The gas giant PDS 70b made headlines last month as the first newly forming planet to ever be directly imaged. Now a team of scientists has gone a step further: they’ve captured evidence that this planet is actively accreting material, and they’ve measured the rate at which it’s growing.
The Search for Evidence
In the recent era of high-resolution observations, indirect evidence of planet formation abounds. In particular, we’ve captured a number of spectacular images of gapped disks surrounding young stars — disks in which we think the first planets of those systems are being born. According to models, planets will grow as they accrete matter from the surrounding protostellar disk, simultaneously clearing a gap in the disk as they orbit.
In spite of the accumulation of indirect evidence, direct evidence was long lacking — until recently. The young (10 million years old) dwarf star PDS 70, located just 370 light-years from Earth, is surrounded by a disk with a distinctive gap. And just last month, scientists announced that they’ve directly imaged, and confirmed, the presence of a newborn planet orbiting within the gap.
But just demonstrating that a planet lies within the gap isn’t yet enough — the next step is to prove that this planet, PDS 70b, is actively accreting material. This is where high-contrast observations from the Magellan Adaptive Optics system come in.
A Sign of Accretion
In a new study led by Kevin Wagner (University of Arizona, Amherst College, and NASA NExSS Earths in Other Solar Systems Team), a team of scientists used the adaptive optics system on the 6.5-m Magellan Clay Telescope in Chile to image the PDS 70 system in Hα (656 nm) and nearby continuum wavelengths. The presence of Hα emission at the location of the planet PDS 70b would indicate shocked, hot, infalling hydrogen gas — a smoking gun demonstrating that this planet is still accreting matter.
Sure enough, Wagner and collaborators detected the presence of an Hα signal from PDS 70b on two sequential nights this past May — a signal that has less than a 0.1% probability of being a false positive. It seems fairly safe to say this baby planet is still growing.
Nearing Full Size
But how fast is it growing, and how far along is it? Wagner and collaborators use their Hα luminosity measurements to calculate a mass accretion rate for PDS 70b, finding that the gas giant is growing at a rate of 10^-8±1 Jupiter masses per year. At this rate, and based on the age of the system, the authors estimate that PDS 70b likely accreted mass at a much higher rate in the past, and it has already acquired more than 90% of its final mass.
This nearby planet caught in the act of forming will make for an excellent study target in the future, as we continue to piece together our understanding of how planets are born and grow in protoplanetary disks.
“Magellan Adaptive Optics Imaging of PDS 70: Measuring the Mass Accretion Rate of a Young Giant Planet within a Gapped Disk,” Kevin Wagner et al 2018 ApJL 863 L8. doi:10.3847/2041-8213/aad695
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This post originally appeared on AAS Nova, which features research highlights from the journals of the American Astronomical Society.