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  #631 (permalink)  
Old 09-October-2008, 03:37 PM
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Default 4-1/2 hours to closest approach

Timeline at: Planetary Society Weblog: Cassini flies within 25 kilometers of Enceladus tomorrow

Closest approach
2008 October 09, 1207 PDT, Thursday
2008 October 09, 1507 EDT, Thursday
2008 October 09, 1907 UTC, Thursday

4-1/2 hours to closest approach
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Old 09-October-2008, 08:52 PM
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Timeline at: Planetary Society Weblog: Cassini flies within 25 kilometers of Enceladus tomorrow

Coming up now:

Quote:
[12:52:40 PDT; 15:52:40 EDT; 19:52:40 UTC] Enceladus enters Saturn's shadow
Enceladus will remain in eclipse for 2.5 hours.
45 minutes past closest approach

===

From the inbound: Planetary Photojournal: Focus on Enceladus


Quote:
Ring shadows line the face of distant Saturn, providing an exquisite backdrop for the brilliant, white sphere of Enceladus. This icy moon, with its heavily modified surface and towering plume of icy material, is a target of intense study for Cassini during its Equinox mission.
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Old 11-October-2008, 06:26 PM
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There will be a series of DPS40 talks on Enceladus, live-streamed, today at 2:30 EST.

The link to the stream is:
http://cornellmediasite.cit.cornell....playerType=WM7

Last edited by borman; 11-October-2008 at 06:31 PM.. Reason: time correction
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Old 11-October-2008, 06:41 PM
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Quote:
Originally Posted by borman View Post
DPS40
Considering, and rejecting, Department of Public Sanitation, my mind turned to a faint memory of Emily Lakdawalla recently mentioning some meeting with webcasts.

Planetary Society Weblog: Cassini flies within 25 kilometers of Enceladus [October 9]

Quote:
I expect to learn much more about the results from August -- and possibly even from tomorrow's encounter -- at the upcoming Division of Planetary Sciences meeting, which begins on Friday. Sadly, the Society couldn't afford to send me to the conference this time around, but I'm very happy to learn that many (all?) of the oral sessions will be streamed live over the Web. I plan to tune in -- if you can stomach the scientific discussion, you're welcome to also!
Such as (times EDT):

Quote:
[Saturday, October 11]
Early Afternoon Session: 1:30 to 2:30 p.m.
Session 7: Special Session: Dynamical Classification of Planetary Bodies: http://cornellmediasite.cit.cornell....9-6f48d0706d61

Mid-Afternoon Sessions: 2:30 to 3:30 p.m.
Session 8: Enceladus: http://cornellmediasite.cit.cornell....b-ded936f07705
Session 9: Moon: http://cornellmediasite.cit.cornell....1-c1e8f214aea9
Edit: I tried the "Dynamical Classification of Planetary Bodies" which should have started half-past the hour, but all I get is "Waiting for presentation to begin". It's 20 minutes late (now) or something's not working or misscheduled.

DPS 40, the 40th meeting, AKA DPS08, has a website at Cornell: 40th annual meeting of the Division for Planetary Sciences of the American Astronomical Society

Edit: Something's not working. But something else is, in the wrong place. I found, underway:

Dynamical Classification of Planetary Bodies: http://cornellmediasite.cit.cornell....9-6f48d0706d61

at:

Enceladus: http://cornellmediasite.cit.cornell....b-ded936f07705

Edit: They swapped the URLs for the above two.

Enceladus presentation is at: http://cornellmediasite.cit.cornell....9-6f48d0706d61 and the webcast is on now, but the speaking hasn't quite started. Edit. Wait. No, it looks like a repeat the "Dynamical Classification of Planetary Bodies" talk at that URL (but the viewer software calls it "Enceladus"). Grr. Where's Enceladus?
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Old 11-October-2008, 07:35 PM
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http://cornellmediasite.cit.cornell....playerType=WM7

The links in the program got transposed.
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Old 11-October-2008, 07:36 PM
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There will be a series of DPS40 talks on Enceladus, live-streamed, today at 2:30 EST.

What defines a planet? :
http://cornellmediasite.cit.cornell....playerType=WM7

Enceladus:

http://cornellmediasite.cit.cornell....playerType=WM7
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Old 11-October-2008, 07:48 PM
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Quote:
Originally Posted by borman View Post
Right now, that should be Enceladus. The title in the viewer is "Enceladus". But it's the 4-speaker presentation on dynamic classifications of planets, recently done live.
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Old 11-October-2008, 07:52 PM
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Right now: Enceladus: http://cornellmediasite.cit.cornell....9-6f48d0706d61

Viewer has it entitled: "Special Session: Dynamical Classification of Plantary Bodies" but it's Enceldaus right now. Later it may be a replay of planet classification. It's live, Enceladus now.

I should add that later, also, it may possibly be a replay of the Enceladus presentation.

The Cornell Mediasite I presume, from a small sampling, has channels for presentations. If the live webcast hasn't begun, a slide tells you it hasn't started. If you come in later, it replays a record of the live presentation from earlier. If you're lucky. And if the URLs aren't swapped between two different presentations, and the phase of the moon is just right.
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Old 11-October-2008, 09:25 PM
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An interesting set of talks.

Now, it seems the heat is climbing upwards to 13 GW. There may be a heat transition in one of the stripes, but it is too early to be sure of this. The high resolution pass gave lower (around 167K) compared to an earlier pass (187K). There is a pressure constraint that impacts on the "Cold Faithful" and Nimmo friction theories. There seems to be a large error in determining the age of the stripes. From one consideration they might be over 3 billion years old, but from cometary impacts only 400 million years or less. Tidal stress and libration can give heat, but it is unusual that it is not over the entire moon, like Europa, and only at the South Pole.

(Personal comment: Tidal stresses might not be responsible for the stripes, but they may be important for maintaining them and preventing them from "healing" or freezing up)

The flexing of the stripes might be responsible for the "shark fin" features. There was no discusiion of the October 9 data other than to acknowledge its reception. Perhaps the AGU talks will include this recent data.
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Old 12-October-2008, 03:29 PM
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Gad, I wish I had wandered into this thread yesterday...or Emily's invitation; I used to read every word in her blog, and I have to do so again. That the Planetary Society can't afford to send her is another troubling sign of the times; so to speak - the very real effect upon those who rely upon donations from the public to function. In many cases, these donations turn into trusts; and the budget is spawned from the revenue yield these trusts. But in a grueling market where trillions of dollars evaporate; so do the revenues from trust funds.

But back to the tiger stripes: The surface temperature measured is a minimal constraint upon the temperature of the engine below. Also, even though the second pass should have had higher resolution (and less of the colder surface mass impinging upon the reading) the 20 deg K increase is really a confirmation of the earlier pass. Amazing phenomenon. If we were truly a geek society; we would have another mission on the way and and at least two more missions planned. It would be interesting (saddening) to know how much more the media spends covering Paris Hilton's faux campaign than it does covering DPS40.
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Old 16-October-2008, 02:00 AM
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The Hi-Res readings were the colder readings. Because the instrument works in a non-linear way, they want to check for possible systematics being responsible for the change at Damascus rather than announce the the temperature fall is real. One of the possible models if the change is real is to consider that the heat engine is turned off for just Damascus. This might imply a moving "hot spot" beneath the surface, something similar to how the Hawiian Islands are made.

Also of interest is the identification of relic tiger stripes and offsets where one piece of stripe got separated by faulting from the main relic stripe body. It is sort of like a jig-saw puzzle or rubrics cube where the history needs to be re-assembled by partial rotations which in turn may give some idea of the timescale over which these rotations occured. Maybe one can trace the motions of the "hot spot" by the re-assembly of relic stripes.
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Old 16-October-2008, 01:10 PM
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According to the VIMS instrument, Titan's lakes are only millimeters thick which means the lakes are actually either dry mudflats or are coated with a thin film of something that block sunlight. No data from north polar lakes available yet, though. Specular reflections may have been seen.

Speaking of north polar lakes, Titan's thick atmosphere bends light which allows Cassini to peek lakes beyond the terminator that have so far been in darkness.

New dark splotches have appeared in the southern polar region suggesting that the lakes there are starting to fill as the southern summer is coming to an end. There apparently have been torrential rains in the recent months.
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Old 25-October-2008, 01:22 AM
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Not new, but well done.

Courtesy of BA Blog: The Big Picture: Enceladus

Boston.com does Enceladus up close
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Old 25-October-2008, 02:09 PM
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Those pictures are beautiful.
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Old 31-October-2008, 07:11 PM
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About 30 minutes past Enceladus closest approach.

NASA Enceladus Blog

Quote:
Well, here we go again! Close on the heels of the first two exciting and successful targeted Enceladus flybys of the Cassini Equinox Mission, we have another Enceladus encounter this week!

[October 31 UTC] is the third of three Enceladus flybys in a series [...]
dmuller has a great countdown and clock page that will provide temporal orientation for this flyby: Cassini Real-Time Simulation

Outbound observations underway.

In about 3 days there is a Titan flyby, 2008 November 3, 1735 UTC. (Roughly. Approaching end of daylight saving time for me is obscuring my vision.)
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Old 02-November-2008, 01:25 AM
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BA Blog: Cassini hi-reses Enceladus

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It almost doesn’t look real, does it? Click to get to more images, including embiggened ones. This mosaic has a max resolution of 12.3 meters per pixel! Those little round boulders you can see in the (hi-res) image? Yeah, they’re not much bigger than a typical house.
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Old 06-November-2008, 11:17 PM
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Planetary Society Weblog: Enceladus!

Quote:
Nearly a week after yet another super-close flyby of Enceladus by Cassini, I am finally taking the time to try and work through the pictures and make sense of them. Unfortunately, I am not sure I can say anything much more intelligent about these images than, "wow, these are cool."
Lots of yummy images there.
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Old 07-November-2008, 12:25 AM
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New thermal readings of potential cooling hot spots might help sort out if the temperature change was a systematic or real and if the hot spot has cooled even more since the last flyby. This might help set some constraints on the heating mechanism.

The new images may present some more jig-saw puzzle images for re-assembling relic tiger stripes.
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Old 26-November-2008, 10:29 PM
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Universe Today: Underground Water Reservoirs Power Geysers on Enceladus

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Saturn's moon Enceladus may indeed hide an underground reservoir of water. Scientists analyzed the plumes seen spewing from the moon with the Cassini spacecraft, and found water vapor and ice. "There are only three places in the solar system we know or suspect to have liquid water near the surface," said Joshua Colwell Cassini team scientist from the University of Central Florida. "Earth, Jupiter's moon Europa and now Saturn's Enceladus. Water is a basic ingredient for life, and there are certainly implications there. If we find that the tidal heating that we believe causes these geysers is a common planetary systems phenomenon, then it gets really interesting."

Using data from Cassini's Ultraviolet Imaging Spectrograph (UVIS), the team's findings support a theory that the plumes observed are caused by a water source deep inside Enceladus. An Earth analog is Lake Vostok in Antarctica, where liquid water exists beneath thick ice.
[...]
Although there is no solid conclusion yet, there may be one soon. Enceladus is a prime target of Cassini during its extended Equinox Mission, underway now through September 2010.
Nature News: Enceladus shoots supersonic jets of water

Quote:
Four supersonic jets of water vapour have been detected within the enormous geyser of gas and dust that spurts from the south polar region of Saturn's icy moon Enceladus. [...]
JPL News: Enceladus Jets: Are They Wet or Just Wild?
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Old 12-December-2008, 03:31 AM
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Maintaining a heated ocean by resonance absorption


A recent article published in Nature invokes large amplitude Rossby waves to capture obliquity tidal energy 3 orders more efficiently than normal tidal forces contribute:

Strong ocean tidal flow and heating on moons of the outer planets

Abstract: http://www.nature.com/nature/journal...ture07571.html


Recently, tidal force theory took a hit when it was discovered that the plumes were more active at the wrong place in the orbit of Enceladus. But considering the 3 orders of magnitude increase where the lake is of just the right size to admit the resonance constructively, this may help resolve the Goldilocks problem that makes Enceladus special.

The effect seems similar to the Tesla earthquake machine theory or the anecdote regarding the tenor who sings the correct pitch to shatter a crystal glass that absorbs the energy. Similar is where a key an octave or twelfth above another key on a piano is softly depressed so that only the damper is raised and then the fundamental is struck loudly and then damped; one can hear the energy of the overtones captured by the lightly depressed key. If the fundamental pitch loudly struck does not contain the higher depressed key in its overtone structure, then the energy transfer is much less amplified.

There may be a condition of equilibrium that is attained where the heating causes the lake to grow beyond the harmonic, only to freeze to shrink back to the correct harmonic to then accept the tidal harmonic energy. It tends to be self-maintaining. The plumes may serve as a governor if the heating gets too hot on occasion.

There still remains the problem of how the lake initially formed from solid ice to reach the volume to where resonance absorption can kick in to sustain the heat.
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Old 15-December-2008, 11:53 PM
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NASA Cassini-Huygens Mission News Release: Saturn's Dynamic Moon Enceladus Shows More Signs of Activity

Quote:
The closer scientists look at Saturn's small moon Enceladus, the more they find evidence of an active world. The most recent flybys of Enceladus made by NASA's Cassini spacecraft have provided new signs of ongoing changes on and around the moon. The latest high-resolution images of Enceladus show signs that the south polar surface changes over time.
Quote:
"Of all the geologic provinces in the Saturn system that Cassini has explored, none has been more thrilling or carries greater implications than the region at the southernmost portion of Enceladus," said Carolyn Porco, Cassini imaging team leader at the Space Science Institute in Boulder, Colo.

A panel of Cassini scientists, including Porco, presented these new findings today in a news briefing at the American Geophysical Union's fall meeting in San Francisco.
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Old 15-December-2008, 11:57 PM
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Planetary Society Weblog: Ganesa Macula isn't a dome

Surprise!

Quote:
I'll have much more to say about Titan later today, but this was perhaps the most surprising point made in this morning's sessions at the American Geophysical Union meeting about Saturn's largest moon, Titan: Ganesa macula is not a dome.

Most of you are probably saying "The what what isn't a dome? And why should I care?" So let me explain. First of all, here is a Cassini radar image of the feature on Titan that is named Ganesa Macula.
Quote:
But Ganesa is not a dome, which means it's no longer resonable to cite it as the most obvious example of a cryovolcanic feature on Titan.
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Old 29-January-2009, 07:49 PM
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Cassini press release:

Quote:
MEDIA RELATIONS OFFICE
CASSINI IMAGING CENTRAL LABORATORY FOR OPERATIONS (CICLOPS)
SPACE SCIENCE INSTITUTE, BOULDER, COLORADO
http://ciclops.org

Joe Mason (720) 974-5859 CICLOPS/Space Science Institute, Boulder, Colo.

Michael Buckley (240) 228-7536 Johns Hopkins University Applied Physics Laboratory, Laurel, Md.

For Immediate Release: January 29, 2009

CASSINI FINDS HYROCARBON RAINS MAY FILL TITAN LAKES

Recent images of Titan from NASA's Cassini spacecraft affirm the presence of lakes of liquid hydrocarbons by capturing changes in the lakes brought on by rainfall.

For several years, Cassini scientists have suspected that dark areas near the north and south poles of Saturn's largest satellite might be liquid-filled lakes. An analysis published today in the journal Geophysical Research Letters of recent pictures of Titan's south polar region reveals new lake features not seen in images of the same region taken a year earlier. The presence of extensive cloud systems covering the area in the intervening year suggests that the new lakes could be the result of a large rainstorm and that some lakes may thus owe their presence, size and distribution across Titan's surface to the moon's weather and changing seasons.

The high-resolution cameras of Cassini's Imaging Science Subsystem (ISS) have now surveyed nearly all of Titan's surface at a global scale. An updated Titan map, being released today by the Cassini Imaging Team, includes the first near-infrared images of the leading hemisphere portion of Titan's northern "lake district" captured on Aug. 15-16, 2008. (The leading hemisphere of a moon is that which always points in the direction of motion as the moon orbits the planet.) These ISS images complement existing high-resolution data from Cassini's Visible and Infrared Mapping Spectrometer (VIMS) and RADAR instruments.

Such observations have documented greater stores of liquid methane in the northern hemisphere than in the southern hemisphere. And, as the northern hemisphere moves toward summer, Cassini scientists predict large convective cloud systems will form there and precipitation greater than that inferred in the south could further fill the northern lakes with hydrocarbons.

Some of the north polar lakes are large. If full, Kraken Mare -- at 400,000 square kilometers -- would be almost five times the size of North America's Lake Superior. All the north polar dark "lake" areas observed by ISS total more than 510,000 square kilometers -- almost 40 percent larger than Earth's largest "lake," the Caspian Sea.

However, evaporation from these large surface reservoirs is not great enough to replenish the methane lost from the atmosphere by rainfall and by the formation and eventual deposition on the surface of methane-derived haze particles.

"A recent study suggested that there's not enough liquid methane on Titan's surface to resupply the atmosphere over long geologic timescales," said Dr. Elizabeth Turtle, Cassini imaging team associate at the Johns Hopkins University Applied Physics Lab in Laurel, Md., and lead author of today's publication. "Our new map provides more coverage of Titan's poles, but even if all of the features we see there were filled with liquid methane, there's still not enough to sustain the atmosphere for more than 10 million years."

Combined with previous analyses, the new observations suggest that underground methane reservoirs must exist.

Titan is the only satellite in the solar system with a thick atmosphere in which a complex organic chemistry occurs. "It's unique," Turtle said. "How long Titan's atmosphere has existed or can continue to exist is still an open question."

That question and others related to the moon's meteorology and its seasonal cycles may be better explained by the distribution of liquids on the surface. Scientists also are investigating why liquids collect at the poles rather than low latitudes, where dunes are common instead.

"Titan's tropics may be fairly dry because they only experience brief episodes of rainfall in the spring and fall as peak sunlight shifts between the hemispheres," said Dr. Tony DelGenio of NASA's Goddard Institute for Space Studies in New York, a co-author and a member of the Cassini imaging team. "It will be interesting to find out whether or not clouds and temporary lakes form near the equator in the next few years."

Titan and the transformations on its surface brought about by the changing seasons will continue to be a major target of investigation throughout Cassini's Equinox mission.

The Titan map and images of the lakes are available at: http://ciclops.org, http://saturn.jpl.nasa.gov , and http://www.nasa.gov/cassini .

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory (JPL), a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team consists of scientists from the U.S., England, France, and Germany. The imaging operations center and team leader (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo. The Applied Physics Laboratory, a division of Johns Hopkins University, meets critical national challenges through the innovative application of science and technology.
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Old 07-February-2009, 06:09 AM
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"The presence of extensive cloud systems covering the area in the intervening year suggests that the new lakes could be the result of a large rainstorm and that some lakes may thus owe their presence, size and distribution across Titan's surface to the moon's weather and changing seasons."

Suggestions should always be taken with a grain of caution: If you've been around long enough, you know how certain we were that there was plant life, growing and ebbing on Mars ~50 years ago.

I don't object to methane rains on Titan, but I think if there is a vibrant methane cycle, we should have found higher concentrations of ethane and other more complex organics during Huygens descent, especially in the lower atmosphere and very near the surface, and that the concentrations of these hydrocarbons on the surface should be black, not red: Organics polymerized by uv turn black. I think that the methane in the atmosphere on Titan, wherever it is coming from; is gradually escaping rather than concentrating and raining, just as it is on Mars. The colors are all wrong.
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Old 10-April-2009, 06:58 PM
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Two Iapetus videos:

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Iapetus Spins and Tilts

Saturn's two-faced moon tilts and rotates for Cassini in this mesmerizing movie sequence of images acquired during the spacecraft's close encounter with Iapetus on Nov. 12, 2005.
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Flight over Iapetus

Cassini sails low over the surface of Iapetus on approach to its close encounter with the enigmatic moon on Sept. 10, 2007.
Its flight takes it over the rugged, mountainous ridge along the moon's equator, where ancient, impact battered peaks -- some topping 10 kilometers (6 miles) in height -- are seen rising over the horizon and slipping beneath the spacecraft as it flies.
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Old 11-April-2009, 07:38 PM
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Cruising with Pan

'Saturn's small, walnut-shaped moon, Pan, embedded in the planet's rings, coasts along in this movie clip from the Cassini spacecraft.'
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Old 23-July-2009, 02:44 AM
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Cassini press release:

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Saturnian Moon Shows Evidence of Ammonia

Data collected during two close flybys of Saturn's moon Enceladus by NASA's Cassini spacecraft add more fuel to the fire about the Saturnian ice world containing sub-surface liquid water. The data collected by Cassini's Ion and Neutral Mass Spectrometer during Enceladus flybys in July and Oct. 2008, were released in the July 23 issue of the journal Nature.

"When Cassini flew through the plume erupting from Enceladus on October 8 of last year, our spectrometer was able to sniff out many complex chemicals, including organic ones, in the vapor and icy particles," said Hunter Waite, the Cassini Ion and Neutral Mass Spectrometer Lead Scientist from the Southwest Research Institute in San Antonio, Texas. "One of the chemicals definitively identified was ammonia."

On Earth, the presence of ammonia means the potential for sparkling clean floors and counter tops. In space, the presence of ammonia provides strong evidence for the existence of at least some liquid water.

How could ammonia equate to liquid water inside an ice-covered moon in one of the chillier neighborhoods of our solar system? As many a homeowner interested in keeping their abodes spick and span know, ammonia promptly dissolves in water. But what many people do not realize is that ammonia acts as antifreeze, keeping water liquid at lower temperatures than would otherwise be possible. With the presence of ammonia, water can exist in a liquid state to temperatures as low as 176 degrees Kelvin (-143 degrees Fahrenheit).

"Given that temperatures in excess of 180 Kelvin (-136 degrees Fahrenheit) have been measured near the fractures on Enceladus where the jets emanate, we think we have an excellent argument for a liquid water interior," said Waite.

Cassini discovered water vapor and particles spewing from Enceladus in 2005. Since then, scientists have been trying to determine if the plume originates from a liquid source inside the moon or is due to other causes.

"Ammonia is sort of a holy grail for icy volcanism," said William McKinnon,
a scientist from Washington University in Saint Louis, Missouri. "This is the first time we've found it for sure on an icy satellite of a giant planet. It is probably everywhere in the Saturn system."

Just how much water is contained within Enceladus' icy interior is still up for debate. So far, Cassini has made five flybys of Enceladus, one of the chief targets for Cassini's extended mission. Two close flybys are scheduled for November of this year, and two more close flybys are scheduled for April and May or 2010. Data collected during these future flybys may help settle the debate.

"Where liquid water and organics exist, is there life?" asked Jonathan Lunine a Cassini scientist from the University of Arizona, Tucson. "Such is the case for Earth; what was found on Enceladus bolsters this moon's promise for containing potential habitable environments."

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Cassini orbiter was designed, developed and assembled at JPL. JPL manages the mission for the Science Mission Directorate at NASA Headquarters in Washington.

More information about the Cassini mission is available at http://www.nasa.gov/cassini or http://saturn.jpl.nasa.gov .
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Old 01-September-2009, 09:28 PM
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Yet another amazing animation, this one compiled from the raw JPEGs by Bill Harris over at UMSF.com:
Janus undergoes an inverse eclipse, passing through the narrow slot of sunlight filtering through the Cassini Division.
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Old 06-September-2009, 12:00 PM
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Perhaps this has been mentioned here (it's a long thread), but in attending a panel at DragonCon yesterday given by four JPL Cassini-Huygens team members, I learned how they propose to end the spacecraft's mission. The concern is that if left to it's own devices after the propellant is exhausted, it might potentially impact one of the icy moons. The heat generated by the RTG might create a pool/puddle of liquid whatever where there had been none before and introduce an undesired variable in the local environment.

So, the proposal is to use the last of the fuel to whip the craft around Titan in such a way as to cause Cassini to go between the rings and the planet (there's just 3000 km safe separation), gather important data not available otherwise and then have it impact the planet on a subsequent go-round.
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Old 07-September-2009, 06:56 PM
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"The heat generated by the RTG might create a pool/puddle of liquid whatever where there had been none before and introduce an undesired variable in the local environment."
...
"impact the planet on a subsequent go-round."
And this will NOT introduce an undesired variable in the local environment?

I personally say, go to Saturn - close and personal.
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