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Headshot of Emily Lakdawalla

New Rosetta views and first science on comet Churyumov-Gerasimenko from EPSC

Posted by Emily Lakdawalla

11-09-2014 16:56 CDT

Topics: Rosetta and Philae, pretty pictures, comets, amateur image processing, comet Churyumov-Gerasimenko, spacecraft

Just weeks after their arrival at comet Churyumov-Gerasimenko, the Rosetta science team showcased their first results at the European Planetary Science Congress. The session included results from most of the science teams, but arguably the most exciting "result" to come out of the mission this week was this view of the comet -- and the spacecraft studying it -- from the Philae lander. I've flipped the image 180 degrees so that the Sun appears to be illuminating it from the top.

Philae's passenger-side view of comet Churuymov-Gerasimenko

ESA / Rosetta / Philae / CIVA

Philae's passenger-side view of comet Churuymov-Gerasimenko
The Philae lander, attached to the side of Rosetta opposite its high-gain antenna, has six micro-cameras positioned around its circumference to capture panoramic views of its landing site after it touches down: the CIVA instrument. While Philae is still attached to Rosetta, two of CIVA's cameras are able to see the solar panels -- and sometimes other things, including, in this case, the comet. Churyumov-Gerasimenko was about 50 kilometers away when the spacecraft took this photo. Two images with different exposure times were merged to bring out the sunlit details on the comet in combination with the very faintly lit backside of the spacecraft's solar panels. This image has been rotated 180 degrees from the original so that solar illumination appears to be coming from the top.

The comet was brightly sunlit, but Philae and its cameras were on the shadowed side of the spacecraft and we're looking at the undersides of the solar panels (whose topsides are facing where they should be, toward the Sun). I was having trouble understanding the lighting geometry of this image because of what looked like bright hinges between the solar panels. So I went to dig up some photos of the solar panels under testing:

Rosetta's solar panels during deployment testing, May 2002

ESA / Anneke Le Floc'h

Rosetta's solar panels during deployment testing, May 2002
Rosetta's enormous five-paneled solar wings were tested at the European Research and Technology Centre, Noordvijk, the Netherlands, in May 2002. The spacecraft is oriented with its high-gain antenna upward and the Philae lander downward. The solar panels are steerable, able to rotate to catch the most favorable angle to the Sun.

And here's a related view, in which you can see how Philae is bolted to the spacecraft, with the panels folded at the side:

Rosetta and Philae prepare to undergo vibration testing, April 2002

ESA / Anneke Le Floc'h

Rosetta and Philae prepare to undergo vibration testing, April 2002
The box-shaped Rosetta spacecraft, fully assembled with solar panels folded at side and Philae lander attached, awaits vibration testing at the European Space Research and Technology Centre in Noordvijk, the Netherlands.

If you look closely at the joints between the panels, you can see that they are connected with some flexible electronic tape, a tape that is transparent. In the CIVA image of Rosetta at the comet, we're seeing the shaded backsides of the solar panels, but the Sun can shine through and into the tape that connects the panels, and some of that light is scattered toward the camera, making them appear bright. CIVA is a panoramic camera instrument, designed to capture the view around Philae once it lands on the comet. Most panoramic camera instruments on landers are single cameras on a rotating mast, but Philae's panoramic camera doesn't have moving parts; instead, it has six micro-cameras pointed in fixed directions. While Philae is attached to Rosetta, the two side cameras can see both of the solar panels. Handy! It has to be awesome for the team to be able to see the hardware they built, out there in space with the comet behind.

ESA / ATG medialab

Philae's panoramic camera
Rosetta's lander Philae is equipped with the CIVA instrument (Comet Infrared and Visible Analyser). CIVA has six microcameras used to take panoramic pictures. This artist’s impression shows Philae using CIVA to create a panoramic view of its surroundings. The comet surface is an artist’s impression.

So, on to science. For me, one of the most exciting pieces of news was that the COSIMA instrument has successfully collected comet dust and is ready to use its ion gun to turn the grains into ions and measure their composition with the instrument's ion mass spectrometer. "These are among the first dust grains to have been collected from beyond the Solar System’s snow line – the distance from the Sun at which ice grains can form," COSIMA principal investigator Martin Hilchenbach wrote in a blog post about the team's results.

COSIMA's first comet dust

ESA / Rosetta / MPS for COSIMA Team

COSIMA's first comet dust
Between August 11 and 24, the COSIMA instrument on Rosetta exposed a 1-centimeter-square target plate (left) to space to see if they could collect comet dust. Some time between August 17 and 24, the plate collected two large dust grains. More information via the ESA blog.

Both the ALICE ultraviolet spectrometer and the VIRTIS visible and infrared spectrometer are forming a picture of the comet as a very dark, relatively warm surface that lacks exposed water ice. "The new VIRTIS measurements have allowed the team to rule out some models of the comet surface and to favour a comet surface composed of a porous and  highly thermally insulating dusty crust that is depleted of water ice. As they reported today, this is also consistent with the VIRTIS global measurements of thermal inertia – a measure of a body’s resistance to changes in temperature – that is compatible with the value for high porosity dusty materials," VIRTIS PI Fabrizio Capaccioni wrote in a blog entry about his team's results. Alice has, however, detected the byproducts of water ice in the comet's coma.

And, finally, there was a new OSIRIS image of the comet. Almost all of the pictures that you have seen from the comet so far have come from the NavCam; this is the first OSIRIS photo in about a month, and only the second one ever that demonstrates how amazing the OSIRIS data set on the comet is going to be, in all its 4-megapixel glory. OSIRIS is the biggest framing camera on a deep-space mission; its 2048-pixel-square photos are worth examining in all their incredible detail. By popular demand, I have added a scale bar onto the photo.

OSIRIS view of comet Churyumov-Gerasimenko on September 5, 2014

ESA / Rosetta / DLR / MPS for OSIRIS Team MPS / UPD / LAM / IAA / SSO / INTA / UPM / DASP / IDA

OSIRIS view of comet Churyumov-Gerasimenko on September 5, 2014
Rosetta's highest-resolution camera, OSIRIS, snapped this view looking across the "body" to the back of the "head" of the comet on September 5, 2014. At full resolution, a pixel spans only 1.1 meters; the entire image is about 2.25 kilometers square.

The area of this image overlaps slightly with the area in the previous OSIRIS image. The previous OSIRIS release was a 3D one -- two photos taken from slightly different positions -- and that allowed amateur image processor Mattias Malmer to create a shape model of the comet. He used that high-resolution shape model to produce this synthetic 3D view of a part of the area covered by the OSIRIS image above. Grab your red-blue glasses and enjoy (or use one of the links below to see the 3D another way):

Synthetic 3D view of Churyumov-Gerasimenko from September 5, 2014 image

ESA / Rosetta / DLR / MPS for OSIRIS Team MPS / UPD / LAM / IAA / SSO / INTA / UPM / DASP / IDA / Mattias Malmer

Synthetic 3D view of Churyumov-Gerasimenko from September 5, 2014 image
Amateur image processor Mattias Malmer used an earlier OSIRIS 3D image to create a 3D model of the comet, onto which he draped the September 5 OSIRIS image to produce this synthetic 3D view.

Crossed-eye stereo

Parallel-eye stereo

Flicker gif

I was not at the European Planetary Science Congress meeting, but Pamela Gay was, and she was tweeting furiously. Here are some highlights of her tweets from the EPSC Rosetta session:

Finally, I'll leave you with the most recent NavCam view of the comet:

NavCam view of comet Churyumov-Gerasimenko on September 10, 2014

ESA / Rosetta / NavCam / Emily Lakdawalla

NavCam view of comet Churyumov-Gerasimenko on September 10, 2014
Four images taken by Rosetta's NavCam have been destriped and mosaicked to make this high-resolution view. Sunlight is reflecting off of the top of the comet's "body" and bouncing into the shadowed region of the comet's "head", weakly illuminating it. A strongly stretched version shows this region more clearly and also reveals diffuse material in the coma.
See other posts from September 2014


Or read more blog entries about: Rosetta and Philae, pretty pictures, comets, amateur image processing, comet Churyumov-Gerasimenko, spacecraft


AJA: 09/11/2014 06:27 CDT

Are there any hypotheses that describe how a relatively small, relatively cold cometary nucleus can acquire "layers, blocks and plates"?

morganism: 09/12/2014 02:15 CDT

so, imagine. original body dissassociation creates impactors along the same orbit, because micrograv impacts do create intersecting ejecta. These impactors later strike the main body, compressing the maternal clathrate to more robust material. Body, non-impacted, non-compressed material erodes first, outgassing easily, creating the "lily pad" shape, of the non-cratered, un-compressed ,and faster eroding , body material. Then the compressed impcrater body is exposed to more thermal shock, and the exposed crater "cup". starts to degrade, filling crater with fine debris, and dropping rocks , and lots of bigger materials to the negative angle exterior to the eroded craters. This gives you LOTS of depth on interior crater levels, (look at Hyperion. and imagine it sanded down), and only subject to re-surfacing events, will you find any redistribution and leveling. Don't land on smooth spots in craters, they will be parabolas, way to much loose electrostatic material , that will coat the body and solar panels instantaneously, and hider any attachment attempts. What you really want is recently exposed faults, or aim for a "cliff" that has a clear orbital insertion approach. Any "safe" , smooth landing site is likely a bed of carbon, prob 10s of meters deep, and not likely to provide any info on the body's compsition

lodaya: 09/12/2014 06:14 CDT

Re Pamela Gay's point: Need to predict effects before effects start. This is completely open-ended. Here are some thoughts, all questions and no answers, but I hope they help. One way is by observing the erosion or other sculpting effects we can see on the comet surface. Can we figure out what the power requirements of a jet which did that will be? Assuming Rosetta at a distance of 30 km (or whatever) how much perturbation would that cause? For an analogy on earth, how would a jet compare with a really small (and I suppose colder) volcano? A geyser? A gigantic blast furnace? What would be a reasonable estimate of the width of a jet? A hundred metres? A few hundreds? Suppose a jet starts up and it is feared that Rosetta will get in its path resulting in damage. How quickly can one respond and in what way can one move the craft to enter an orbit which avoids it? Suppose during this perihelion the Sun really gets to work on the ices inside the neck and dislocates the two lobes of the comet further from each other. How extreme can this be?

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