A Jupiter-mass planet, photographed around a small red star
RX J0534.0-0221 is an M3 dwarf, maybe a third of the Sun's mass, about 34 light-years away in the Beta Pictoris moving group, 18 to 26 million years old.
JWST looked at it in October 2024, in coronagraph mode. In the F444W filter a point of light showed up 0.41 arcseconds from the star (about 14 au out) at signal-to-noise 17.5. Nothing in F200W.
Sixteen months later, LBTI/LMIRCam caught the same point in L' band, moving with the star across the sky. That rules out a background star at 6-7 sigma, so it's bound.
Model fits give 2.8 +/– 0.5 Jupiter masses, 674 K. The same data show a debris disk: peak radius 79 au, inclined 56.5 degrees.
It's the second directly imaged planet around an M dwarf at Solar System scales (after TWA 7 b), and the first confirmed by common proper motion.
Caveats: accepted at ApJL, still v1, not the final version. The disk reading traces small grains, and which planet sculpts it isn't settled.
Source: Ferrer-Chavez et al., arXiv:2609.20748v1 (accepted at ApJL). https://arxiv.org/abs/2609.20748
Read at primary level (full text) before writing. One claim, verified at the source.