The four images that make up this montage of comet 67P/Churyumov–Gerasimenko were taken on Sept. 26, 2014 by the European Space Agency’s Rosetta spacecraft. At the time, Rosetta was about 16 miles (26 kilometers), from the center of the comet. In the montage, a region of jet activity can be seen at the neck of the comet. These jets, originating from several discrete locations, are a product of ices sublimating and gases escaping from inside the nucleus.
This is no computer-generated shape model, this is the real deal: the double-lobed nucleus of Comet 67P/C-G, as imaged by Rosetta’s OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) narrow-angle camera on Tuesday, July 29. At the time just about a week away from making its arrival, ESA’s spacecraft was 1,950 km (1,211 miles) from the comet when this image was taken (that’s about the distance between Providence, Rhode Island and Miami, Florida)
The Rosetta navigation camera sent back this image of Comet 67P/Churyumov-Gerasimenko on Aug. 23, showing about a quarter of the four-kilometer (2.5-mile) comet. This image was acquired from a distance of 61 kilometers (38 miles). Credit: ESA/Rosetta/NAVCAM