Posted on by Evan Gough

JWST Uses “Interferometry Mode” to Reveal Two Protoplanets Around a Young Star

Astronomers used the JWST's interferometry mode to study the PDS 70 extrasolar system. Image Credit: Blakely et al. 2024.

The JWST is flexing its muscles with its interferometry mode. Researchers used it to study a well-known extrasolar system called PDS 70. The goal? To test the interferometry mode and see how it performs when observing a complex target.

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Posted on by Evan Gough

Here’s a First. Astronomers See a Moon Forming Around a Baby Exoplanet

A color-enhanced image of millimeter-wave radio signals from the ALMA observatory in Chile shows a disk of gas and dust (right of center) around exoplanet PDS 70 c, the first-ever observation of the kind of circumplanetary disk that is believed to have birthed the moons of Jupiter more than 4 billion years ago. CREDIT A. Isella, ALMA (ESO/NAOJ/NRAO))

Astronomers have discovered, for the first time, moons forming in the disk of debris around a large exoplanet. Astronomers have suspected for a long time that this is how larger planets—like Jupiter in our own Solar System—get their moons. It’s all happening around a very young star named PDS 70, about 370 light years away in the constellation Centaurus.

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