When the Undertones sang about “Teenage Kicks,” they could well have been inadvertently referring to the chaotic and violent “teenage” periods of planetary systems that are shaped by collisions between bodies of various sizes, such as the impact upon Earth by a massive body that created the moon.
Now, using the world’s largest radio telescope project, the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have captured snapshots representing the chaotic “teenage years” of planets forming around infant stars.
“We’ve often seen the ‘baby pictures’ of planets forming, but until now, the ‘teenage years’ have been a missing link,” team co-leader Meredith Hughes of Wesleyan University, Connecticut, said in a statement. “This project gives us a new lens for interpreting the craters on the moon, the dynamics of the Kuiper Belt, and the growth of planets big and small. It’s like adding the missing pages to the Solar System’s family album.”
Teenage kicks
Hughes and colleagues used the 66 radio telescopes located in the Atacama desert region of northern Chile that make up ALMA to observe 24 disks of dusty debris around infant stars, the detritus that remains after planets have formed.
“Debris discs represent the collision-dominated phase of the planet formation process,” ARKS team member Thomas Henning of the Max Planck Institute for Astronomy (MPIA) said. “With ALMA, we are able to characterise the disc structures pointing to the presence of planets. In parallel, with direct imaging and radial velocity studies, we are searching for young planets in these systems.”
Evidence of this period of the solar system’s history can be seen in the icy ring of comets beyond the orbit of Neptune known as the Kuiper Belt. These objects were created through massive collisions and planetary migrations that occurred around the sun billions of years ago, around the same time as Earth’s moon was forming.
Planet baby pictures are fairly easy to obtain because the gas-rich disks in which they form, protoplanetary disks, are bright. Debris disks like the 24 seen by ALMA are thousands of times fainter, which is why they have proved so elusive for many years.
ALMA collected the radio wavelength emissions from dust particles and other molecules in these disks to build a picture of their complex structures, revealing multiple rings, wide and smooth outer halos, and unexpected arcs and clumps.
“We’re seeing real diversity – not just simple rings, but multi-ringed belts, halos, and strong asymmetries, revealing a dynamic and violent chapter in planetary histories,” ARKS team member and University of Exeter researcher Sebastián Marino said.
The key to this level of detail is the fact that with its 66 antennas, ALMA and its radio interferometry technique provide a wider view than any single telescope. This has confirmed that the teenage phase of planetary systems is a time of great upheaval.
“These discs record a period when planetary orbits were being scrambled and huge impacts, like the one that forged Earth’s moon, were shaping young solar systems,” team member Luca Matrà, of Trinity College Dublin, Ireland, added.
The team’s research was published on Tuesday (Jan. 20) in the journal Astronomy & Astrophysics.
