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.
“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.
In the study published 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.
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. 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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