Museum Blog

How Rosetta’s Comet Got Its Shape

Posted 9/29/2015 12:09 AM by Kim Evans | Comments

 Rosetta_s_comet_node - large.jpg

Two comets collided at low speed in the early Solar System to give rise to the distinctive ‘rubber duck’ shape of Comet 67P/Churyumov–Gerasimenko, say Rosetta scientists.

The origin of the comet’s double-lobed form has been a key question since Rosetta first revealed its surprising shape in July 2014.

Two leading ideas emerged: did two comets merge or did localized erosion of a single object form the ‘neck’?

Now, scientists have an unambiguous answer to the conundrum. By using high-resolution images taken between 6 August 2014 and 17 March 2015 to study the layers of material seen all over the nucleus, they have shown that the shape arose from a low-speed collision between two fully fledged, separately formed comets.

“It is clear from the images that both lobes have an outer envelope of material organized in distinct layers, and we think these extend for several hundred meters below the surface,” says Matteo Massironi, lead author from the University of Padova, Italy, and an associate scientist of the OSIRIS team.

“You can imagine the layering a bit like an onion, except in this case we are considering two separate onions of differing size that have grown independently before fusing together.”

The results of the study are reported in the journal Nature and were presented September 28th at the European Planetary Science Congress in Nantes, France.

To reach their conclusion, Matteo and his colleagues first used images to identify over 100 terraces seen on the surface of the comet, and parallel layers of material clearly seen in exposed cliff walls and pits. A 3D shape model was then used to determine the directions in which they were sloping and to visualize how they extend into the subsurface.

It soon became clear that the features were coherently oriented all around the comet’s lobes and in some places extended to a depth of about 650 m.

“To be sure, we also looked at the relationship between the local gravity and the orientations of the individual features all around the reconstructed comet surface.”

The team found that orientation of a given layer and the direction of the local gravity are closer to perpendicular in the model with two separate objects, rather than in the one with a single combined nucleus.

Finally, the team notes that even though erosion is not the root cause of the comet’s double-lobed shape, it nevertheless does play an important role in the comet’s evolution today.

Local variations seen in the structure of the surface likely result from different rates of sublimation – when ice turns directly into a gas – of frozen gases embedded within the individual layers, which are not necessarily distributed evenly throughout the comet.

“How the comet got its curious shape has been a major question since we first saw it. Now, thanks to this detailed study, we can say with certainty that it is a ‘contact binary’,” says Holger Sierks, OSIRIS (Optical, Spectroscopic and Infrared Remote Imaging System) principal investigator at the Max Planck Institute for Solar System Research in Göttingen.

Source: ESA




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