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"Our water-soaked world, teeming with life and unique in the universe as far as we know, is something of a mystery - we're not sure how all this water got here," said Stefanie Milam, Webb Deputy Project Scientist for Planetary Science and a co-author on the study reporting the finding. "Understanding the history of water distribution in the Solar System will help us to understand other planetary systems, and if they could be on their way to hosting an Earth-like planet," she added.
Comet Read is a main-belt comet - an object that resides in the main asteroid belt but which periodically displays a halo, or coma, and tail like a comet. Main-belt comets themselves are a fairly new classification, and Comet Read was one of the original three comets used to establish the category. Before that, comets were understood to originate in the Kuiper Belt and Oort Cloud, beyond the orbit of Neptune, where their ices could be preserved farther from the Sun. Frozen material that vaporises as they approach the Sun is what gives comets their distinctive coma and streaming tail, differentiating them from asteroids. Scientists have long speculated that water ice could be preserved in the warmer asteroid belt, inside the orbit of Jupiter, but definitive proof was elusive - until Webb.
"In the past we've seen objects in the main-belt with all the characteristics of comets, but only with this precise spectral data from Webb can we say yes, it's definitely water ice that is creating that effect," explained astronomer Michael Kelley of the University of Maryland, lead author of the study.
"With Webb's observations of Comet Read, we can now demonstrate that water ice from the early Solar System can be preserved in the asteroid belt," Kelley said.
The missing carbon dioxide was a bigger surprise. Typically carbon dioxide makes up about 10 percent of the volatile material in a comet that can be easily vapourised by the Sun's heat. The science team presents two possible explanations for the lack of carbon dioxide. One possibility is that Comet Read did have carbon dioxide when it formed, but has lost that because of warm temperatures.
"Being in the asteroid-belt for a long time could do it - carbon dioxide vaporises more easily than water ice, and could percolate out over billions of years," Kelley said. Alternatively, he said, Comet Read may have formed in a particularly warm pocket of the Solar System, where no carbon dioxide was available.
The next step is taking the research beyond Comet Read to see how other main-belt comets compare, says astronomer Heidi Hammel of the Association of Universities for Research in Astronomy (AURA), lead for Webb's Guaranteed Time Observations for Solar System objects and co-author of the study. "These objects in the asteroid belt are small and faint, and with Webb we can finally see what is going on with them and draw some conclusions. Do other main-belt comets also lack carbon dioxide? Either way it will be exciting to find out," Hammel said.
Co-author Milam imagines the possibilities of bringing the research even closer to home. "Now that Webb has confirmed there is water preserved as close as the asteroid belt, it would be fascinating to follow up on this discovery with a sample collection mission, and learn what else the main-belt comets can tell us."
Research Report:Spectroscopic identification of water emission from a main-belt comet
Related Links
James Webb Space Telescope
Asteroid and Comet Mission News, Science and Technology
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