Science matters. Wonder matters. You matter.<\/strong> On October 15, 2025, astronomers said that \u2013 for the first time \u2013 they\u2019ve detected the presence of heavy water in the planet-forming disk of a young star. Specifically, radio telescope observations of the star V883 Ori show heavy water in its protoplanetary disk. The water formed when molecular clouds collapsed to create that star. The results indicate that water in planetary systems can be older than the star around which it formed.<\/p>\n Plus, our own solar system once looked similar to V883 Ori, 4.5 billion years ago. Therefore, it\u2019s likely that some of the life-giving water around us is even older than the sun.<\/p>\n Margot Leemker of the University of Milan is the lead author of the paper that presented these new findings. She said:<\/p>\n Our detection indisputably demonstrates that the water seen in this planet-forming disk must be older than the central star and formed at the earliest stages of star and planet formation.<\/p>\n This presents a major breakthrough in understanding the journey of water through planet formation, and how this water made its way to our solar system, and possibly Earth, through similar processes.<\/p>\n<\/blockquote>\n The researchers published their study in the peer-reviewed journal Nature Astronomy<\/em> on October 15, 2025.<\/p>\n Water is a molecule made of one oxygen atom and two hydrogen atoms. Most hydrogen atoms, created during the Big Bang, consist of a proton and electron. In addition, the Big Bang also created very small amounts of deuterium. This is a form of hydrogen that has a proton, electron and neutron.<\/p>\n Heavy water is chemically described as D2<\/sub>O. That means each molecule of heavy water is made of two deuterium (D) atoms and one oxygen (O) atom. In our solar system, heavy water is mixed in with regular water in very small quantities. Here on Earth, roughly one out of every 41 million water molecules is heavy water.<\/p>\n Astronomers have long been fascinated by how water is created in our universe. How did it form? How old is it? Did water in our solar system originate in molecular clouds before the sun existed? Or was the water destroyed and recreated during the planet-forming phase of our solar system?<\/p>\n Molecular clouds in space consist of gases and dust grains. Hydrogen is the most abundant gas, created during the Big Bang. Other gases in these clouds include oxygen and carbon monoxide. There are also dust particles suspended in the clouds, mostly silicate and carbon grains. Long-dead stars that ended as planetary nebulae or supernovae formed these heavier gases and dust.<\/p>\n Under certain conditions in these frigid molecular clouds, water forms when oxygen atoms on grains of dust capture hydrogen atoms. As a result, the water is frozen onto the dust grains.<\/p>\n If a molecular cloud is massive enough, gravity will cause it to collapse to form a protostar. That\u2019s a very young star still gathering mass from its surrounding cloud. This process generates a lot of heat. As a result, some of the frozen water near the protostar converts to a gaseous form. However, the water in other regions of the dust cloud remain frozen.<\/p>\n The spinning motion of the protostar and surrounding cloud eventually forms a protoplanetary disk of gas and dust. As the system evolves, bodies such as planets coalesce in the disk. In addition, comets and asteroids from the disk\u2019s cold outer fringes carry more water into the inner regions. Moreover, some may impact planets, adding to their water content. <\/p>\n The Big Bang did not create high levels of deuterium. It created deuterium at only 27 parts per million relative to regular hydrogen. Therefore, one would expect naturally occurring heavy water in the universe to be just as scarce.<\/p>\n However, that\u2019s not the case. Complex chemical processes in the frigid molecular clouds result in more deuterium atoms landing on dust grains to combine with oxygen to create heavy water ice. As a result, the molecular clouds have a higher-than-expected ratio of heavy water to ordinary water, compared to the deuterium-hydrogen ratio in the universe. <\/p>\n The astronomers used the Atacama Large Millimeter\/Submillimeter Array (ALMA) to measure the ratio of heavy water to ordinary water in the V883 Ori planet-forming disk. And they found it to be similar to the ratio in star-forming molecular clouds. The heavy water acts as a tracer, showing that some water in the V883 Ori disk originated from the molecular cloud that created the star. If that\u2019s the case, the same could also be true for our solar system.<\/p>\n Paper co-author John Tobin of the National Radio Astronomy Observatory said:<\/p>\n Until now, we weren\u2019t sure if most of the water in comets and planets formed fresh in young disks like V883 Ori, or if it\u2019s \u2018pristine,\u2019 originating from ancient interstellar clouds. <\/p>\n The detection of heavy water, using sensitive isotopologue ratios (D2<\/sub>O\/H2<\/sub>O), proves the water\u2019s ancient heritage and provides a missing link between clouds, disks, comets and ultimately planets. This finding is the first direct evidence of water\u2019s interstellar journey from clouds to the materials that form planetary systems, unchanged and intact.<\/p>\n<\/blockquote>\n Bottom line: Astronomers found ancient water in the planet-forming disk of a young star. This heavy water formed in molecular clouds before the star was born.<\/p>\n Source: Pristine ices in a planet-forming disk revealed by heavy water<\/p>\n Via National Radio Astronomy Observatory<\/p>\n Via European Southern Observatory<\/p>\n <\/div>\n
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Ancient water in a protoplanetary disk and what that means for us<\/h3>\n
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What is heavy water?<\/h3>\n
From molecular clouds to protoplanetary disks<\/h3>\n
Ancient water in V883 Ori<\/h3>\n
Finding ancient water in the planet-forming disk<\/h3>\n
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