Moon-forming region seen around planet in another solar system
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[July 23, 2021]
By Will Dunham
(Reuters) - Scientists for the first time
have spotted a moon-forming region around a planet beyond our solar
system - a Jupiter-like world surrounded by a disk of gas and dust
massive enough that it could spawn three moons the size of the one
orbiting Earth.
The researchers used the ALMA observatory in Chile's Atacama desert to
detect the disk of swirling material accumulating around one of two
newborn planets seen orbiting a young star called PDS 70, located a
relatively close 370 light years from Earth. A light year is the
distance light travels in a year, about 5.9 trillion miles (9.5 trillion
km).
It is called a circumplanetary disk, and it is from these that moons are
born. The discovery, the researchers said, offers a deeper understanding
about the formation of planets and moons.
More than 4,400 planets have been discovered outside our solar system,
called exoplanets. No circumplanetary disks had been found until now
because all the known exoplanets resided in "mature" - fully developed -
solar systems, except the two infant gas planets orbiting PDS 70.
"These observations are unique - so far - and have been long waited for,
in order to test the theory of planet formation and directly observe the
birth of planets and of their satellites," said astronomer Myriam
Benisty of the University of Grenoble, who led the study published on
Thursday in the Astrophysical Journal Letters.
In our solar system, the impressive rings of Saturn, a planet around
which more than 80 moons orbit, represent a relic of a primordial
moon-forming disk, said study co-author Stefano Facchini of the European
Southern Observatory.
The orange-colored star PDS 70, roughly the same mass as our sun, is
about 5 million years old - a blink of the eye in cosmic time. The two
planets are even younger.
Both planets are similar (although larger) to Jupiter, a gas giant that
is our solar system's biggest planet. It was around one of the two
planets, called PDS 70c, that a moon-forming disk was observed.
Researchers previously had found initial evidence of a disk around this
planet, but now have confirmed it.
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An undated image, taken with the Atacama Large Millimeter/submillimeter
Array (ALMA), in which the European Southern Observatory is a
partner, shows wide (left) and close-up (right) views of the
moon-forming disc surrounding PDS 70c, a young Jupiter-like planet
nearly 400 light-years away. The close-up view shows PDS 70c and its
circumplanetary disc center-front, with the larger circumstellar
ring-like disc taking up most of the right-hand side of the image.
The star PDS 70 is at the center of the wide-view image on the left.
ALMA (ESO/NAOJ/NRAO)/Benisty et al/Handout via REUTERS
Both planets are "still in their youth," Facchini
said, and are at a dynamic stage in which they are still acquiring
their atmospheres. PDS 70c orbits its star at 33 times the distance
of the Earth from the sun, similar to the planet Neptune in our
solar system. Benisty said there are possible additional so-far
undetected planets in the system.
Stars burst to life within clouds of interstellar gas and dust
scattered throughout galaxies. Leftover material spinning around a
new star then coalesces into planets, and circumplanetary disks
surrounding some planets similarly yield moons.
The dominant mechanism thought to underpin planet formation is
called "core accretion," said study co-author Richard Teague of the
Harvard-Smithsonian Center for Astrophysics.
"In this scenario, small dust grains, coated in ice, gradually grow
to larger and larger sizes through successive collisions with other
grains. This continues until the grains have grown to a size of a
planetary core, at which point the young planet has a strong enough
gravitational potential to accrete gas which will form its
atmosphere," Teague said.
Some nascent planets attract a disk of material around them, with
the same process that gives rise to planets around a star leading to
the formation of moons around planets.
The disk around PDS 70c, with a diameter about equal to the distance
of the Earth to the sun, possesses enough mass to produce up to
three moons the size of Earth's moon. It is unclear how many will
form, if any.
(Reporting by Will Dunham in Washington, Editing by Rosalba O'Brien)
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