DiscoverSETI LiveA Vaporizing Planet: Why BD+05 4868 b is Turning to Dust
A Vaporizing Planet: Why BD+05 4868 b is Turning to Dust

A Vaporizing Planet: Why BD+05 4868 b is Turning to Dust

Update: 2025-09-12
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Join communications specialist Beth Johnson for a live interview with astrophysicist Marc Hon (MIT), lead author of a new study revealing one of the most extreme exoplanets ever discovered — a small, rocky world that's literally disintegrating as it orbits its star. BD+05 4868 b is a Mercury-sized planet just 140 light-years away that’s orbiting so close to its star, it’s roasting at around 1650°C. The heat is intense enough to vaporize the planet’s rocky surface, creating a massive comet-like tail of mineral dust stretching millions of kilometers across space. This rare discovery — only the fourth known disintegrating planet — offers scientists an unprecedented opportunity to study the geology of an alien world, and upcoming JWST observations could even reveal the chemical makeup of its interior. (Recorded live 17 July 2025.)

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A Vaporizing Planet: Why BD+05 4868 b is Turning to Dust

A Vaporizing Planet: Why BD+05 4868 b is Turning to Dust

SETI Institute