Star Light Simulator illuminates the search for life around the Milky Way’s most common stars
Italian researchers have demonstrated experimentally for the first time that microorganisms can photosynthesise using the infrared-dominated light emitted by the most common type of star in the Milky Way. The results from the Star Light Simulator, presented at the Europlanet Science Congress (EPSC) 2022, suggest that life could develop around stars different from our Sun and produce oxygen-rich worlds that are habitable by more complex organisms.
Most stars in our Milky Way are the smallest type of hydrogen-burning star, known as red M-dwarfs. They are cooler and less luminous than our Sun and primarily emit light in the infrared and far-infrared, with very low emissions at visible wavelengths. Due to their abundance, many exoplanets have been found around M-dwarfs. However, whether or not these planets could support life has been the subject of much debate in recent years.
The Star Light Simulator, built by a collaboration of teams from the National Institute for Astrophysics (INAF), the Institute of Photonics and Nanotechnology (IFN-CNR) and the Department of Biology in Padua, can generate light intensities and spectra at different ranges to reproduce the light for any star. For this experimental setup, the team recreated the emitted light from an M-dwarf along with an atmospheric simulator chamber that replicated an artificial planetary environment.
“We initially focused on cyanobacteria since they have extraordinary capacities to withstand every environment on the Earth, as well as a known ability to survive in near-infrared light,” said Prof Nicoletta La Rocca of the University of Padua, who led the study. “When these acclimatised to the simulated environment, we extended our tests to mosses and various types of red and green microalgae.”
All the experiments were successful, with all the microrganisms demonstrating that they could grow and photosynthesise under M-dwarf light.
Prof La Rocca commented: “Life as we know it depends on liquid water, so that is one of the major criteria for an exoplanet to be considered to be habitable. More complex terrestrial life forms also depend on oxygen. On Earth, photosynthesising cyanobacteria played a vital role in oxidising our atmosphere. The new experimental results extend our knowledge of potentially habitable environments and hence, where we might expect to find a planet harbouring complex life.”
The results have been submitted for publication in a special issue of the open-access Life journal in the special issue “Frontiers in Extremophiles: From Life at Edges on Earth to Space Exploration”.
La Rocca, N., Battistuzzi, M., Claudi, R., Cocola, L., and Poletto, L.: Responses of eukaryotic photosynthetic organisms to simulated M-dwarf star light. , Europlanet Science Congress 2022, Granada, Spain, 18–23 Sep 2022, EPSC2022-495, 2022.
The Star Light Simulator (left) and illuminated (right). It has 25 channelt total, emitting light from 365 nanometres (UV light) to 940 nanometres (infrared light). Credit: La Rocca et al.
Prof Nicoletta La Rocca
Department of Biology
University of Padua
EPSC2022 Press Office
+44 7756 034243
About the Europlanet Science Congress (EPSC)
The Europlanet Science Congress (https://www.epsc2022.eu/) formerly the European Planetary Science Congress, is the annual meeting of the Europlanet Society. With a track record of 16 years, and regularly attracting around 1000 participants, EPSC is the largest planetary science meeting in Europe. It covers the entire range of planetary sciences with an extensive mix of talks, workshops and poster sessions, as well as providing a unique space for networking and exchanges of experiences.
Since 2005, Europlanet (www.europlanet-society.org) has provided Europe’s planetary science community with a platform to exchange ideas and personnel, share research tools, data and facilities, define key science goals for the future, and engage stakeholders, policy makers and European citizens with planetary science.
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