Rosetta provides evidence for daily water-ice cycle on comets

ESA’s spacecraft finds an important piece of information about comets from 67P

The Rosetta spacecraft arrived at Comet 67P on 6 August 2014. Image Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

The Rosetta spacecraft arrived at Comet 67P on 6 August 2014. Image Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

The Rosetta spacecraft’s Visible, InfraRed and Thermal Imaging Spectrometer (VIRTIS) has identified a region on Comet 67P/Churyumov-Gerasimenko’s surface where water ice appears and disappears in sync with its rotation period.

“We found a mechanism that replenishes the surface of the comet with fresh ice at every rotation: this keeps the comet ‘alive,’” says lead scientist Maria Cristina De Sanctis from INAF-IAPS in Rome, Italy.

Comets are celestial bodies comprising a mixture of dust and ices, which they periodically shed as they swing towards their closest point to the Sun along their highly eccentric orbits. As sunlight heats the frozen nucleus of a comet, the ice in it – mainly water but also other ‘volatiles’ such as carbon monoxide and carbon dioxide – transforms directly into a gas. This gas flows away from the comet, carrying dust particles along and, together, the gas and dust build up the bright halo and tails that are characteristic of comets.

A key feature that Rosetta’s scientists are investigating is the way in which activity on the comet and the associated outgassing are driven, by monitoring the increasing activity on and around the comet since Rosetta’s arrival. The team studied a set of data taken in September 2014, concentrating on a one square kilometres region on the comet’s neck. At the time, the comet was about 500 million kilometres (310 million miles) from the Sun and the neck was one of the most active areas.

As the comet rotates, taking just over 12 hours to complete a full revolution, the various regions undergo different illumination. “We saw the telltale signature of water ice in the spectra of the study region but only when certain portions were cast in shadow,” says Cristina. “Conversely, when the Sun was shining on these regions, the ice was gone. This indicates a cyclical behaviour of water ice during each comet rotation.”

The data from Rosetta suggest that water ice on and a few centimetres below the surface ‘sublimates’ when illuminated by sunlight, turning it into gas that then flows away from the comet. Then, as 67P rotates and the same region falls into darkness, the surface rapidly cools again.

Water-ice cycle on Comet 67P. image Credit: ESA

Water-ice cycle on Comet 67P. image Credit: ESA

However, the underlying layers remain warm owing to the sunlight they received in the previous hours, and, as a result, subsurface water ice keeps sublimating and finding its way to the surface through the comet’s porous interior. But as soon as this ‘underground’ water vapour reaches the cold surface, it freezes again, blanketing that patch of comet surface with a thin layer of fresh ice.

Eventually, as the Sun rises again over this part of the surface on the next comet day, the molecules in the newly formed ice layer are the first to sublimate and flow away from the comet, restarting the cycle.

“We suspected such a water ice cycle might be at play at comets, on the basis of theoretical models and previous observations of other comets but now, thanks to Rosetta’s extensive monitoring at Comet 67P, we finally have observational proof,” says Fabrizio Capaccioni, VIRTIS principal investigator also based at INAF-IAPS.

From the data, it is possible to estimate the relative abundance of water ice with respect to other material. Down to a few centimetres deep over the portion of the comet nucleus that was surveyed, water ice accounts for ten to 15 per cent of the material and appears to be well-mixed with the other constituents.

The scientists also calculated how much water vapour was being emitted by the patch that they analysed with VIRTIS, and showed that this accounted for about three per cent of the total amount of water vapour coming out from the whole comet at the same time, as measured by Rosetta’s microwave sensor. “It is possible that many patches across the surface were undergoing the same diurnal cycle, thus providing additional contributions to the overall outgassing of the comet,” adds Capaccioni.

The scientists are now busy analysing VIRTIS data collected in the following months, as the comet’s activity increased around the closest approach to the Sun.

“These initial results give us a glimpse of what is happening underneath the surface, in the comet’s interior,” says Matt Taylor, Project Scientist of the Rosetta spacecraft. “Rosetta is capable of tracking changes on the comet over short as well as longer time scales, and we are looking forward to combining all of this information to understand the evolution of this and other comets.”

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