The conditions for life surviving on planets entirely covered in water are more fluid than previously thought, opening up the possibility that water worlds could be habitable, according to a study.
Scientists have assumed that planets covered in a deep ocean would not support the cycling of minerals and gases that keeps the climate stable on Earth, and thus would not be friendly to life.
The study, published in The Astrophysical Journal, found that ocean planets could stay in the “sweet spot” for habitability much longer than previously assumed.
The researchers from the University of Chicago and Pennsylvania State University in the US based their findings on more than a thousand simulations.
“This really pushes back against the idea you need an Earth clone – that is, a planet with some land and a shallow ocean,” said Edwin Kite, an assistant professor at UChicago.
As telescopes get better, scientists are finding more and more planets orbiting stars in other solar systems.
Such discoveries are resulting in new research into how life could potentially survive on other planets, some of which are very different from Earth – some may be covered entirely in water hundreds of miles deep.
A newly discovered planet orbiting a nearby star could be the closest world to Earth providing a comfortable home for life. The Earth-sized planet, named Ross 128b, is just 11 light years away. Since life needs an extended period to evolve, and because the light and heat on planets can change as their stars age, scientists usually look for planets that have both some water and some way to keep their climates stable over time.
Kite, and Eric Ford from Penn State set up a simulation with thousands of randomly generated planets, and tracked the evolution of their climates over billions of years.
“The surprise was that many of them stay stable for more than a billion years, just by luck of the draw,” Kite said.
“Our best guess is that it’s on the order of 10 per cent of them,” he said. These lucky planets sit in the right location around their stars.
They happened to have the right amount of carbon present, and they do not have too many minerals and elements from the crust dissolved in the oceans that would pull carbon out of the atmosphere, researchers said.
They have enough water from the start, and they cycle carbon between the atmosphere and ocean only, which in the right concentrations is sufficient to keep things stable.
“How much time a planet has is basically dependent on carbon dioxide and how it’s partitioned between the ocean, atmosphere and rocks in its early years,” said Kite.
“It does seem there is a way to keep a planet habitable long-term without the geochemical cycling we see on Earth,” he said.
The simulations assumed stars that are like our own, but the results are optimistic for red dwarf stars, too, Kite said.
Exoplanets with water, University of Chicago, solar systems, minerals, Pennsylvania State University, planets with water, dwarf stars, planet climates, oceans, planet simulations >