Flying Through an Icy Saltwater Spray

Cassini Probes Subsurface Oceans of Enceladus

As it swooped past the south pole of Saturn's moon Enceladus on 14 July 2005, Cassini acquired high resolution views of this puzzling ice world. Courtesy NASA/ESA/Space Science Institute

Take a look at that moon. It’s called Enceladus and it orbits the planet Saturn. It looks all serene and quiet, in this view. And, probably looks cold and lifeless.

But, in reality, this little world has a hidden ocean beneath that icy surface. And, as on Earth, when we we think “ocean”, we often think “life”.

How can such a cold-looking place support an ocean? Doesn’t it have to be… um… warm?  Well, as it turns out, a confluence of gravitational forces (between Saturn, Enceladus and neighboring moons)  keep the subsurface water just warm enough to exist as in a liquid-slushy state. Couple that with tectonic actions that crack the surface and allow water under pressure to escape out to space, and suddenly Enceladus is way more than a quiet, icy world. It’s a place that spouts plumes of ice crystals out to space.

And, since the Cassini Solstice mission spacecraft is there studying those worlds, and occasionally sails through these plumes, we get an instant sample of the interior saltwater reservoirs of Enceladus after it has sprayed out to space. The plumes originate from the ‘tiger stripe’ surface fractures at the moon’s south pole, and create the faint E-ring, which traces the orbit of Enceladus around Saturn.

Jets of icy particles bursting from Saturn's moon Enceladus are shown in this NASA/ESA/ASI Cassini image taken on 27 November 2005. This and other recent images of Enceladus backlit by the Sun show the fountain-like sprays of the fine material that tower over the south polar region. This image was taken looking more or less broadside at the 'tiger stripe' fractures observed in earlier Enceladus images. It shows discrete plumes of a variety of apparent sizes above the limb of the moon. Credits: NASA/JPL/Space Science Institute

Today, NASA and ESA released information about the sampling runs that the Cassini spacecraft has been making through the icy plumes that the spacecraft first discovered in 2005. During three passes, done in 2008 and 2009, the mission’s Cosmic Dust Analyzer measured the composition of icy grains that had just been ejected from Enceladus. Close to the moon, the plume particles are large and rich in salt. In fact, about 99 percent of the total mass of solid material ejected through these plumes is very salty — but  most of it falls back to the surface of this icy world.

So, how salty are we talking about?  It appears that the particles that are the saltiest have what scientists call an “ocean-like” composition. That tells us most of the ice that gets shot out in the plumes comes from liquid salt water inside Enceladus.

Scientists studying these plumes have come up with this scenario to explain the plumes: deep underneath Enceladus’ surface, perhaps 80 km down, there is a layer of water between the rocky core and the icy mantle (structural  layers). It is kept liquid by tidal forces generated by Saturn and some neighboring moons, as well as by the heat generated by radioactive decay (from elements that exist inside the moon and have been there since it formed).

Salt in the rock dissolves into the water, which accumulates in liquid reservoirs beneath the icy crust. When the outermost layer cracks open, the reservoir is exposed to space. The drop in pressure causes the liquid to evaporate, with some of it flash-freezing into salty ice grains: together these create the plumes.

Roughly 200 kg of water vapor gets lost every second as these plumes stream out to space.  According to the team’s calculations, the water reservoirs must have large evaporating surfaces, otherwise they would easily freeze over, and that would stop the plume action dead.

This is one of those findings that simply amazes me about what we are able to learn from our science missions in space. If I walked up to you on the street and asked you, “How can we figure out whether or not a frozen world out near Saturn has subsurface oceans, and how much salt would they have, if they exist?”  you would look at me blankly. It’s not on your daily radar, but that doesn’t make such a discovery unimportant.  If you stop to think about why we’d even want to know such a thing, it wouldn’t take long to make a connection between water, salt water, warm salt water and… life.  And, finding out places in our solar system where life could survive (and this is NOT a story about whether or not life exists there — that’s a whole other issue), tells us a lot about places where it DOES survive and exist. Mainly, here on Earth.  We know of extreme places on Earth that have similar environments to Enceladus — and life exists in those Earthly habitats.  So, now we know of at least one other place in the outer solar system where the conditions to harbor life mimic those on Earth.  Kinda makes Enceladus seem all warm, fuzzy, and neighborly, all of a sudden.  Not that life is there… but, the cradle of life is possible there.

Back from a Week Away

Exploring an Ice World

An unprocessed image of the moon Helene, orbiting Saturn. Taken by the Cassini spacecraft, June 18, 2011. Courtesy NASA/Cassini Solstice Mission.

I took a week off from writing (everybody  needs a short vacation, right?) and am now back in front of the screen, going through the latest astro-news.

What caught my eye first thing today was the ongoing Cassini Solstice mission. It’s the little spacecraft that just keeps going and going. While her older sisters Voyager and Pioneer are out exploring the outer limits of our solar system, and her little sister New Horizons is headed to Pluto, Cassini keeps sending back images and data about the Saturnian system. The latest views are of a little moon called Helene.

It’s an icy world, which is why I tuned into the story.  Today, June 20, we woke up to snow (which has since turned to rain).  Seems rather incongruous the day before summer solstice (for the northern hemisphere). But, the snow outside reminded me of the snow “out there” – orbiting Saturn like a lopsided iceberg.

It doesn’t take a very close inspection of the image to see the mottled, serrated-looking surface of this little world and to figure out that it looks just plain cold. As to be expected, since temperatures of ice worlds are far, far colder than the conditions we experience here on Earth. Helene is really an irregularly shaped chunk of ice that orbits Saturn in the same orbital path as another moon, Dione. It appears to have been beat up by collisions with other debris in Saturn’s orbit.

Spotting Another Ice Chunk in Space

Animation showing the comet moving against the background of stars. Images taken at the Pan-STARRS 1 Telescope on the night of June 5-6, 2011. Hawaii time is 10 hours earlier than Universal Time (UT). Credit: Henry Hsieh, PS1SC

The distant solar system contains many icy bodies, including these chunky worlds orbiting the gas and ice giant planets. But, there are icy chunks out there that aren’t gravitationally bound to any planets — and astronomers using the Pan-STARRS telescope on Haleakala in Hawai’i spotted one of them just outside the orbit of Jupiter. It’s a comet, called C/2001 L4 (PANSTARRS).  A preliminary orbit computed by the Minor Planet Center in Cambridge, Mass., shows that the comet will come within about 30 million miles (50 million km) of the sun in early 2013, about the same distance as Mercury. The comet will pose no danger to Earth.

The good news about this find is that as it gets closer to the Sun, astronomers have excellent chances to study this comet and figure out just how bright it will appear to be in our skies. If conditions are right, once the comet gets close enough to Earth (say, within the orbit of Mars), it should start to sprout a plasma tail. That’s the tail of ionized gases that streams out from a comet when it gets close enough to the Sun for solar radiation to heat up the gases (and cause them to glow).

It’s tough to know right now just what the composition of the comet is — certainly it’s made of ice. But, how much dust is embedded in that ice?  What kind of ice is it?  Astronomers should be able to tell as they study the comet’s tail with spectrographs (instruments that break up the light from an object into its component wavelengths — and each gas gives off a specific “fingerprint” in the spectrum).

Astronomers think that this comet could be on its first trip around the Sun.  It mostly like comes from the Oort Cloud, that collection of icy objects left over from the formation of the Sun and planets, some 4.5 billion years ago. This cloud lies at the very fringes of the solar system and is a treasure trove of objects that can tell us what conditions were like ‘way back when.

Keep an eye out for this comet in a couple of years. It probably won’t be easy to spot, but if you do see it, you’ll be seeing an object that harks back to a time when our Sun was still forming and the planets were still a work in progress.

Exploring Science and the Cosmos

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