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Home»Science»Astronomers uncover a brand new sort of planet that in all probability smells like rotten eggs
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Astronomers uncover a brand new sort of planet that in all probability smells like rotten eggs

Buzzin DailyBy Buzzin DailyMarch 16, 2026No Comments4 Mins Read
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Astronomers uncover a brand new sort of planet that in all probability smells like rotten eggs
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Astronomers have used the James Webb House Telescope (JWST) to research a brand new sort of planet. This molten lava world past the photo voltaic system seemingly smells like rotten eggs, and suggests that there’s a a lot wider range of worlds past our photo voltaic system than beforehand acknowledged.

The additional-solar planet, or exoplanet, is designated L 98-59 d, and it orbits a small purple star positioned about 35 light-years away. Information from the JWST and an array of Earth-based telescopes counsel that this exoplanet, which is round 1.6 occasions the dimensions of the Earth, is extraordinarily low-density. Its ambiance is filled with hydrogen sulfide, a compound identified for its distinct rotten egg stench.

Below regular circumstances, L 98-59 d would both be labeled as a rocky fuel dwarf, with an environment wealthy in hydrogen, or as a water-rich “hycean” ocean world. Nonetheless, this exoplanet matches into neither class, justifying the creation of a brand new class of exoplanets replete with heavy sulfur molecules.

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“This discovery means that the classes astronomers at the moment use to explain small planets could also be too easy. Whereas this molten planet is unlikely to help life, it displays the vast range of the worlds which exist past the photo voltaic system,” group chief Harrison Nicholls of the College of Oxford within the UK mentioned in a press release. “We might then ask: what different varieties of planets are ready to be uncovered?”

Oceans of magma

Nicholls and colleagues have been ready to make use of superior laptop simulations to retell the practically 5 billion-year historical past of L 98-59 d. They then in contrast these fashions to precise telescope information to reconstruct what should be occurring deep beneath the floor of this exoplanet.

They decided that L 98-59 d seemingly has a mantle of molten silicate, much like the lava discovered on Earth, and an ocean of magma that spans the entire planet. This huge world magma ocean permits the exoplanet to lock away enormous quantities of sulphur over huge durations of time. Sulfur-rich gases have then been launched into the ambiance of L 98-59 d over billions of years. This consists of the sulfur dioxide and different sulfur-based molecules the JWST noticed within the planet’s higher ambiance.

The magma reservoir might have additionally helped L 98-59 d maintain on to its hydrogen and sulphur-rich ambiance, stopping it from being misplaced to house on account of bombardment of X-rays from its dad or mum star.

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NASA’s James Webb House Telescope, seen right here in an artist’s illustration (Picture credit score: NASA GSFC/CIL/Adriana Manrique Gutierrez)

Over billions of years, molecules have been exchanged between the planet’s ambiance and its inside, shaping it into the primary world in a brand new class of gas-rich sulphurous planets sustaining long-lived magma oceans.

The group’s simulations present that L 98-59 d was seemingly born with huge quantities of unstable materials and will have as soon as been a a lot bigger sub-Neptune planet. The world seemingly shrank and cooled over billions of years, dropping some, however not all, of its ambiance.

“What’s thrilling is that we are able to use laptop fashions to uncover the hidden inside of a planet we are going to by no means go to,” group member Raymond Pierrehumbert of the College of Oxford mentioned. “Though astronomers can solely measure a planet’s dimension, mass, and atmospheric composition from afar, this analysis exhibits that it’s potential to reconstruct the deep previous of those alien worlds – and uncover varieties of planets with no equal in our personal photo voltaic system.”

The group’s outcomes have been revealed on Monday (March 16) within the journal Nature Astronomy.

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