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Alien worlds might not have a night and day. How would that change evolution?

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Alien worlds might not have a night and day. How would that change evolution?

Getty Images Moon and sunlight over hill in Italy (Credit: Getty Images)Getty Images

Distinct days and nights have helped life flourish on Earth. But many alien worlds capable of supporting life may not have such clear delineations.

Do aliens sleep? You may take sleep for granted, but research suggests many planets that could evolve life don’t have a day-night cycle. It’s hard to imagine, but there are organisms living in Earth’s lightless habitats, deep underground or at the bottom of the sea, that give us an idea what alien life without a circadian rhythm may be like. 

There are billions of potentially habitable planets in our galaxy. How do we arrive at this number? The Milky Way has between 100 billion and 400 billion stars.

Seventy percent of these are tiny, cool red dwarfs, also known as M-dwarfs. A detailed exoplanet survey published in 2013 estimated that 41% of M-dwarf stars have a planet orbiting in their “Goldilocks” zone, the distance at which the planet has the right temperature to support liquid water.

These planets only have the potential to host liquid water, though. We don’t yet know if any of them actually do have water, much less life. Still, that comes to 28.7 billion planets in the Goldilocks zones of M-dwarfs alone. This is not even considering other types of stars like our own yellow Sun. 

Rocky planets orbiting in an M-dwarf’s habitable zone are called M-Earths. M-Earths differ from our Earth in fundamental ways. For one thing, because M-dwarf stars are much cooler than the Sun, they are close-in, which makes the gravitational pull of the star on the planet immensely strong.

Getty Images On Earth, the effect of sunlight fades as you head deeper into the ocean – yet the black depths support much life (Credit: Getty Images)Getty Images

On Earth, the effect of sunlight fades as you head deeper into the ocean – yet the black depths support much life (Credit: Getty Images)

The star’s gravity pulls harder on the near side of the planet than the far side, creating friction that resists and slows the planet’s spin over aeons until spin and orbit are synchronised. This means most M-Earths are probably tidally locked, which is when one hemisphere always faces the sun while the other always faces away.

A tidally locked planet’s year is the same length as its day. The Moon is tidally locked to the Earth, which is why we always see only one face of the Moon and never its far side.

A tidally locked planet may seem exotic, but most potentially habitable planets are probably like this. Our closest planetary neighbour, Proxima Centauri b (located in the Alpha Centauri system four light-years away), is probably a tidally locked M-Earth.

Unlike our Earth, then, M-Earths have no days, no nights and no seasons. But life on Earth, from bacteria to humans, has circadian rhythms tuned to the day-night cycle.

Sleep is only the most obvious of these. The circadian cycle affects biochemistry, body temperature, cell regeneration, behaviour and much more. For example, people who receive vaccinations in the morning develop more antibodies than those who receive them in the afternoon because the immune system’s responsiveness varies throughout the day.

Temperature variations caused by thermal vents, humidity fluctuations, and changes in environmental chemistry or currents can all trigger bio-oscillations in organisms

We don’t know for sure how important periods of inactivity and regeneration are to life. Maybe beings that evolved without cyclical time can just keep on chugging, never needing to rest.

To inform our speculation, we can look at organisms on Earth that thrive far from daylight, such as cave-dwellers, deep-sea life and microorganisms in dark environments like the Earth’s crust and the human body.

Getty Images The nearest Earth-like planet, Proxima Centauri b, is thought to be a tidally locked M-Earth, which may affect distinct days and nights (Credit: Getty Images)Getty Images

The nearest Earth-like planet, Proxima Centauri b, is thought to be a tidally locked M-Earth, which may affect distinct days and nights (Credit: Getty Images)

Temperature variations caused by thermal vents, humidity fluctuations and changes in environmental chemistry or currents can all trigger bio-oscillations in organisms. This hints that biorhythms have intrinsic benefits.

Recent research shows M-Earths could have cycles that replace days and seasons. To study questions like these, scientists have adapted climate models to simulate what the environment on an M-Earth would look like, including our neighbour Proxima Centauri b.

While the star remains fixed in the sky of these planets, the environment will be changing

In these simulations, the contrast between an M-Earth’s dayside and nightside seems to generate rapid jets of wind and atmospheric waves like those that cause Earth’s jet stream to bend and meander. If the planet has water, the dayside probably forms thick clouds full of lightning.

Interactions between winds, atmospheric waves and clouds may shift the climate between different states, causing regular cycles in temperature, humidity and rainfall. The lengths of these cycles will vary by planet from tens to hundreds of Earth days, but they won’t be related to its rotation period. While the star remains fixed in the sky of these planets, the environment will be changing.

Perhaps life on M-Earths would evolve biorhythms synchronised to these cycles. If a circadian clock organises internal biochemical oscillations, it may have to.

Or perhaps evolution would find a weirder solution. We could imagine species that live on the planet’s dayside and migrate to the nightside to rest and regenerate. A circadian clock in space instead of in time.

This thought should remind us that, if life exists out there, it will upend assumptions we didn’t know we had. The only certainty is that it will surprise us.

Maureen Cohen is a postdoctoral research associate in Venus global climate modelling at The Open University.

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