'Habitable' Exoplanets Might Not Be Very Earth-Like After All

One of the most exciting moments in exoplanet science came in late February, when NASA's Spitzer Space Telescope announced the discovery of seven rocky planets orbiting in or near the habitable zone of their parent star, TRAPPIST-1, which lies 40 light years away from Earth.

"The discovery sets a new record for greatest number of habitable-zone planets found around a single star outside our solar system," NASA said in a statement. "All of these seven planets could have liquid water — key to life as we know it — under the right atmospheric conditions, but the chances are highest with the three in the habitable zone."

Comparing the habitability of our own planet to the conditions on newly-discovered exoplanets, however, could be misleading, according to the authors of a commentary in the journal Nature Astronomy. They argue that even though scientists have found hundreds of Earth-sized planets, there is no available technology to show us if their surfaces are remotely Earth-like.

Lead author Elizabeth Tasker said the language used by NASA and others can be "unnecessary and dangerous," in the sense that the public could get overly hopeful that life exists on these other planets.

Tasker, who is an associate professor in the department of solar system science at the Japan Aerospace Exploration Agency, was not involved in the TRAPPIST-1 discovery.

Artist's impression of Gliese 832 c, which some scientists consider a potentially habitable exoplanet, shown to scale with Earth. The announcement of Gliese 832 c was an impeteus for a new paper that criticizes habitability metrics used by exoplanet scientists.

In studying the data, however, she noted that the team found that many of the planets orbit in resonant configurations, meaning that one planet's orbit is a direct ratio of another. In other words: The inner planet in the TRAPPIST-1 system, for example, orbits eight times in the period it takes the outer planet to orbit two.

Tasker said this probably suggests these worlds formed further out from the star and over the years, their mutual gravitational attraction pulled them in closer. "They may not be terrestrial planets, but maybe the cores of gas giants because they formed in a similar region to our own solar system," she said.

Tasker's interest in the habitability of new-found planets sprung from the announcement of Gliese 832c in 2014. In the scientific paper announcing the discovery of the planet, the authors cautioned that this "super-Earth" is more likely a "super-Venus" with a massive atmosphere. On Venus, the surface roasts at oven temperatures and can crush unprotected spacecraft in moments. Yet, Tasker said that many of the media stories fawned over Gliese 832c as a potentially habitable world.

Tasker said the oversimplification of comparing exoplanets to our own planet arises from something called the Earth similarity index. The index uses four parameters: the radius of the planet, the radius of Earth, the stellar flux (or radiation) of the exoplanet's star, and the solar flux of our own sun. This metric is used by entities such as the Planetary Habitability Laboratory at the University of Puerto Rico at Arecibo, which ranks planets on a habitability index.

"In practice, these [parameters] aren't independent," Tasker said. For example, the flux coming from the star gives equilibrium temperature, which is different from planetary surface temperature — and doesn't take into account how much radiation the planet receives, she said.

Read more at Discovery News