Australian Sky & Telescope — July 2017

(Wang) #1
http://www.skyandtelescope.com.au 25

SOURCE: ESA / ROSETTA / NAVCAM & OSIRIS TEAMS


its full instrument suite for more than two years, sometimes
getting as close to the surface as about 7 km early in the mission
— and down to 2 km during its end-of-mission orbits. Yet at
times the spacecraft had to stand off at distances of 300 to
400 km or more because the comet became so active that the
resulting blizzard of dust blinded Rosetta’s star trackers. Two
distant excursions, 1,000 to 1,500 km away, enabled studies of
the comet’s tail and its interaction with the solar wind.
Why go to all this trouble and expense? Because we were
seeking some fundamental understanding about comets,
which are made from the primitive materials present
during the formation of the Solar System. So by studying
one up close, we stood to learn about the conditions and
constituents that formed the Sun’s planets.
Since comets spend most of their time in the distant Kuiper

Belt or Oort Cloud — very difficult or impossible to study
with spacecraft — we observe the ones that venture inward as
escaped examples of those regions of the Solar System. And
because comets sometimes also hit the inner planets (including
Earth) and deliver water, other volatiles and organics, studying
them up close can tell us how they might have influenced
conditions here, including those important to the origin of life.
First and foremost, how do we explain the dramatic shape
of Rosetta’s target? Two-lobed objects do exist among small
bodies like asteroids and comets, and in fact three of the
five other comets imaged by flyby missions have this general
shape. But Comet 67P is a wonderfully extreme example.
There are two main possibilities: Either two objects slowly
collided and stuck together, or the neck region preferentially
eroded due to an abundance of volatile ices there that escaped

20 m

Rosetta’s
shadow

March–July 2015
Increasing comet activity February 24, 2015
Close encounter

November 12, 2014
Philae lands on nucleus

October 7, 2014
“Selfie” while orbiting close to comet

August 6, 2014
Orbiting close to comet

July 14, 2014
Shape of nucleus revealed
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