Two planets lighter than candy floss
Two Jupiter-sized planets orbit a star 1,110 light years away in the southern constellation Volans. Their names are TOI-791b and TOI-791c.
Both are roughly the size of Jupiter. Jupiter's density is 1.33 grams per cubic centimeter. These two manage just 0.038 and 0.047, making them lighter, gram for gram, than cotton candy. They are, essentially, planet-shaped clouds [17]. The planets are siblings, formed from the same swirling disc of gas around their young star, and they travel in a 5:3 orbital resonance: for every five laps the inner planet completes, the outer finishes almost exactly three. Each transit across their host star lasts more than 11 hours, far too long for a single night at most observatories. To catch one in full, the team turned to Antarctica, where Concordia Station sits under months of continuous polar darkness. They did it. Neither planet was found by professional astronomers. Citizen science volunteers in the Planet Hunters TESS project spotted them first, picking anomalies out of NASA satellite data in their spare time [121].
What each field noticed (2)
Two Planets Lighter Than Candy Floss
The physics here are almost farcical: these planets are roughly 30 times less dense than Jupiter, lower even than spun sugar at a fairground. The leading theory is that they formed in the cold outer reaches of their young solar system, where hydrogen and helium could pile onto a small rocky core without limit. Universe Today noted what makes them scientifically priceless: their orbital resonance creates small, measurable wobbles in transit timing, and it was those wobbles that allowed the team to weigh them. Without the resonance, the masses would have stayed hidden [17].
Read the storyTwo 'Super-Puff' Planets Lighter Than Candy Discovered by Researchers
The Good News angle was the people who found them: ordinary people with internet connections, a spare hour, and access to NASA's TESS data. The volunteers spotted the anomalies; professional astronomers then confirmed, weighed, and published. Only a handful of super-puff planets are known, and it is even rarer to find two in the same system. The planet-hunting citizen science pipeline from amateur eye to peer-reviewed paper is very real [121].




