We’ve Found Possible Signs of Life in Venus’s Clouds. Whoa!

Venus is our closest planetary neighbour, and above its oppressive surface, in the clouds, there is a mystery.

In the planet’s clouds, scientists have discovered traces of phosphine, a substance that may be produced by living organisms.

In Venus’ hazy atmosphere, life may exist, as scientists have long assumed. The surface of Venus reaches temperatures of more than 800 degrees Fahrenheit, making it unfriendly. No probe sent to the planet has managed to survive for more than a few hours. But the planet’s atmosphere, which is made up of thick layers of sulfuric acid clouds, might offer a special environment for the development of new lifeforms.

“We know that the molecule phosphine is a biomarker on Earth,” astronomer Jane Greave, of Cardiff University in Wales, said in a pre-recorded statement released by the Royal Astronomical Society. “It’s been suggested that there are possible habitats in the cloud decks of Venus, so somewhere where little lifeforms could live.”

Fair enough, this most recent discovery does not specifically point to the existence of life on other planets, but it is the closest thing we’ve ever come. The only explanations for the molecule, according to the researchers, are that it is either being produced by a living entity or that it was created by a chemical process that is currently unknown to science. They published their findings in the journals Nature Astronomy and Astrobiology today.

Molecular of the Day

Phosphine (PH3) is made up of a single phosphorus atom sandwiched by three hydrogen atoms. “I like to think of phosphine as ammonia’s evil cousin,” Greaves said. (Ammonia, by comparison, is made up of a nitrogen atom surrounded by three hydrogen atoms.)Anaerobic microbes, which thrive in environments without oxygen here on Earth, also produce phosphine. “They’ve got a completely different way of life to much of what we’re used to,” Greaves said.

Scientists have yet to determine how these microbes produce the compound, which can also be produced in a laboratory. Phosphine is poisonous to many animals, and the colorless, flammable gas has been used in chemical warfare and by farmers to snuff out tenacious pests.

The chemical has also been discovered elsewhere in the solar system, in the cores of Jupiter and Saturn. But, unlike Venus, there is a reason. The stifling heat and crushing pressure on these planets is strong enough to shatter hydrogen and phosphorus atoms together. However, there isn’t enough heat or pressure on Venus for phosphine to be produced this way.

Conditions aren’t so bad 31 miles above the Venusian surface. Temperatures linger at about 86 degrees Fahrenheit well above the rocky planet’s cloud decks. At this altitude, the air pressure is comparable to that found on Earth’s surface. The only catch is that Venus’s clouds are sulfuric alkaline, creating an extremely caustic environment.

However, in other cases, life on Earth flourishes under these conditions. Microbes have been identified in rocky crevices deep beneath the oceans and around geothermal springs in areas like Yellowstone and Iceland. The microorganisms that create phosphine have been found in the stomachs of animals such as penguins, deep sea worms, and, yes, humans.


In order to identify the chemical makeup of distant atmospheres, scientists use radio telescopes to make observations across a wide swath of wavelengths of light. Greaves and her colleagues studied compounds in Venus’ deadly atmosphere using the James Clark Maxwell radio telescope atop Hawaii’s Mauna Kea volcano in 2017.

“If you look at a very specific wavelength, a little bit of that light is missing because the phosphine molecules have absorbed and so it’s not present,” Greaves said.

Greaves contacted MIT researchers after discovering the signal of phosphine, and the two partnered to make additional observations using Chile’s Atacama Large Millimeter Array in 2019. If the new coronavirus pandemic had not come earlier this year and largely shut down the world’s observatories, the scientists would have made additional measurements.

According to National Geographic, the researchers were eventually able to establish a range of altitudes where the molecule was plentiful, between 32 and 37 miles above the surface. And it was plentiful: the scientists measured phosphine concentrations ranging from 5 to 20 parts per billion—much more than the quantity found in Earth’s atmosphere and far more than the team expected to find.

Dreaming about phosphine

Some experts are sceptical about the findings, assuming that an error occurred during the data collection process.

“They took the right steps to verify the signal, but I’m still not convinced that this is real,” ALMA observatory scientist John Carpenter told National Geographic. “If it’s real, it’s a very cool result, but it needs follow-up to make it really convincing.” Other researchers chalk the findings up to some sort of undiscovered geochemical process.

It is not a novel thought that life could exist amid the caustic clouds of Venus.In the magazine Nature in 1967, astronomers Harold Morowitz and Carl Sagan wrote, “The conditions in Venus’s lower clouds match those on Earth more than any other alien environment yet known.” Despite Venus’s promise as a cradle for life, it has been largely overlooked, perhaps due to the logistical challenges of travelling there, or perhaps because other sites in the solar system—look at you, Mars and Europa—seemed more enticing.

NASA’s Mariner 2 became the first spacecraft to sail by Venus in 1962. The Soviet Union responded by sending its Venera spacecraft to the planet. The Venera 7 spacecraft was the first to survive a soft landing on Venus, although it melted within seconds. Venera 9 took the first image of the Venusian surface.

The Magellan mission, conducted by NASA in 1989, produced the first global map of Venus. At the moment, only the Japanese Aerospace Exploration Agency’s Akatsuki orbiter is monitoring Venus. In comparison, Mars has eight current missions.

NASA, on the other hand, is now investigating two potential Discovery Program trips to Venus. One project, VERITAS (Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy), attempts to scan the planet’s surface in order to unearth its many geologic mysteries.

The other mission, DAVINCI+, will examine Venus’s atmosphere by sending a probe to the planet’s rocky surface. During the descent, it will collect trace gas samples and image the volatile atmosphere as well as the rocky surface below.

“Venus is the key to understanding how Earth-size planets evolve,” Martha Gilmore, an astronomer at Wesleyan University and a co-developer of both projects, said in a February press statement. “Like Earth, we predict Venus had an ocean that may have lasted for billions of years. Like Earth, Venus may be volcanically and tectonically active today.”

The two missions “will focus on Venus’s contemporary and ancient past as recorded in rocks and the atmosphere,” according to Gilmore. While Mars has been the centre of attention for decades, Venus’s turn may not be far behind.

The Indian Space Research Organization has announced plans to undertake a Venus expedition in the next years. Meanwhile, Rocket Lab CEO Peter Beck has been forthcoming about his company’s plans to launch a private research journey to Venus.

“The biggest question that I can possibly think of to try and and answer is: Is life on Earth unique or is prolific throughout the universe?” Beck said in an interview on the Orbital Mechanics podcast. “If you could find life in the clouds of Venus, then you would gravitate to the natural assumption that actually life is prolific.”