on May 9, 2007.

Panoramic scan across Saturn's rings (labeled)
Panoramic scan across Saturn's rings (labeled)
From a vantage point about a million kilometers away and 39 degrees to the north of the ring plane, Cassini scanned across the unlit side of Saturn's rings, acquiring images through multiple color filters. Images taken through red, green, and blue filters have been combined into this approximately natural color panorama, which shows details as small as 6 kilometers across (which is much larger than any of the individual particles within the rings). Because the light is shining from the back of the rings toward Cassini, parts of the rings that are mostly transparent but contain lots of fine dust, like the F ring and the Cassini division, are particularly bright. Credit: NASA / JPL / SSI
Here's a zoom on the Cassini division, showing the locations of the newly named gaps. They truly are gaps, devoid even of dust, because they look black regardless of whether Cassini sees the rings from the sunlit side or, as in the image here, with the Sun shining through the rings to Cassini. The Cassini division itself is not entirely empty; it's a black gap when you look at it with the Sun behind you (the classical view from Earth) but it has lots of dust within it, so when you see when you see it with the Sun shining from behind, it lights up as the dust scatters the light. But those gaps are still black. Something, most likely an orbital resonance where particles in those regions get a periodic and regular push from the gravity of one of Saturn's moons, keeps those black lanes free even of dust.
New names for gaps in the Cassini Division within Saturn's rings
New names for gaps in the Cassini Division within Saturn's rings
On February 9, 2009, the International Astronomical Union announced nine new names for gaps within Saturn's rings, including seven gaps within the Cassini division. The Cassini division separates Saturn's main A and B rings. Credit: NASA / JPL / SSI / diagram by Emily Lakdawalla
Some of you may be excited any time new names show up on maps of places in the solar system, but others may be wondering why these new names are important (especially because they all honor dead white guys). The reason they're important is because, in general, stuff in space does not get formally named until scientists need to be able to name things because they're getting ready to publish the results of research performed on those things. It's awkward to talk about "gap A" and "moonlet S/2004 S2" -- having formal names makes an article much easier to scan and understand. Which means that Cassini is doing its job: revealing previously unknown things to us so that we can study and understand them. Go Cassini!

 
See other posts from February 2009

 

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

Noachian valley networks near Newcomb Crater, Mars

Rosetta approaches Churyumov-Gerasimenko (5 NavCam views, July 23-27, 2014)
Shape model of comet 67P/Churyumov-Gerasimenko based on data up to July 24, 2014
Comet 67P/Churyumov-Gerasimenko on July 20, 2014
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!