In a paper published this week in the journal Astrobiology, researchers focused on the possible existence of the Earth-like phototrophy — the process by which energy from the Sun is captured and converted into chemical energy — in the clouds of Venus.“Our study provides tangible support for the potential for phototrophy and/or chemotrophy by microorganisms in Venus’ clouds,” said Professor Rakesh Mogul, a researcher in the Chemistry & Biochemistry Department at the California State Polytechnic University Pomona.
“The acidity and water activity levels potentially fall within an acceptable range for microbial growth on Earth, while the constant illumination with limited UV suggests that Venus’ clouds could be hospitable for life.”
“We believe that Venus’ clouds would make a great target for habitability or life detection missions, like those currently planned for Mars and Europa.”
According to the team, photosynthesis could occur round-the-clock in Venus’ clouds with the middle and lower clouds receiving solar energy similar to the Earth’s surface.
Much like on Earth, hypothetical phototrophs in Venus’ clouds would have access to solar energy during the day.
In a fascinating twist, Professor Mogul and colleagues found that photosynthesis may continue through the night due to thermal or infrared energy originating from the surface and the atmosphere.In this habitat, light energy would be available from both above and below the clouds, which could provide photosynthetic microorganisms ample opportunities to diversify across the cloud layers.
Both the solar and thermal radiation in Venus’ clouds possess wavelengths of light that can be absorbed by the photosynthetic pigments found on Earth.
The researchers found that after filtering through the Venusian atmosphere, scattering and absorption scrubs the sunlight of much of the ultraviolet radiation (UV) that is harmful to life, providing a benefit like Earth’s ozone layer.
Using a radiative transfer model, they showed that the present-day middle and lower cloud layers above Venus receive significantly less UV, 80-90% less flux in the UV-A when compared to Earth’s surface, and are essentially depleted of radiation in the UV-B and UV-C, which represent the most harmful components of the UV.
To gauge the nighttime photosynthetic potential via Venus’ thermal energy, they compared the photon fluxes rising from Venus’ hot atmosphere and surface to the photon fluxes measured within low-light phototrophic habitats on Earth: (i) hydrothermal vents in the East Pacific Rise, where geothermal emissions are reported to support phototrophy at depths of 2.4 km; and (ii) the Black Sea, where solar powered phototrophs are found at depths of 120 m.
These comparisons showed that photon fluxes from Venus’ atmosphere and surface exceed the fluxes measured in these low-light phototrophic environments on Earth.
While a recent study concluded that Venus’ clouds were too dry to support terrestrial life, Professor Mogul and co-authors found that the chemical conditions of Venus’ clouds could be partly composed of neutralized forms of sulfuric acid, such as ammonium bisulfate.
These chemical conditions would exhibit dramatically higher water activities when compared to the previous calculations and much lower acidities when compared to current models for Venus.
