Hopes of finding life on Venus are DASHED as clouds don’t contain enough water to sustain aliens

Scientists have dashed any remaining hopes of finding life on Venus, the second-closest planet to the Sun.  

Clouds on Venus don’t contain enough water to sustain even organisms that are adapted to live in extreme environments on Earth, they reveal. 

The researchers, led by Queen’s University Belfast, looked at data from various scientific probes, including Galileo, sent to different planets in the Solar System. 

There is more than a 100 times less water available in Venus’ atmosphere than what is necessary for any organisms to survive, they found.   

Venus is terrestrial planet similar in size to Earth, but it has a surface temperature around 867°F (464°C) and pressure 92 times that of our home planet. 

Image of Venus showing its acidic clouds, taken by the ultraviolet imager of the Venus Climate Orbiter Akatsuki on November 27, 2018

Image of Venus showing its acidic clouds, taken by the ultraviolet imager of the Venus Climate Orbiter Akatsuki on November 27, 2018

Image of Venus showing its acidic clouds, taken by the ultraviolet imager of the Venus Climate Orbiter Akatsuki on November 27, 2018

Known as Earth’s ‘evil twin’, scientists believe Venus was likely habitable 700 million years ago, before it mysteriously became inhabitable. 

Today, Venus is a world of intense heat, crushing atmospheric pressure and clouds of corrosive acid. 

A high level of sulphuric acid droplets in the planet’s clouds reduce ‘water activity’, the scientists explain.  

‘In our study, we looked at the effective concentration of water molecules which we scientifically called water activity,’ author Dr John E Hallsworth at the School of Biological Sciences, Queen’s University Belfast told PA Media. 

‘Not only we found the effective concentration of water molecules is slightly below what is needed for the most resilient microorganism on Earth, its more than 100 times too low.

This picture of Venus was taken by the Galileo spacecraft, at a range of almost 1.7 million miles. A spatial filter has been applied in order to emphasise the smaller scale cloud features, and the rendition has been colourised to a bluish hue in order to show the subtle contrasts in the cloud markings and to indicate that it was taken through a violet filter

This picture of Venus was taken by the Galileo spacecraft, at a range of almost 1.7 million miles. A spatial filter has been applied in order to emphasise the smaller scale cloud features, and the rendition has been colourised to a bluish hue in order to show the subtle contrasts in the cloud markings and to indicate that it was taken through a violet filter

This picture of Venus was taken by the Galileo spacecraft, at a range of almost 1.7 million miles. A spatial filter has been applied in order to emphasise the smaller scale cloud features, and the rendition has been colourised to a bluish hue in order to show the subtle contrasts in the cloud markings and to indicate that it was taken through a violet filter

VENUS: EARTH’S SISTER WORLD 

Venus and Earth are remarkably similar in size but their histories differ.

The second planet from the Sun sits in the inner edge of the habitable zone, in fact scientists believe it may have been habitable 700 million years ago.

A single day on the inhospitable world is 243 Earth days, compared to the 24 hours on Earth. 

It is a terrestrial planet similar in size, mass proximity to the sun and bulk composition as the Earth. 

However, it has the densest atmosphere of the terrestrial planets, made up of 96% carbon dioxide and a pressure at the surface 92 times greater than Earth. 

It has the hottest surface of any planet in the solar system with a mean temperature of 867 degrees Fahrenheit. 

Its clouds are made of sulfuric acid, with acid rain falling to the hot surface.

It may have had oceans in the past, but the water would have been vaporised as temperatures rose due to a runaway greenhouse effect. 

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‘It is almost at the bottom of the scale and an unbridgeable distance from what life requires to be active.’

The results appear to contradict research published last year that suggested phosphine gas in Venus’s atmosphere was an indicator of life in the planet’s clouds. 

While Venus doesn’t appear to be habitable, researchers found that Jupiter’s clouds have the right water conditions that would allow life as we know it. 

‘One thing which we found which was unexpected was that the clouds of Jupiter actually have the right temperature and water activity combination to support active life,’ Dr Hallsworth added. 

‘We absolutely hadn’t expected that.

‘I am not suggesting there is life on Jupiter – it would need the right nutrients to be there and I am not sure of that. 

‘Life doesn’t only need a nice temperature and water availability to be active. But still, it is a profound and exciting finding and totally unexpected.’ 

Water activity, measured on a scale of 0 to 1, is equivalent to the relative humidity, or availability of water, in a planet’s atmosphere. 

The water activity of an environment can considerably affect organisms, including those that are capable of living in extreme environments, known as extremophiles. 

Laboratory studies have shown that life requires a water activity of at least 0.585 for metabolism and reproduction to take place.

The authors found droplets of sulphuric acid reduce the water activity of Venus’ clouds to below 0.004 – more than 100 times less than the limit for life. 

Illustration of stormy clouds on Jupiter, based on images from the Stellar Reference Unit camera of the Juno mission (NASA)

Illustration of stormy clouds on Jupiter, based on images from the Stellar Reference Unit camera of the Juno mission (NASA)

Illustration of stormy clouds on Jupiter, based on images from the Stellar Reference Unit camera of the Juno mission (NASA)

Researchers used temperature and pressure data taken from the Galileo Atmospheric Entry Probe (pictured). Galileo became the became first spacecraft to orbit Jupiter in 1995

Researchers used temperature and pressure data taken from the Galileo Atmospheric Entry Probe (pictured). Galileo became the became first spacecraft to orbit Jupiter in 1995

Researchers used temperature and pressure data taken from the Galileo Atmospheric Entry Probe (pictured). Galileo became the became first spacecraft to orbit Jupiter in 1995

In comparison, the representative water activity in Mars’ clouds is 0.537, which is slightly below the habitable range for life and similar to that of the second layer, or stratosphere, of the Earth’s atmosphere. 

The lowest atmospheric layer of Earth, the troposphere, is, however, permissible for life. 

Jupiter’s atmosphere has a ‘biologically permissive’ water activity of more than 0.585 for temperatures between 14°F and 104°F (-10°C and 40°C), although factors such as cloud composition may limit habitability.

‘We derive water activity of atmospheres without a model of any sort, based only in direct observations of pressure, temperature, and water concentration,’ said study co-author Professor Christopher P McKay at NASA.    

NASA's Galileo probe is depicted here in this artist's impression passing over one of Jupiter's moons

NASA's Galileo probe is depicted here in this artist's impression passing over one of Jupiter's moons

NASA’s Galileo probe is depicted here in this artist’s impression passing over one of Jupiter’s moons

Professor McKay said the findings for Venus were ‘unfortunate’ because he was ‘very interested in searching for life on other worlds’.  

‘It’s also unfortunate that our conclusions are based directly on measurements – it is not a model with assumptions so it is hard to imagine that the results will change as we do further exploration,’ he said. 

However, the researchers said the methods used in their study can also be used to determine water activity in the atmospheres of planets beyond the Solar System, and help narrow down the search for alien life.

The findings, published in Nature Astronomy, come after NASA and the European Space Agency recently announced three missions to Venus in the coming years.   

NASA announced its two new $500 million missions at the start of June, which will launch in the next 10 years to understand how Venus ‘became an inferno-like world’.

Just over a week later, the ESA said it will send a probe, known as EnVision, to study ‘Earth’s evil twin’, targeting a launch in the early 2030s. 

CARBON DIOXIDE AND SULPHURIC ACID DROPLETS FEATURE IN THE ATMOSPHERE OF VENUS

Venus’s atmosphere consists mainly of carbon dioxide, with clouds of sulphuric acid droplets. 

The thick atmosphere traps the sun’s heat, resulting in surface temperatures higher than 470°C (880°F).

The atmosphere has many layers with different temperatures. 

At the level where the clouds are, about 30 miles (50 km) up from the surface, it’s about the same temperature as on the surface of the Earth.

As Venus moves forward in its solar orbit while slowly rotating backwards on its axis, the top level of clouds zips around the planet every four Earth days.

They are driven by hurricane-force winds travelling at about 224 miles (360 km) per hour. 

Atmospheric lightning bursts light up these quick-moving clouds. 

Speeds within the clouds decrease with cloud height, and at the surface are estimated to be just a few miles (km) per hour.

On the ground, it would look like a very hazy, overcast day on Earth and the atmosphere is so heavy it would feel like you were one mile (1.6km) deep underwater.

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