Rosetta bound for outer Solar System after final Earth swingby (w/ Video)

Rosetta
Artist view of ESA's Rosetta cometary probe. The spacecraft is covered with dark thermal insulation in order to keep its warmth while venturing into the coldness of the outer Solar System, beyond Mars orbit. Selected in November 1993 as a cornerstone mission of ESA's long-term science programme, the Rosetta probe was launched by an Ariane 5 on 2 March 2004, on an 11-year journey to the comet 67P/Churyumov-Gerasimenko.

(PhysOrg.com) -- This morning, mission controllers confirmed that ESA’s comet chaser Rosetta had swung by Earth at 8:45 CET as planned, skimming past our planet to pick up a gravitational boost for an epic journey to rendezvous with comet 67P/Churyumov-Gerasimenko in 2014.

Rosetta passed over the ocean, just South of the Indonesian island of Java, at exactly 08:45:40 CET, at a speed of 13.34 km/s with respect to an an of 2481 km. The swingby was pre-planned and fully automated, and the was in direct communication with Earth at the time, via the ESa New Norcia Station.

Cool animation showing today's swingby as seen from Rosetta. The second half of the animation shows what you see if you were sitting on board Rosetta and watching Earth approach and then recede. Credit: ESA

The successful swingby was confirmed at 09:05 CET when mission controllers re-established contact with Rosetta via ESA’s Maspalomas station in Spain. Although a detailed analyses is in progress, spacecraft operators have confirmed that the swingby provided a boost of 3.6 km/s.

Europe’s chaser has now flown a little over 4500 million km of its 7100 million km journey to its destination comet 67P/Churyumov-Gerasimenko. This was Rosetta’s fourth planetary swingby and the third and final swingby of Earth.

Science close to Earth

Some of Rosetta's instruments have been on since early November, performing imaging, magnetospheric, and atmospheric observations, as well as looking for water on the Moon. The first round of images and data recorded just before and during the swingby will be downloaded later today.

is now departing Earth to meet asteroid (21) Lutetia in July 2010. It has gained sufficient orbital energy to achieve its final goal: a rendezvous with comet 67P/Churyumov-Gerasimenko in 2014. The spacecraft is scheduled to enter deep-space hibernation by mid 2011 for the coldest leg of her journey to receive a wake up call only in spring 2014.

Rosetta darting across the night

During the night of 12/13 November, scientists working at ESA's Optical Ground Station in Tenerife, Spain, conducted observations to view Rosetta as the satellite approached Earth.

Rosetta darting across the night
Click image to view animation. Credits: ESA/ K.Wirth

The animation above comprises images recorded 13 November, 03:05 to 03:25. It comprises 18 images with an exposure time of 15 s and a separation of 69 s. The field is located in the constellation of Cetus and has a size of 10 x 10 arcmin. The telescope was tracking Rosetta so that the spacecraft appears as a dot in the centre of the image while the stars appear as stripes.

Provided by European Space Agency (news : web)

Citation: Rosetta bound for outer Solar System after final Earth swingby (w/ Video) (2009, November 13) retrieved 21 September 2024 from https://phys.org/news/2009-11-rosetta-bound-outer-solar-earth.html
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