3D view of Philae’s descent to comet

JPL Image Release

This 3D image shows what it would look like to fly 2 miles (3 km) above the surface of comet 67P/Churyumov-Gerasimenko. The image was generated by data collected by the ROLIS instrument aboard the European Space Agency's Philae spacecraft during the decent to the spacecraft's 12th November initial touchdown on the comet. Image Credit: ESA/Rosetta/Philae/ROLIS/DLR
This 3D image shows what it would look like to fly 2 miles (3 km) above the surface of comet 67P/Churyumov-Gerasimenko. Image Credit: ESA/Rosetta/Philae/ROLIS/DLR

The 3D image was generated from data collected by the Rosetta Lander Imaging System (ROLIS) aboard the European Space Agency’s Philae spacecraft during the descent to the spacecraft’s initial 12th November touchdown on the comet. The European Space Agency also released an audio track of the first of the lander’s three touchdowns on the surface of the comet.

The stereographic image was generated using two images acquired by ROLIS when Philae was a little less than 2 miles (3 kilometers) from the surface. The images were taken two minutes apart – about one hour prior to the spacecraft’s initial touchdown on 67P at 8:03 a.m. PST (11:03 a.m. EST). In the image, the landing site Agilkia can be seen immediately below. In the top right of the field of view, one of the landing gear feet can be seen. The resolution is about 10 feet (3 meters) per pixel. To appreciate the 3D effect, the image must be viewed with red-blue glasses.

At the time Philae made its first touchdown on the comet, a short but significant “thud” was heard by Philae’s Cometary Acoustic Surface Sounding Experiment (CASSE) as the spacecraft made its first touchdown. The two-second recording from space is the very first of the contact between a man-made object with a comet upon landing. The CASSE sensors are located in the feet at the base of all three legs of the lander.

“The Philae lander came into contact with a soft layer several centimetres thick,” said Klaus Seidensticker, lead scientist for the CASSE instrument from the German Aerospace Center’s Institute of Planetary Research, Berlin. “Then, just milliseconds later, the feet encountered a hard, perhaps icy layer on 67P/Churyumov-Gerasimenko.”

Comets are time capsules containing primitive material left over from the epoch when our Sun and its planets formed. Rosetta will be the first spacecraft to witness at close proximity how a comet changes as it is subjected to the increasing intensity of the sun’s radiation. Observations will help scientists learn more about the origin and evolution of our Solar System and the role comets may have played in seeding Earth with water, and perhaps even life.

Rosetta is an ESA mission with contributions from its member states and NASA. Rosetta’s Philae lander is provided by a consortium led by the German Aerospace Center, Cologne; Max Planck Institute for Solar System Research, Gottingen; French National Space Agency, Paris; and the Italian Space Agency, Rome. ROLIS and CASSE were developed by the German Aerospace Center’s Institute of Planetary Research in Berlin. NASA’s Jet Propulsion Laboratory, Pasadena, California, a Division of the California Institute of Technology in Pasadena, manages the U.S. contribution of the Rosetta mission for NASA’s Science Mission Directorate in Washington. JPL also built the MIRO instrument and hosts its principal investigator, Samuel Gulkis. The Southwest Research Institute (San Antonio and Boulder), developed the Rosetta orbiter’s IES and Alice instruments, and hosts their principal investigators, James Burch (IES) and Alan Stern (Alice).

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