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Marco Parigi

Citizen scientist spots changes on Rosetta's comet

Posted by Marco Parigi

27-02-2017 6:00 CST

Topics: citizen science, Rosetta and Philae, comets, comet Churyumov-Gerasimenko

Back in 2015, as Rosetta’s comet, 67P, was approaching perihelion, scientists noticed the surface changing before their eyes. These “very significant alterations,” according to the European Space Agency, were located in Imhotep, the smooth region on the comet’s large lobe.

One exciting aspect of the Rosetta mission was that on a comet, there was a high expectation that visible changes would occur during perihelion, which is the point in the orbit where the comet makes its closest approach to the Sun. How these changes relate to the processes theorised to happen on comets is still a work in progress. Many new papers are proposing various mechanisms, and data from the mission will be informing scientific results for years to come.

Thousands of Rosetta images are available from the European Space Agency. In March 2016, ESA put out a call for citizen scientists to help spot changes on the comet’s surface.

I like looking through comet images for changes, so I decided to contribute. It’s a wonderful way for non-scientists to get involved. The process has been very rewarding—as one becomes more and more familiar with features, changes start to jump out, and there are usually multiple images of the same area to help validate differences.

Here’s a change I discovered last year. Take a look at these two raw images. Can you spot the difference?

Comet 67P before...

ESA / Rosetta / NAVCAM

Comet 67P before...
Rosetta NAVCAM image ROS_CAM1_20150128T215001_P.png, captured on January 28, 2015.
...and after

ESA / Rosetta / NAVCAM

...and after
Rosetta NAVCAM image ROS_CAM1_20160501T105855_P.png, captured on May 1, 2016.

It’s tricky! The lighting and camera angles are slightly different. But if you look closely, you’ll notice this:

Can you spot the change?

ESA / Rosetta / NAVCAM

Can you spot the change?

Do you see it now? Part of the cliff has apparently collapsed during the interval between the two images.

With the help of fellow comet enthusiast Andrew Cooper, I concluded the time window for the cliff collapse can likely be narrowed to between February 18 and March 1, 2016. That means it happened after perihelion, with comet 67P outside the orbit of Mars—which is interesting, considering the most dramatic outbursts of activity occurred closer to the August 2015 perihelion.

What’s also interesting about this discovery is where it happened. The “top” of the cliff is located in a region called Anuket, and the “bottom” is in a region called Sobek. The cliff collapsed from Anuket into Sobek.

I became very familiar with this part of the comet due to my work on narrowing down the time of the collapse. In the September 2016 issue of the journal Astronomy and Astrophysics, a paper was released describing the different regions of the comet. Reading the through the paper, I noticed a discrepancy: the border between Anuket and Sobek was wrong. Here’s what the paper showed; can you see the cliff from above, contained entirely within the Anuket region?

Southern hemisphere of Comet 67P

From M.R. El-Maarry et al. (2016)

Southern hemisphere of Comet 67P
Regional surface morphology of comet 67P/Churyumov-Gerasimenko from Rosetta/OSIRIS images: The southern hemisphere (before erratum).

I described the mapping discrepancy in the comments section of ESA's original article asking for citizen scientist contributions. The paper’s lead author, Ramy El-Maarry, replied to say I was correct, and an erratum was issued correcting the boundaries.

Here is the upgraded diagram from the paper’s erratum, which was published in February 2017. Notice how the boundary between Anuket and Sobek now runs along the bottom of the region where the cliff collapsed:

Southern hemisphere of Comet 67P (corrected)

From M.R. El-Maarry et al. (2016)

Southern hemisphere of Comet 67P (corrected)
Regional surface morphology of comet 67P/Churyumov-Gerasimenko from Rosetta/OSIRIS images: The southern hemisphere (after erratum).

The front page of the erratum paper acknowledges me and Andrew Cooper for having spotted the inconsistencies. Not bad for a couple citizen scientists! I believe it is a wonderful idea for ESA to make spacecraft data available to the public, and allow everyone to contribute to the mission.

 
See other posts from February 2017

 

Or read more blog entries about: citizen science, Rosetta and Philae, comets, comet Churyumov-Gerasimenko

Comments:

Gerald: 02/28/2017 05:56 CST

Hi Marco, congratulations, that your continued efforts -- and those of A.Cooper, of course -- now lasting for years, finally pay!

Marco: 02/28/2017 09:15 CST

Hi again Gerald, I was afraid that perhaps we may never have the chance to continue discussions again :-) This is of course the same change that you made a morph of and that we discussed endlessly the detail and ramifications. Since then is when I narrowed the timing down. Still waiting for OSIRIS to release their images from February 2016 :-(

a.cooper : 02/28/2017 10:46 CST

Hi Gerald, nice to hear from you again, and thanks for your support. We miss your informed opinion since the ESA Rosetta blog closed the comments. I'm sure Marco would welcome a visit to his site. We could resume our two-year-long debate on cometary theory, 67P's morphological evolution and its implications for the protoplanetary disk.

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