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. 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.