ESA Rosetta Mission to Comet 67P/Churyumov-Gerasimenko Could Shatter Mainstream ‘Dirty Snowball’ Comet Understanding – Electric Comet Model To Fill Gap

Three Surprising Comet Facts We’ve Already Learned from Rosetta

For the comet probe Rosetta, the good science is just beginning. But the long-traveled probe is already sending back surprises.

source JPL/NASA
source ESA/Rosetta CLICK PICTURE FOR FULL RESOLUTION
August 15, 2014
By William Herkewitz
Article from Popular Mechanics

Today, after 10 years of space travel, the Rosetta explorer became the first to orbit a comet. The best is yet to come—the scientists behind the satellite are preparing to land a harpoon-like probe on the surface this November. Yet new information is already pouring in. What scientists have discovered is already starting to transform our understanding of Rosetta’s target comet, 67P/Churyumov-Gerasimenko (C-G for short), and cometary science.

Here are three surprising facts we’ve already learned:

1. C-G looks nothing like we’d expect

Holger Sierks, the lead scientist behind OSIRIS—Rosetta’s 4-megapixel-camera—explains that while Rosetta has been approaching its rendezvous with C-G for years, the probe is only just now getting its first snapshots of the comet’s core. “It took us up until June just to fill one single pixel of our camera,” Sierks says. Now that the satellite is a mere 60 miles away, more recent images have detailed C-G’s odd shape: something halfway between a rubber ducky and a lumpy potato.


Current Standard Model of the ‘Dirty Snowball’ composition of Comets

cometcatcher.png

credit : Science Magazine CLICK PICTURE FOR FULL RESOLUTION


Rosetta Mission Findings by the Thunderbolts Project

No Room for Dirty Snowballs | Space News



“It was so surprising to see that this is not a [smooth], hull-shaped body, as we’ve thought it’d be,” Sierks says. The scientists are still putting together why the comet might have such an odd shape. One possibility is that C-G is actually two comets that have been fused together, he says, although it’s also possible the comet was somehow carved—through impacts or some other unknown force—into the strange figure.

2. The surface is hotter than we guessed, and surprisingly ice-free

Comets are largely composed of rock and ice, but strictly looking at the surface of C-G might make you think otherwise: “We recorded a maximum temperature that’s around [-63 degrees Fahrenheit],” says Fabrizio Capaccioni, the head of the mission’s thermal imaging camera. That temperature is hotter than the researchers would have guessed, and “that tells us that the first [inch] of the surface crust is porous, dusty, and contains almost no ice,” Capaccioni says.

Close up detail focusing on a smooth region on the ‘base’ of the ‘body’ section of comet 67P/Churyumov-Gerasimenko. (Photo Credit: ESA/Rosetta/MPS for OSIRIS Team)

Close up detail focusing on a smooth region on the ‘base’ of the ‘body’ section of comet 67P/Churyumov-Gerasimenko. (Photo Credit: ESA/Rosetta/MPS for OSIRIS Team)

This is a big surprise to the scientists, many of whom expected to find a glassy, clean surface of crystal ice. But the comet still is icy below the surface, “and we see water coming out, so there must be a way for the water to escape,” Capaccioni says.

3. Despite its dry surface, C-G expels an astronomical amount of water… but not on its dark side

Samuel Gulkis, the head of Rosetta’s water-tracking radio telescope, reported two months ago at a press briefing that C-G, though it is only 2.5 miles wide, expels so much water that “it would fill an Olympic-size swimming pool in about 100 days.”

Today he’s back with more data and reports that “one of the interesting things we’ve seen is that on the dark side of the comet, there’s very little gas, [including water,] being produced.” The facts about C-G’s water content are perhaps the most pressing to the scientists involved. Cosmic questions ranging from where Earth’s water came from to where and under what conditions comets like C-G originate all hinge on understanding the water on comets.

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