This article is not about you or your posterior body section involved in releasing gas.  Researchers established on Monday that the seventh planet from the sun has an upper ambiance crammed with one of the most crucial smelliest chemical substances known to humans, hydrogen sulfide.

 

This view of Uranus was recorded by Voyager 2 on Jan 25, 1986, as the spacecraft left the planet behind and set forth on the cruise to Neptune Voyager was 1 million kilometers (about 600,000 miles) from Uranus when it acquired this wide-angle view. Image Credit: NASA/JPL

 

The odorous gas is what offers rotten eggs — and human flatulence — their distinct and horrendous smell.  “If an unfortunate human were ever to descend through Uranus’s clouds, they would be met with very unpleasant and odiferous conditions,” Said physisist Patrick Irwin, from the University of Oxford who led the study.

 

This view of Uranus was recorded by Voyager 2 on Jan 25, 1986, as the spacecraft left the planet behind and set forth on the cruise to Neptune Voyager was 1 million kilometers (about 600,000 miles) from Uranus when it acquired this wide-angle view. Image Credit: NASA/JPL

 

Scientists detected manifestations of “the noxious gas swirling high in the giant planet’s cloud tops” after viewing how sunlight would rebound off Uranus’s atmosphere, the Gemini Observatory, which uses a high-power telescope located on top of Hawaii’s Mauna Kea volcano.

The new results were clear after decades of monitoring and even a sojourn by the Voyager 2 spacecraft to Uranus. Even before asserting this revelation, scientists had long unquestioned that hydrogen sulfide resided in the planet’s atmosphere however never “conclusively detected” the chemical previously, according to Science News.

This view of Uranus was recorded by Voyager 2 on Jan 25, 1986, as the spacecraft left the planet behind and set forth on the cruise to Neptune Voyager was 1 million kilometers (about 600,000 miles) from Uranus when it acquired this wide-angle view. Image Credit: NASA/JPL

 

Uranus’s atmospheric make up was very difficult to investigate because, when a clouds form by condensation, they hide the gas engaged in forming the clouds underneath the levels that can commonly be viewed with telescopes, Leigh Fletcher, a member of the research team, said in the news release. “Only a tiny amount remains above the clouds as a saturated vapor,” said Fletcher, who is a planetary scientist at the University of Leicester in Britain. “The superior capabilities of Gemini finally gave us that lucky break.”

Discerning this data is important in comprehending Uranus’ birthplace and its evolution. This will help scientist learn about how other planets were created.

Written by Cesar Moya