ALMA Traces The History Of Water In Planet Formation Back To The Interstellar Medium
Scientists studying a nearby protostar have detected the presence of water in its circumstellar disk. The new observations made with the Atacama Large Millimeter/submillimeter Array (ALMA) mark the first detection of water being inherited into a protoplanetary disk without significant changes to its composition. These results further suggest that the water in our Solar System formed billions of years before the Sun. The new observations are published today in Nature.
V883 Orionis is a protostar located roughly 1,305 light-years from Earth in the constellation Orion. The new observations of this protostar have helped scientists to find a probable link between the water in the interstellar medium and the water in our Solar System by confirming they have similar composition.
V883 Ori is the link to understanding water in our Solar System from NRAO Outreach on Vimeo.
Most of the time, water in the circumstellar disks surrounding protostars is in the form of ice, sometimes extending out long distances from the star. In the case of V883 Ori, the snowline extends 80 au from the star; that’s 80 times the distance between Earth and the Sun, as shown in this animation. But, the temperature at V883 Ori is just hot enough that much of the ice in its disk has turned to gas, making it possible for radio astronomers to study that water in detail. New observations with the Atacama Large Millimeter/submillimeter Array (ALMA) have revealed that the water in V883 Ori’s disk is of the same basic composition as water on objects in our Solar System. This suggests that the water in our own Solar System formed billions of years before the Sun in the interstellar medium. Credit: ALMA (ESO/NAOJ/NRAO), J. Tobin, B.Saxton (NRAO/AUI/NSF)
“We can think of the path of water through the Universe as a trail. We know what the endpoints look like, which are water on planets and in comets, but we wanted to trace that trail back to the origins of water,” said John Tobin, an astronomer at the National Science Foundation’s National Radio Astronomy Observatory (NRAO) and the lead author on the new paper. “Before now, we could link the Earth to comets, and protostars to the interstellar medium, but we couldn’t link protostars to comets. V883 Ori has changed that, and proven the water molecules in that system and in our Solar System have a similar ratio of deuterium and hydrogen.”
Observing water in the circumstellar disks around protostars is difficult because in most systems water is present in the form of ice. When scientists observe protostars they’re looking for the water snow line or ice line, which is the place where water transitions from predominantly ice to gas, which radio astronomy can observe in detail. “If the snow line is located too close to the star, there isn’t enough gaseous water to be easily detectable and the dusty disk may block out a lot of the water emission. But if the snow line is located further from the star, there is sufficient gaseous water to be detectable, and that’s the case with V883 Ori,” said Tobin, who added that the unique state of the protostar is what made this project possible
V883 Ori’s disk is quite massive and is just hot enough that the water in it has turned from ice to gas. That makes this protostar an ideal target for studying the growth and evolution of solar systems at radio wavelengths.
“This observation highlights the superb capabilities of the ALMA instrument in helping astronomers study something vitally important for life on Earth: water,” said Joe Pesce, NSF Program Officer for ALMA. “An understanding of the underlying processes important for us on Earth, seen in more distant regions of the galaxy, also benefits our knowledge of how nature works in general, and the processes that had to occur for our Solar System to develop into what we know today.”
To connect the water in V883 Ori’s protoplanetary disk to that in our own Solar System, the team measured its composition using ALMA’s highly sensitive Band 5 (1.6mm) and Band 6 (1.3mm) receivers and found that it remains relatively unchanged between each stage of solar system formation: protostar, protoplanetary disk, and comets. “This means that the water in our Solar System was formed long before the Sun, planets, and comets formed. We already knew that there is plenty of water ice in the interstellar medium. Our results show that this water got directly incorporated into the Solar System during its formation,” said Merel van ‘t ’Hoff, an astronomer at the University of Michigan and a co-author of the paper. “This is exciting as it suggests that other planetary systems should have received large amounts of water too.”
Clarifying the role of water in the development of comets and planetesimals is critical to building an understanding of how our own Solar System developed. Although the Sun is believed to have formed in a dense cluster of stars and V883 Ori is relatively isolated with no nearby stars, the two share one critical thing in common: they were both formed in giant molecular clouds.
“It is known that the bulk of the water in the interstellar medium forms as ice on the surfaces of tiny dust grains in the clouds. When these clouds collapse under their own gravity and form young stars, the water ends up in the disks around them. Eventually, the disks evolve and the icy dust grains coagulate to form a new solar system with planets and comets,” said Margot Leemker, an astronomer at Leiden University and a co-author of the paper. “We have shown that water that is produced in the clouds follows this trail virtually unchanged. So, by looking at the water in the V883 Ori disk, we essentially look back in time and see how our own Solar System looked when it was much younger.”
Tobin added, “Until now, the chain of water in the development of our Solar System was broken. V883 Ori is the missing link in this case, and we now have an unbroken chain in the lineage of water from comets and protostars to the interstellar medium.”
Resource
“Deuterium-enriched water ties planet-forming disks to comets and protostars,” J. Tobin et al, 8 March 2023, Nature, https://doi.org/10.1038/s41586-022-05676-z
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About ALMA
The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Organisation for Astronomical Research in the Southern Hemisphere (ESO), the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the Ministry of Science and Technology (MOST) and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).
ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.
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Astrobiology, Astrochemistry
