Astronomers have created a “habitability index” to compare and rank exoplanets to help prioritize which of the thousands discovered warrant close inspection in the search for life beyond Earth.
“Basically, we’ve devised a way to take all the observational data that are available and develop a prioritization scheme,” says Rory Barnes, professor of astronomy at the University of Washington, “so that as we move into a time when there are hundreds of targets available, we might be able to say, ‘OK, that’s the one we want to start with.'”
The Kepler Space Telescope has allowed astronomers to detect thousands of exoplanets—those beyond our solar system—far more than can be investigated one by one. The James Webb Space Telescope, set for launch in 2018, will vastly enhance the search for life by actually measuring the atmospheric composition of a rocky, possibly Earthlike planet far off in space.
Astronomers detect some planets when they “transit” or pass in front of their host star, thus blocking some of the light. The Transiting Exoplanet Survey Satellite, or TESS, is scheduled to launch in 2017 and will find many more worlds in this way. But it’s the Webb telescope and its “transit transmission spectroscopy” that will really be able to study planets closely to hunt for life.
But access to such telescopes is expensive and the work is methodical and time-consuming. The new index is a tool to help fellow astronomers decide which worlds might have a better chance of hosting life, and are worthy of their limited resources.
Traditionally, astronomers have focused the search by looking for planets in their star’s “habitable zone”—more informally called the “Goldilocks zone” —which is the swath of space that’s “just right” to allow an orbiting Earth-like planet to have liquid water on its surface, perhaps giving life a chance. But so far that has been just a sort of binary designation, indicating only whether a planet is, or is not, within that area considered right for life.
“That was a great first step, but it doesn’t make any distinctions within the habitable zone,” Barnes says. “Now it’s as if Goldilocks has hundreds of bowls of porridge to choose from.”
The habitability index is more nuanced, producing a continuum of values that astronomers can punch into a Virtual Planetary Laboratory Web form to arrive at the single-number habitability index, representing the probability that a planet can maintain liquid water at its surface.
To create the index, researchers factored in estimates of a planet’s rockiness because rocky planets are the more Earth-like. They also accounted for “eccentricity-albedo degeneracy,” which comments on a sort of balancing act between the a planet’s albedo—the energy reflected back to space from its surface—and the circularity of its orbit, which affects how much energy it receives from its host star.
The two counteract each other. The higher a planet’s albedo, the more light and energy are reflected off to space, leaving less at the surface to warm the world and aid possible life. But the more noncircular or eccentric a planet’s orbit, the more intense is the energy it gets when passing close to its star in its elliptic journey.
A life-friendly energy equilibrium for a planet near the inner edge of the habitable zone—in danger of being too hot for life—would be a higher albedo, to cool the world by reflecting some of that heat into space, Barnes says. Conversely, a planet near the cool outer edge of the habitable zone would perhaps need a higher level of orbital eccentricity to provide the energy needed for life.
The researchers ranked planets found by the Kepler Space Telescope, in its original mission and its “K2” follow-up mission. The best candidates for habitability and life are those planets that get about 60 percent to 90 percent of the solar radiation that the Earth receives from the sun, which is in keeping with current thinking about a star’s habitable zone.
“This innovative step allows us to move beyond the two-dimensional habitable zone concept to generate a flexible framework for prioritization that can include multiple observable characteristics and factors that affect planetary habitability,” says Victoria Meadows, professor of astronomy. “The power of the habitability index will grow as we learn more about exoplanets from both observations and theory.”
Published in the Astrophysical Journal, the research is part of the ongoing work of the Virtual Planetary Laboratory to study faraway planets in the ongoing search for life. The NASA Astrobiology Institute funded the work.
Source: University of Washington