A newly published study from the Harvard-Smithsonian Center for Astrophysics reveals that UV light may have played a critical role in the emergence of life on Earth and could be a key for where to look for life elsewhere in the Universe.
A new study by Sukrit Ranjan of the Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, Massachusetts, and colleagues suggests that red dwarf stars might not emit enough UV light to kick-start the biological processes most familiar to our planet. For example, certain levels of UV might be necessary for the formation of ribonucleic acid, a molecule necessary for all forms of known life.
“It would be like having a pile of wood and kindling and wanting to light a fire, but not having a match,” said Ranjan. “Our research shows that the right amount of UV light might be one of the matches that gets life as we know it to ignite.”
This research is focused on the study of red dwarf stars, which are smaller and less massive than the Sun, and the planets that orbit them. Recently, several planetary systems with potential habitable zones, where liquid water could exist, have been discovered around red dwarfs including Proxima Centauri, TRAPPIST-1, and LHS 1140.
Using computer models and the known properties of red dwarfs, the authors estimate that the surface of rocky planets in the potentially habitable zones around red dwarfs would experience 100 to 1,000 times less of the ultraviolet light that may be important to the emergence of life than the young Earth would have. The chemistry that depends on UV light might shut down at such low levels, and even if it does proceed, it could operate at a much slower rate than on the young Earth, possibly delaying the advent of life.
“It may be a matter of finding the sweet spot,” said co-author Robin Wordsworth of the Harvard School of Engineering and Applied Science. “There needs to be enough ultraviolet light to trigger the formation of life, but not so much that it erodes and removes the planet’s atmosphere.”
Previous studies have shown that the red dwarf stars in systems such as TRAPPIST-1 may erupt with dramatic flares in UV. If the flares deliver too much energy, they might severely damage the atmosphere and harm life on surrounding planets. On the other hand, these UV flares may provide enough energy to compensate for the lower levels of UV light steadily produced by the star.
“We still have a lot of work to do in the laboratory and elsewhere to determine how factors, including UV, play into the question of life,” said co-author Dimitar Sasselov, also of the CfA. “Also, we need to determine whether life can form at much lower UV levels than we experience here on Earth.”
There is intense interest in probing these questions because red dwarf stars provide some of the most compelling candidates for detecting putative planets with life, including those mentioned above. As telescopes such as the James Webb Space Telescope and the Giant Magellan Telescope come online in coming years, scientists need the most information possible to pick out the best targets in their search for life outside our Solar System.
One limitation of these studies is that we know only one example where life formed on a planet, the Earth, and even here we are not certain exactly how life emerged. If life is found on a red dwarf’s planet, it might imply a pathway to the origin of life that is very different from what we think might have played out on Earth.
These results were published in the July 10th, 2017 issue of The Astrophysical Journal.
Reference: “The Surface UV Environment on Planets Orbiting M-Dwarfs: Implications for Prebiotic Chemistry & Need for Experimental Follow-Up” by Sukrit Ranjan, Robin Wordsworth and Dimitar D. Sasselov, 11 July 2017, The Astrophysical Journal.
DOI: 10.3847/1538-4357/aa773e
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