Nearby exoplanet stinks of rotten eggs, scientists discover

Scientists found trace amounts of hydrogen sulphide in a nearby exoplanet - which may give clues as to how it influences planets' atmospheres.

Undated handout photo issued by Johns Hopkins University of a nearby planet, exoplanet HD 189733 b, a Jupiter-sized gas giant outside of our solar system. Issue date: Monday July 8, 2024.
Image: The exoplanet HD 189733 b. Pic: PA
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We all have difficult neighbours - even the Earth.

Now scientists have found that a planet close to our own world stinks of rotten eggs.

The research, from scientists at the Johns Hopkins University in the US, suggests that the atmosphere of the planet HD 189733 b, a Jupiter-sized gas giant, has trace amounts of hydrogen sulphide.

HD 189733 b is an exoplanet - meaning it is outside our solar system.

The discovery of hydrogen sulphide on the exoplanet offers scientists new clues about how sulphur, a building block of planets, might influence the insides and atmospheres of exoplanets.

At only 64 light-years from Earth, HD 189733 b is the nearest "hot Jupiter" astronomers can observe passing in front of its star.

The planet also has extremely high temperatures of about 927C and is known for vicious weather, including raining glass that blows sideways on winds of 5,000mph.

Guangwei Fu, an astrophysicist at Johns Hopkins University, said: "Hydrogen sulphide is a major molecule that we didn't know was there.

"We predicted it would be, and we know it's in Jupiter, but we hadn't really detected it outside the solar system.

"We're not looking for life on this planet because it's way too hot, but finding hydrogen sulphide is a stepping stone for finding this molecule on other planets and gaining more understanding of how different types of planets form."

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The planet was discovered in 2005, and since then has been important for detailed studies of exoplanetary atmospheres.

The new data is from the James Webb Space Telescope and was published in the journal Nature. The research also ruled out the presence of methane in HD 189733 b.

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"We had been thinking this planet was too hot to have high concentrations of methane, and now we know that it doesn't," Mr Fu said.

The researchers hope to track sulphur in more exoplanets and determine how high levels of that compound might influence how close they form near their parent stars.