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EarthSky // Science Wire, Space Release Date: May 15, 2014

Rosetta’s target comet is getting active

The target of ESA’s Rosetta mission has started to reveal its true personality as a comet, its dusty veil clearly developing over the last six weeks.

Rosetta-comet

Between March 27th and May 4th, Rosetta approached comet 67P/Churyumov-Gerasimenko from a distance of around 5 million to 2 million kilometers. This sequence of images shows the comet’s movement against the background star field during this time. Rosetta (and the comet) are between 640 and 610 million km from the sun. The comet is seen to develop a dust coma as the sequence progresses, with clear activity already visible in late-April. Image credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

Rosetta is on a 10-year mission to study Comet 67P/Churyumov-Gerasimenko up close as the comet enters the solar system. The spacecraft woke up from hibernation in January and will enter orbit around the comet in August. If all goes well, it will be the first spacecraft to orbit a comet’s nucleus and the first lander to do a controlled touchdown, in November, on the surface of a comet. The comet is just a few kilometers across.

The sequence of images presented here of comet 67P/Churyumov–Gerasimenko were taken between 27 March and 4 May, as the gap between craft and comet closed from around 5 million km to 2 million km.

By the end of the sequence, the comet’s dusty veil – the ‘coma’ – extends some 1300 km into space. By comparison, the nucleus is roughly only 4 km across, and cannot yet be ‘resolved’.

The coma has developed as a result of the comet moving progressively closer to the sun along its 6.5 year orbit. Even though it is still more than 600 million km from the sun – more than four times the distance between Earth and sun – its surface has already started to warm, causing its surface ices to sublimate and gas to escape from its rock–ice nucleus.

As the gas escapes, it also carries a cloud of tiny dust particles out into space, which slowly expands to create the coma.

As the comet continues to move closer to the Sun, the warming continues and activity rises, and pressure from the solar wind will eventually cause some of the material to stream out into a long tail.

Rosetta and the comet will be closest to the Sun in August 2015, between the orbits of Earth and Mars.

The onset of activity now offers scientists the opportunity to study dust production and structures within the coma before getting much closer.

“It’s beginning to look like a real comet,” says Holger Sierks, principal investigator for OSIRIS, the Optical, Spectroscopic and Infrared Remote Imaging System, at the Max Planck Institute for Solar System Research, Germany.

“It’s hard to believe that only a few months from now, Rosetta will be deep inside this cloud of dust and en route to the origin of the comet’s activity.”

In addition, tracking the periodic changes in brightness reveals the nucleus is rotating every 12.4 hours – about 20 minutes shorter than previously thought.

“These early observations are helping us to develop models of the comet that will be essential to help us navigate around it once we get closer,” says Sylvain Lodiot, ESA Rosetta spacecraft operations manager.

OSIRIS and the spacecraft’s dedicated navigation cameras have been regularly acquiring images to help determine Rosetta’s exact trajectory relative to the comet. Using this information, the spacecraft has already started a series of manoeuvres that will slowly bring it in line with the comet before making its rendezvous in the first week of August.

Detailed scientific observations will then help to find the best location on the comet for the Philae lander’s descent to the surface in November.

Via ESA