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What is comet dust made of? Rosetta finds out.

The European Space Agency's Rosetta spacecraft, currently in orbit around Comet 67P/Churyumov鈥揋erasimenko, is examining the dust being shed by the comet as it hurtles toward the sun.

Rosetta's NAVCAM view of Comet 67P/Churyumov鈥揋erasimenko on 12 Jan 2015.

ESA/Rosetta/NAVCAM 鈥 CC BY-SA IGO 3.0

January 26, 2015

Sen鈥擡ven before the Philae probe landed on comet 67P/Churyumov鈥揋erasimenko in November, to international acclaim, Europe's Rosetta spacecraft that carried it was already studying the dust being shed by it.

Between August and October 2014鈥攂efore Philae's famous 12 November landing鈥擱osetta was orbiting the four km-wide comet at a distance of 30 km. Dust emanating from the comet due to solar radiation (there's no air to blow particles around) effectively "blew" into Rosetta's eyes. But this was a good thing.

Scientists observed the dust disintegrating on impact with an instrument sensor. This told them that the dust grains weren't bound together well, and that there was also no ice present.

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These were dry, "fluffy" grains鈥攚hich should be unusual as comets are typically composed of up to 50-per cent water ice. But scientists found the grains were instead made of sodium, which is a major constituent of interplanetary dust.

The comet has an orbital period of 6.5 years. As it nears perihelion (closest approach to the Sun) in August 2015, it will warm up and the vapour from evaporating water-ice will lift the dry dust into the coma that surrounds all comets that approach the Sun.

Eventually, there will be enough solar energy to remove all the old dust altogether鈥攄ust which the Philae lander found could be up to 20cm thick.

Dr Martin Hilchenbach of the Max Planck Institute said in a statement: 鈥淲e believe that these fluffy grains collected by Rosetta originated from the dusty layer that built up on the comet鈥檚 surface since its last close approach to the Sun.鈥

Hilchenbach is Principle Investigator of the COSIMA instrument (COmetary Secondary Ion Mass Analyser) on-board Rosetta that studied the dust. He expects to see more ice-rich debris again in the months to come.聽

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In fact on Thursday NASA reported a "significant increase" in the amount of water that 67P/Churyumov鈥揋erasimenko is releasing (about 1.2 litres in vapour form). Once it passes perihelion and speeds away from the Sun again, it should cool down, its watery coma should recede, and it will start to pick up fine interplanetary dust once again.聽

Rosetta is a European Space Agency mission and was launched in 2004 to answer questions about comets, because they may hold clues about the formation of our聽Solar System.

In December 2014, it discovered that 67P/Churyumov鈥揋erasimenko has three-times more of a heavy version of hydrogen in its water than Earth's oceans do. Comets are thought to be the origins of Earth's water, so聽this discovery cast doubt on that.聽

The results of the new dust聽analysis appear in the journal Nature.

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