Earth’s ‘next door neighbor’ could be home to WATER: New simulations suggest planet just outside of our solar system may be a ‘highly habitable’ world with a liquid ocean
- Proxima b orbits the nearby red dwarf Proxima Centauri just 4.2 light-years away
- Exoplanet sits within habitable zone of its star, suggesting it could support life
- Study suggests it could support liquid water at the surface in a dynamic ocean
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A nearby exoplanet orbiting within the habitable zone of a star just 4.2 light-years from Earth may be home to a vast ocean, boosting its chances of supporting life.
Since its discovery, questions about the conditions at the surface of Proxima b have been swirling; the planet’s mass is just about 1.3 times that of Earth’s, and the red dwarf star it circles is similar in age to our sun.
Studies over the last few years, however, have both bolstered hopes of its habitability and shot them down.
Now, a new study has once again raised the possibility that Proxima b could support life, suggesting that under the right conditions, the exoplanet could sustain liquid water.
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Since its discovery, questions about the conditions at the surface of Proxima b have been swirling; the planet’s mass is just about 1.3 times that of Earth’s, and the red dwarf star it circles is similar in age to our sun. Artist’s impression
‘The major message from our simulations is that there’s a decent chance that the planet would be habitable,’ Anthony Del Genio, a planetary scientist at the NASA Goddard Institute for Space Studies, told LiveScience.
In the study published this month in the journal Astrobiology, the researchers ran what are said to be the first climate simulations of Proxima b with a dynamic ocean.
The planet is thought to be tidally locked with its star, Proxima Centauri, meaning it would have a permanent ‘dayside’ and ‘nightside.’
While any water on the side left in the dark would be frozen, that’s not necessarily the case for the other side.
‘Climate models with static oceans suggest that Proxima b could harbor a small dayside surface ocean despite its weak instellation,’ the researchers explain in the new study.
With a dynamic (moving) ocean considered for the first time, the extent of this liquid water becomes much more significant, in some cases even dipping into parts of the nightside.
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The simulations showed that ‘with a dynamic ocean, a hypothetical ocean-covered Proxima Centauri b with an atmosphere similar to modern Earth’s can have a habitable climate with a broad region of open ocean, extending to the nightside at low latitudes.’
The researchers modelled for different salinity levels and atmospheric greenhouse gas concentrations as well, each of which could play into the size of the liquid regions.
Proxima b orbits the red dwarf Proxima Centauri, which is part of a triple system including the binary pair Alpha Centauri A and B. An artist’s impression is pictured
WHAT MAKES PROXIMA B UNIQUE?
Distance: This is the closest Earth-like planet we could ever find.
Orbiting our nearest star, the planet is only four light years away.
Missions to send spacecraft to the planet to examine for signs of life are already in planning, and could happen within decades.
Composition: The planet is rocky and a similar size to Earth.
Temperature: It lies in the ‘habitable zone’ of its star, which means there could be liquid water on its surface – a key ingredient for alien life.
The temperature on the surface of the planet could be between -90° and 30° Celsius (-130 and 86 Fahrenheit).
Atmosphere: If Proxima b has an atmosphere, the simple ingredients – water, carbon dioxide, and rock – that are needed for the formation of biochemical cycles that we call life, could all be present and interacting on the planet’s surface.
In more than a dozen simulations, the team found the exoplanet almost always had some sort of liquid ocean.
But, don’t get excited to take a dip just yet.
‘We find that an ocean-covered Proxima b could have a much broader area of surface liquid water but at much colder temperatures than previously suggested, due to ocean heat transport and/or depression of the freezing point by salinity,’ the researchers wrote.
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