New radio astronomy
observations of a planetary system in the process of forming show that once the
first planets form close to the central star, these planets can help shepherd
the material to form new planets farther out. In this way each planet helps to
form the next, like a line of falling dominos each triggering the next in turn.
To date over 5000 planetary systems have
been identified. More than 1000 of those systems have been confirmed to host
multiple planets. Planets form in clouds of gas and dust known as
protoplanetary disks around young stars. But the formation process of multi-planet
systems, like our own Solar System, is still poorly understood.
The best example object to study
multi-planet system formation is a young star known as PDS 70, located 367
light years away in the direction of the constellation Centaurus. This is the
only celestial object where already-formed planets have been confirmed within a
protoplanetary disk by optical and infrared observations (First Confirmed Image of Newborn Planet Caught with ESO’s
VLT (ESO) ). Previous
radio wave observations with the Atacama Large Millimeter/submillimeter Array
(ALMA) revealed a ring of dust grains outside the orbits of the two known
planets. But those observations could not see into the ring to observe the
details.
In this research, an international team
led by Kiyoaki Doi, formerly a Ph.D. student at the National Astronomical
Observatory of Japan (NAOJ)/the Graduate University for Advanced Studies,
SOKENDAI and currently a postdoctoral fellow at the Max Planck Institute for
Astronomy, performed high-resolution observations of the protoplanetary disk
around PDS 70. The team again used ALMA, but observed at a longer wavelength of
radio waves. This is because longer wavelengths are better for peering into the
dusty cloud of the protoplanetary disk.
The new ALMA observations clearly show a
concentration of dust grains to the north-west (upper right) in the ring
outside the orbits of the two existing planets. The location of this dust clump
suggests that the already-formed planets interact with the surrounding disk,
concentrating dust grains into a narrow region at the outer edge of their
orbits. These clumped dust grains are thought to grow into a new planet. This
work observationally shows that the formation of planetary systems, like the
Solar System, can be explained by the sequential formation of the planets from
inside to outside by the repetition of this process; like a line of falling
dominos, each one triggering the next.
Source: https://www.nao.ac.jp/en/news/science/2024/20241213-alma.html
Image: Compared to the previous
observations (left), the new ALMA observations (right) at longer wavelengths
can better see into the dust ring and reveal a concentration of dust to the
north-west (upper right) where a new planet is forming. (Credit: ALMA
(ESO/NAOJ/NRAO), W. M. Keck Observatory, VLT (ESO), K. Doi (MPIA))
Journal article: https://www.soken.ac.jp/en/news/2024/20241213.html
Source: Planets Form Through Domino Effect – Scents of Science
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