Eight times the mass of Earth and twice as big, K2-18b orbits in its star’s “habitable zone” at a distance — neither too far nor too close — where water can exist in liquid form, they reported in the journal Nature Astronomy. Water vapors found in the habitable zone of exoplanet’s atmosphere
We have discovered water for the first time in the atmosphere of an exoplanet with Earth-like temperatures that could support life as we know it, scientists revealed Wednesday.
Eight times the mass of Earth and twice as big, K2-18b orbits in its star’s “habitable zone” at a distance — neither too far nor too close — where water can exist in liquid form, they reported in the journal Nature Astronomy.
“This planet is the best candidate we have outside our solar system” in the search for signs of life, co-author Giovanna Tinetti, an astronomer at University College London, told AFP. Water vapors found in the habitable zone of exoplanet’s atmosphere
“We cannot assume that it has oceans on the surface but it is a real possibility.” Of the over 4,000 exoplanets detected to date, this is the first known to combine a rocky surface and an atmosphere with water.
Most exoplanets with atmospheres are giant balls of gas, and the handful of rocky planets for which data is available to seem to have no atmosphere at all.
Even if they did, most Earth-like planets are too far from their stars to have liquid water or so close that any H2O has evaporated.
Discovered in 2015, K2-18b is one hundred of so-called “super-Earths” — planets with less than ten times the mass of ours — spotted by NASA’s Kepler spacecraft.
We expect future space missions to detect hundreds more in the coming decades.
“Finding water in a potentially habitable world other than Earth is exciting,” said lead-author Angelos Tsiaras, also from UCL.
“K2-18b is not ‘Earth 2.0’,” he said. “However, it brings us closer to answering the fundamental question: is the Earth unique?” Working with spectroscopic data captured in 2016 and 2017 by the Hubble Space Telescope, Tsiaras and his team used open-source algorithms to analyze the starlight filtered through K2-18b’s atmosphere.
They found the unmistakable signature of water vapor. Exactly how much remains uncertain, but computer modeling suggested concentrations between 0.1 and 50 percent.
By comparison, the percentage of water vapor in Earth’s atmosphere varies between 0.2 percent above the poles and up to four percent in the tropics.
There was also evidence of hydrogen and helium. Nitrogen and methane may also be present but with current technology remain undetectable, the study said.
Further research will determine the extent of cloud coverage and the percentage of water in the atmosphere.
Water is crucial in the search for life, in part because it carries oxygen.
“Life, as we know, is based on water,” said Tinetti.
K2-18b orbits a red dwarf star about 110 light-years distant — a million billion kilometers — in the Leo constellation of the Milky Way and is probably bombarded by more destructive radiation than Earth.
“It is likely that this is the first of many discoveries of potentially habitable planets,” said UCL astronomer Ingo Waldmann, also a co-author.
“This is not only because super-Earths like K2-18b are the most common planets in our galaxy, but also because red dwarfs — stars smaller than our Sun — are the most common stars.” The new generation of space-based star gazing instruments led by the James Webb Space Telescope and the European Space Agency’s ARIEL mission will describe exoplanet atmospheres in far greater detail.
ARIEL, slated for a 2028 launch, will canvas some 1,000 planets, a large enough sampling to look for patterns and identify outliers.
“Over 4,000 exoplanets have been detected but we know little about their composition and nature,” said Tinetti. “By observing a large sample of planets, we hope to reveal secrets about their chemistry, formation, and evolution.”
(we have published This story from a wire agency feed without modifications to the text. Only the headline has been changed.)