New Images and 3D Model of Comet 67P

New Views of the Rosetta Comet

Images of comet 67P/Churyumov-Gerasimenko taken on July 14, 2014, by the OSIRIS imaging system aboard the European Space Agency’s Rosetta spacecraft have allowed scientists to create this three-dimensional shape model of the nucleus. Credit: ESA/Rosetta/MPS for OSIRIS Team/MPS/UPD/LAM/IAA/SSO/INTA/UPM

New images from ESA’s Rosetta spacecraft reveal surface structures of comet 67P/Churyumov-Gerasimenko, allowing scientists to create a 3D shape model of the nucleus.

As the European Space Agency’s Rosetta probe approaches Comet 67P/Churyumov-Gerasimenko (67P) for an August rendezvous, the comet’s core is coming into sharper focus. Today, ESA released a new set of images and a striking 3D model of 67P’s nucleus.

The resolution of the latest images taken by the spacecraft’s OSIRIS imaging system on July 20th is 330 feet (100 meters) per pixel. At that resolution, 67P appears to consist of two parts: a smaller head connected to a larger body. The connecting region, the neck, is proving to be especially intriguing.

“The only thing we know for sure at this point is that this neck region appears brighter compared to the head and body of the nucleus,” says OSIRIS Principal Investigator Holger Sierks from the Max Planck Institute for Solar System Research in Germany. This collar-like appearance could be caused by differences in material or grain size, or could be a topographical effect–no one knows.

Surface Impressions of Rosetta Comet

Comet 67P/Churyumov-Gerasimenko was imaged by the European Space Agency’s Rosetta spacecraft on July 20, 2014, from a distance of approximately 3,400 miles (5,500 kilometers). These three images were taken two hours apart. Credit: ESA/Rosetta/MPS for OSIRIS Team/MPS/UPD/LAM/IAA/SSO/INTA/UPM

The appearance of 67P reminds mission scientists of comet 103P/Hartley, which was visited in a flyby by NASA’s EPOXI mission in 2010. While Hartley’s ends show a rather rough surface, its middle is much smoother. Scientists believe this waist to be a “gravitational low.” Because it contains the body’s center of mass, material kicked up by, say, meteoroid impacts, that cannot leave the comet’s gravitational field is most likely to be re-deposited there.

Whether this also holds true for 67P’s neck region is still unclear. Another explanation for the high reflectivity could be a different surface composition. In the coming weeks, the OSIRIS team hopes to analyze the spectral data of this region obtained with the help of the imaging system’s filters. These can select several wavelength regions from the reflected light, allowing scientists to identify the fingerprints of certain materials and compositional features.

Rosetta will be the first mission in history to rendezvous with a comet, escort it as it orbits the sun, and deploy a lander to its surface. ESA says the next high-resolution OSIRIS image will be published on July 31st. Stay tuned!

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