{"id":22070,"date":"2022-01-07T10:31:23","date_gmt":"2022-01-07T04:46:23","guid":{"rendered":"https:\/\/www.revoscience.com\/en\/?p=22070"},"modified":"2022-01-07T10:31:27","modified_gmt":"2022-01-07T04:46:27","slug":"life-could-be-thriving-in-the-clouds-of-venus","status":"publish","type":"post","link":"https:\/\/www.revoscience.com\/en\/life-could-be-thriving-in-the-clouds-of-venus\/","title":{"rendered":"Life could be thriving in the clouds of Venus"},"content":{"rendered":"\n BY ERIC VERBETEN <\/strong>\n\n\n\n

MADISON \u2014 Is there life on Venus? For more than a century, scientists have pondered this question. Now, there is renewed interest in Venus as a place that could support living organisms.<\/p>\n\n\n\n

\u201cWe are trying to make the case for exploring Venus and to inspire and inform future missions to collect in situ data with satellites,\u201d says Sanjay Limaye, a University of Wisconsin\u2013Madison Space Science and Engineering Center scientist and co-author of a recent collection of papers on Venus that he hopes will do just that.<\/p>\n\n\n\n

Limaye is an expert on Venus. With more than 45 years of research behind him, he continues to investigate the planet\u2019s dense atmosphere. \u201cAs one of our closest neighbors it is easier to reach Venus compared to other bodies like Titan, Enceladus, or even Mars,\u201d he says.<\/p>\n\n\n\n

Published in 2021 in the journal Astrobiology, the series of articles target Venus as a potential home for microbial life like bacteria and other organisms. The collection emerged from the 2019 Venera-D Venus Cloud Habitability workshop, which convened more than 50 scientists in Moscow to examine existing research and understand the planet\u2019s potential to support life billions of years ago \u2014 and today.<\/p>\n\n\n\n

Formed around the same time as Earth, about 4.5 billion years ago, Venus occupies an orbit between Mercury and Earth. The planet rotates very slowly on its axis, taking 243 Earth days to complete a single rotation. Its massive atmosphere of mostly carbon dioxide makes it a planet of extremes, with scorching temperatures, intense winds, and volcanic activity.<\/p>\n\n\n\n

\"\"<\/figure>\n\n\n\n

Despite the features that make the planet\u2019s surface inhospitable, its thick global cloud cover may present gentler conditions for some microbial life forms due to the availability of sunlight, nutrients, and some water \u2014 all of which can create narrow but habitable zones like those theorized to exist high in the atmosphere.<\/p>\n\n\n\n

The Astrobiology series investigates these aspects and presents reasons to explore whether life may be present, perhaps hidden throughout the planet\u2019s complex clouds. It explores Venus\u2019 history as a potentially life-bearing planet, its habitable zones, and potential signatures of organisms that use light as an energy source.<\/p>\n\n\n\n

Early formation and water<\/strong><\/p>\n\n\n\n

Venus was not always the pressure cooker it is today. Like Earth, its environment included volcanic activity and liquid water oceans. For nearly 3 billion years these thermal vents and oceans could have harbored microorganisms. But that oasis was lost.<\/p>\n\n\n\n

\u201cWhen life began on Earth the conditions on Venus were likely similar,\u201d says Limaye. \u201cSome modeling suggests water could have existed for 1 billion to 3 billion years.\u201d<\/p>\n\n\n\n

In these early days, the sun was dimmer but more intense, radiating the planets with high-energy particles and ultraviolet rays. Around 3.5 billion years after its formation, Venus began to heat up, and over the course of millions of years, its oceans evaporated. With its atmosphere of carbon dioxide and water vapor, a runaway greenhouse effect trapped more of the sun\u2019s energy, creating the planet\u2019s modern dense and hot atmosphere. Venus\u2019 surface pressures are more than 90 times those of Earth, with surface temperatures exceeding 486 degrees Celsius (906 degrees Fahrenheit) \u2014 hot enough to melt lead.<\/p>\n\n\n\n

While these conditions are inhospitable to most life on Earth, small and hardy microorganisms known as extremophiles have extraordinary abilities to survive in the worst imaginable places. It is possible, researchers say, that these ancient organisms adapted to the changing conditions on Venus and eventually found a new home within its thick atmosphere.<\/p>\n\n\n\n

Scientists are skeptical that fossil remains exist on the Venusian surface due to continuous and destructive volcanic activity. However, satellites orbiting the planet offer deep glimpses into its atmosphere and have presented clues of potential life drifting throughout narrow pockets aloft in the Venusian sky.<\/p>\n\n\n\n

Atmospheric mysteries<\/strong><\/p>\n\n\n\n

Since the 1960s, dozens of space missions have examined Venus from all angles. The Pioneer Venus Orbiter and Multiprobe missions in 1978 gave scientists an in-depth look at the top of the atmosphere and through its many layers down to the surface.<\/p>\n\n\n\n

In 1981 the Venera 13 and 14 missions sent back several color panoramas of the surface, information about its clouds and soil, and the first-ever recording of winds on the planet\u2019s surface.<\/p>\n\n\n\n

A few years later, VeGa 1 and VeGa 2 balloons and landers recorded more information about the atmosphere, clouds, winds, and the planet\u2019s surface composition.<\/p>\n\n\n\n

Researchers have also gathered spectral data from Venus, or measurements of how much light is either reflected or absorbed by the planet. Using these data, they can identify chemical signatures such as carbon dioxide, sulfur dioxide and even trace amounts of water vapor.<\/p>\n\n\n\n

Some of Venus\u2019 spectral data reveal prominent and inexplicable dark patches in its cloud layers, showing areas of strong absorption. Limaye and colleagues have contemplated whether microorganisms could be the source of that solar energy absorption, much like the algal patches in Earth\u2019s oceans or lakes \u2014 especially given the presence of trace water, energy, and nutrients like carbon, hydrogen, nitrogen, phosphorous, and sulfur in the clouds.<\/p>\n\n\n\n

\u201cVenus has a potential to harbor conditions for iron- and sulfur-centered metabolism,\u201d says Limaye. \u201cTogether, our lines of reasoning suggest that particles in Venus\u2019 lower clouds contain sufficient mass balance to support microorganisms, water, and solutes, and potentially sufficient biomass to be detected by optical methods.\u201d<\/p>\n\n\n\n

The researchers assert that, as the planet\u2019s surface became more inhospitable, microorganisms may have migrated to calmer and less extreme conditions in Venus\u2019 atmosphere. This could explain why microorganisms may be drifting.<\/p>\n\n\n\n

Atmospheric pressures at 48 to 70 kilometers, or 30 to 43 miles, above the planet\u2019s surface are similar to Earth\u2019s, and Venus\u2019 thick clouds reduce some of the sun\u2019s damaging ultraviolet radiation, creating milder conditions. Extremophiles on Earth have been found to withstand, and even thrive, in similar conditions.<\/p>\n\n\n\n

\u201cIt\u2019s not impossible these microorganisms could have migrated to the clouds and sustained life,\u201d says Limaye.<\/p>\n\n\n\n

The peculiar absorption data has compelled researchers to look more closely at what could produce these signatures, which go beyond common atmospheric and chemical reactions.<\/p>\n\n\n\n

Harvesting light, harboring life<\/strong><\/p>\n\n\n\n

Planetary atmospheres serve many functions, including the filtration of dangerous radiation. On Earth, the atmosphere (and magnetic field) blocks much of the sun\u2019s harmful rays. Plantlife thrives on weaker forms of ultraviolet light that provide fuel for photosynthesis.<\/p>\n\n\n\n

Limaye and colleagues believe Venus\u2019 atmosphere is capable of producing similarly balanced zones. In one study, he and his co-authors showed that the Venusian atmosphere might be able to support phototrophy, or the ability of organisms to harness sunlight for energy.<\/p>\n\n\n\n

\u201cSolar irradiances calculated across Venus\u2019 clouds support the potential for Earth-like phototrophy,\u201d says Limaye, who also adds that the planet\u2019s clouds demonstrate the ability to neutralize harmful gases such as sulfuric acid.<\/p>\n\n\n\n

The planet, Limaye says, also experiences limited ultraviolet flux in the middle and lower clouds, further reinforcing its potential to harbor life. And salt present in cloud droplets may help reduce their acidity, making the droplets more hospitable.<\/p>\n\n\n\n

\u201cThroughout this series of papers, we focus on finding similar conditions on Earth where we know life thrives, but this isn\u2019t the only approach,\u201d says Limaye. \u201cThe search for life is not limited to microbes as we know them on Earth, but there are many possibilities of extremophiles existing and thriving in ways we haven\u2019t imagined.\u201d<\/p>\n\n\n\n

Future missions<\/strong><\/p>\n\n\n\n

Since the 1960s, scientists have launched nearly 50 missions of varying success to study our neighboring planet. The next decade will herald seven missions to explore Venus and uncover its atmospheric and surface mysteries.<\/p>\n\n\n\n

Rocket Labs announced a small probe to look for phosphine, launching in 2023. The India Space Research Organization Venus orbiter is expected to carry radars and is anticipated to arrive around 2026, followed by NASA\u2019s VERITAS radar orbiter in 2027. Launching in 2028, NASA\u2019s DAVINCI mission will feature a dual-purpose spacecraft to collect atmospheric measurements from orbit, in tandem with an atmospheric probe that will sift through the dense atmosphere, collecting data during its descent.<\/p>\n\n\n\n

The Venera-D mission by the Russian Roscosmos State Corporation for Space Activities, proposed for 2029, will deploy an orbiter and lander designed to withstand the harsh conditions on the planet\u2019s surface and collect valuable atmospheric and ground measurements. It will also include a long-lived small lander contributed by NASA. The decade of exploration will end with the European Space Agency\u2019s EnVIsion Radar orbiter, also with contributions from NASA.<\/p>\n\n\n\n

Limaye is encouraged that these future missions will ultimately answer many of the observed mysteries on a planet long considered hostile to life. And with additional workshops, such as the Venera-D: Venus Cloud Habitability System Workshop convened in November 2021, researchers around the world continue the conversation about whether there is life on Venus.<\/p>\n","protected":false},"excerpt":{"rendered":"

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