A new study of the interstellar
comet 3I/ATLAS led by the University of Michigan shows that its water has a
remarkably high content of deuterium. This form of hydrogen is comparatively
less abundant in our solar system, enabling researchers to glean new insights
about other planetary processes at work in our galaxy. Credit: U-M News/Hans
Anderson
Less than a year ago, astronomers discovered a comet soaring
through our sky that was not from our solar system. Although we still don't
know where this interstellar object called 3I/ATLAS came from, research led by
the University of Michigan has revealed new insights about its birthplace.
Wherever that was, it was much colder than the environment that created our
solar system.
A comet rich in heavy water
The new finding is based on the
observation that 3I/ATLAS is remarkably rich in a
specific type of water that contains deuterium. The team's study is published in the journal Nature
Astronomy.
"Our new observations show
that the conditions that led to the formation of our solar system are much
different from how planetary systems evolved in different parts of our
galaxy," said Luis Salazar Manzano, lead author of the new study and a doctoral
student in the U-M Department of Astronomy.
Water is made of two hydrogen atoms
and one oxygen atom, hence its H2O formula. In typical water
molecules, though, those hydrogen atoms have just one proton at their core. In
the comet's water, a high ratio of its water molecules contain deuterium, a
form of hydrogen with the standard issue proton plus a neutron. These heavier
forms of water also exist on Earth, but in much lower quantities than were
observed in 3I/ATLAS.
"The amount of deuterium with
respect to ordinary hydrogen in water is higher than anything we've seen before
in other planetary systems and planetary comets," Salazar Manzano said.
In fact, the ratio was 30 times
that of any comet in our solar system, Salazar Manzano said, and 40 times the
value found in the water in our oceans.
These ratios tell researchers about
the conditions that were present where these celestial objects formed, allowing
them to compare the birthplace of 3I/ATLAS with our solar system when planets
and comets were forming. In particular, this result means 3I/ATLAS came from somewhere colder
and with lower levels of radiation, said Teresa Paneque-Carreño, a co-leader of
the new study and U-M assistant professor of astronomy.
"This is proof that whatever
the conditions were that led to the creation of our solar system are not
ubiquitous throughout space," Paneque-Carreño said. "That may sound
obvious, but it's one of those things that you need to prove."
How astronomers studied 3I/ATLAS
Accomplishing an unprecedented
study like this required a lot of things going right, the team said. It started
with astronomers discovering 3I/ATLAS early enough to enable follow-up studies,
Paneque-Carreño said.
With the comet's timely discovery,
Salazar Manzano and other collaborators could secure time at the MDM
Observatory in Arizona, where they saw some of the earliest evidence of gas
emission from the comet (MDM stands for Michigan, Dartmouth and the Massachusetts
Institute of Technology, the observatory's original partners).
That's when Salazar Manzano
contacted Paneque-Carreño to collaborate, who brought expertise with the
Atacama Large Millimeter/submillimeter Array, or ALMA, in Chile to further
observe and characterize the comet's chemical properties.
ALMA is sensitive enough to detect
the subtle difference between deuterated and conventional water that the team
could characterize the ratio between the two. This study represents the first
time scientists have been able to perform this type of analysis on an
interstellar object.
"Being at the University of
Michigan and having access to these facilities was the key to making this work
possible," Salazar Manzano said. "We were part of a team that was
very talented and very experienced in multiple areas, all of us complemented
each other and that's what allowed us to analyze and interpret these data
sets."
What this means for future searches
This work also shows that it will
be possible to characterize future
interstellar objects in this way to learn more about what goes on in planetary systems
beyond our solar system. Although 3I/ATLAS is only the third interstellar
object that astronomers have discovered to date, that count is likely to
increase as new observatories join the search, Paneque-Carreño said—as long as
we don't make it too hard on ourselves.
"We need to be taking care of our night skies and keeping them clear and dark so we can detect these tiny and faint objects," she said.
edited by Sadie
Harley, reviewed by Robert
Egan

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