Astronomers using the Atacama Large Millimetre/submillimeter Array (ALMA) have detected a circumplanetary disk — a ring-shaped area where moons and other satellites may form — around a protoplanet in the PDS 70 system.
This ALMA image shows a close-up view on the circumplanetary disk surrounding PDS 70c. Image credit: ALMA / ESO / NAOJ / NRAO / Benisty et al.
PDS 70 is a K7-type star located 370 light-years away in the constellation of Centaurus.
Also known as VV1032 Cen and IRAS 14050-4109, the star is only 5.4 million years old.
It hosts two protoplanets and a huge circumstellar disk of dust and gas in which a large region from 20 to 40 AU is cleared of dust.
The inner planet, PDS 70b, is located within the disk gap at a distance of about 22 AU from the star, similar to the orbit of Uranus in our Solar System.
The outer planet, PDS 70c, is located near the outer edge of the disk gap at 34 AU from the star, similar to Neptune’s distance from our Sun.
This ALMA image shows the PDS 70 planetary system. The system features a star at its center and at least two planets orbiting it, PDS 70b (not visible in the image) and PDS 70c, surrounded by a circumplanetary disk (the dot to the right of the star). Image credit: ALMA / ESO / NAOJ / NRAO / Benisty et al.
“Our work presents a clear detection of a disk in which satellites could be forming,” said Dr. Myriam Benisty, an astronomer at the University of Grenoble and the University of Chile.
“The new ALMA observations were obtained at such exquisite resolution that we could clearly identify that the disk is associated with PDS 70c and we are able to constrain its size for the first time.”
Dr. Benisty and colleagues also found that PDS 70c’s disk has about the same diameter as the distance from our Sun to the Earth and enough mass to form up to three satellites the size of the Moon.
“These new observations are also extremely important to prove theories of planet formation that could not be tested until now,” said Dr. Jaehan Bae, an astronomer in the Earth and Planets Laboratory at the Carnegie Institution for Science.
Planets form in dusty disks around young stars, carving out cavities as they gobble up material from this circumstellar disk to grow.
In this process, a planet can acquire its own circumplanetary disk, which contributes to the growth of the planet by regulating the amount of material falling onto it.
At the same time, the gas and dust in the circumplanetary disk can come together into progressively larger bodies through multiple collisions, ultimately leading to the birth of moons.
But astronomers do not yet fully understand the details of these processes.
“In short, it is still uncl