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Gaps in gas disks around stars may not always mark newborn planets

The photo album of baby planets may be emptier than astronomers thought.

New research is prompting..

The photo album of baby planets may be emptier than astronomers thought.

New research is prompting debate about the theory that gaps in planet-forming disks around young stars mark spaces where planets are being created in real time. It turns out that the planets that, according to simulations, would grow up in those gaps dont resemble the full-grown planets observed around more mature stars.

So, maybe these broken-up disks dont point to the formation of planets at all — or at least, not the most common kinds of planets that current telescopes can see.

“The question we raised, and we put it boldly, is whether those gaps in rings are really caused by planets, or they are caused by other things,” says astrophysicist Nelson Ndugu of Mbarara University of Science and Technology in Uganda. “Right now, it is too early to take a side.”

Baby photos [hhmc]

The basic planet formation recipe starts from a cloud of gas and dust, which collapses into a central star surrounded by a rotating disk (SN: 5/12/18, p. 28). Gravity draws the gas and dust into pebble-sized clumps, which cluster into boulders. Eventually those boulders grow large and gravitationally powerful enough to start hoovering up the surrounding gas, ultimately growing into gas giants. Theoretical models suggested that whole process should take about 10 million years to build a Jupiter.

In 2014, astronomers got what looked like their first glimpse of this process in action. The Atacama Large Millimeter/submillimeter Array in Chile, or ALMA, snapped a shot of the young star HL Tau, about 450 light-years away in the constellation Taurus, that showed a disk interrupted by dark gaps (SN: 11/29/14, p. 32).

 Researchers initially attributed such gaps to newborn planets that scooped up disk gas as they grew. A similar process is thought to have <a href="" rel="noreferrer noopener" target="_blank">shaped the rings and moons</a> around Saturn (SN: 9/2/17, p. 16). Then in 2018, astronomers reported a planet called <a href="" rel="noreferrer noopener" target="_blank">PDS 70b</a>, the first infant planet to have been spotted growing in such a disk gap (SN: 8/4/18, p. 5). Later observations found a second planet orbiting the same star. 

Trouble is, the planets orbiting PDS 70 are still the only examples. The theory didnt quite fit for HL Tau, either: The star was only 1 million years old, too young to have gotten so far in forming a planetary system.

“It didnt really make sense,” says astrophysicist Nienke van der Marel at the Herzberg Institute for Astrophysics in Victoria, Canada. In February, she and her colleagues published in the Astrophysical Journal a survey of 16 other protoplanetary disks, with ages ranging from less than half a million years to more than 10 million years. All of the disks were broken into gaps and rings, rather than being smooth expanses of gas.

“That is hard to explain if its caused by planets,” she says. If all of those gaps marked spots of planet formation, that would mean “planets must form extremely fast.”

Middle step mismatch [hhmc]

Even if planets were responsible for all the gaps observed, things still dont add up, Ndugu and colleagues argue in a paper posted at on June 27. The researchers ran computer simulations of planets growing up, and compared the resulting ringed disks to ALMA observations of 20 protoplanetary disks from a 2018 survey called DSHARP.

“We took this [survey] as a middle step for our formation simulations to see what actually happens,” says astrophysicist Bertram Bitsch of the Max Planck Institute for Astronomy in Heidelberg, Germany. The team then let the simulations run until the disk was gone, either coalesced into planets or blown away by the stars radiation.

Both steps of the simulation produced results that deviated from whats observed in the galaxy. First, the simulations suggested the outer reaches of disks needed about 2,000 times Earths mass in pebbles in order to grow planets that could open up the observed gaps. But most stars dont have that much material in their disks outer reaches.

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