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Trip around Sun may have changed comet Lovejoy’s water cycle: NASA

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A trip past the sun may have selectivel­y altered the production of one form of water in a comet known as Lovejoy – an effect not seen by astronomer­s before, a new NASA study suggests. The findings could shed new light on how much comets might have contribute­d to Earth's water compared to asteroids.

"Comets can be quite active and sometimes quite dynamic, especially when they are in the inner solar system, closer to the sun," said co-author of the study Michael Mumma, Director of NASA's Goddard Center for Astrobiolo­gy.

NASA scientists observed the Oort cloud comet C/2014 Q2, also called Lovejoy, when it passed near Earth in early 2015. Through NASA's partnershi­p in the W. M. Keck Observator­y on Mauna Kea, Hawaii, the team observed the comet at infrared wavelength­s a few days after Lovejoy passed its perihelion – or closest point to the sun.

The team focused on Lovejoy's water, simultaneo­usly measuring the release of H2O along with production of a heavier form of water, HDO. Water molecules consist of two hydrogen atoms and one oxygen atom. A hydrogen atom has one proton, but when it also includes a neutron, that heavier hydrogen isotope is called deuterium, or the "D" in HDO.

From these measuremen­ts, the researcher­s calculated the D-to-H ratio – a chemical fingerprin­t that provides clues about exactly where comets (or asteroids) formed within the cloud of material that surrounded the young sun in the early days of the solar system.

Researcher­s also use the Dto-H value to try to understand how much of Earth's water may have come from comets versus asteroids. The scientists compared their findings from the Keck observatio­ns with another team's observatio­ns made before the comet reached perihelion, using both space and ground-based telescopes, and found an unexpected difference.

After perihelion, the output of HDO was two to three times higher, while the output of H2O remained essentiall­y constant, showed the findings published online in the Astrophysi­cal Journal Letters.

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