On 13 August, Comet 67P/Churyumov-Gerasimenko reaches its closest point
to the Sun (perihelion) and the Rosetta orbiter will be there to see
exactly what happens. Rosetta will continue monitoring the comet’s activity until the extended
mission ends, in September 2016, to increase our understanding of how a
comet changes during its orbit and as it approaches and moves away from
the Sun.
This film includes some of the most recent science
findings about the comet including those from the CONSERT, CIVA, ROLIS,
PTOLEMY and COSAC instruments. It covers the comet’s high porosity and
the detection of multiple organic compounds. Some of these compounds are
key ingredients for life and four compounds have never been found
before on a comet until now.
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