Skip to main content

Thank you for visiting You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

Tidal heating shrinks the 'goldilocks zone'

Overlooked factor suggests fewer habitable planets than thought.

Planets orbiting close to M-class dwarf stars may experience too much tidal heating to be able to maintain liquid water. Credit: NASA, ESA, and D. Aguilar (Harvard-Smithsonian Center for Astrophysics)

A previously little-considered heating effect could shrink estimates of the habitable zone of the Milky Way’s most numerous class of stars — ‘M’ or red dwarfs — by up to one half, says Rory Barnes, an astrobiologist at the University of Washington in Seattle. That factor — gravitational heating via tides — suggests a menagerie of previously undreamt-of planets, on which tidal heating is a major source of internal heat. Barnes presented the work yesterday at a meeting of the American Astronomical Society’s Division on Dynamical Astronomy in Timberline Lodge, Oregon.

The habitable zone is the orbital region close enough to a star for a planet to have liquid water, but not so close that all of the water evaporates. For our Sun, the zone extends roughly from the inner edge of the orbit of Mars to the outer edge of that of Venus. For smaller, cooler stars, such as M-class dwarfs, the zone can be considerably closer to the star than Mercury is to the Sun. And because close-in planets are easier to spot than more distant ones, such stars have been a major target for planet hunters seeking Earth-like worlds.

There's just one problem with finding habitable planets around such stars, says Barnes. Because tidal forces vary dramatically with the distance between a planet and its star, closer orbits also result in massively larger tidal forces.

Since planets do not have perfectly circular orbits, these tidal forces cause the planet to flex and unflex each time it moves closer to or further from its star; kneading its interior to produce massive quantities of frictional heat. Substantial heat can be produced, he added, with even slight deviations from a perfectly circular orbit. And, Barnes notes, other factors — such as the rate of the planet's rotation and its axial tilt — can also influence heat production.

A similar tidal process makes Jupiter's moon Io the most volcanic body in the Solar System. "I’m just scaling that Io–Jupiter system up by a factor of 1,000 in mass," Barnes said at the meeting. "It's the same process, on steroids."

Hot effects

Barnes added that this process can also change a planet's orbit, making it more circular. This would reduce the amount of heat being generated. But even if a planet winds up in a near-circular orbit, Barnes says, his calculations show that it could easily have already undergone enough heating to lose all of its water into space. "Terrestrial planets can be permanently sterilized," he said.

Such planets could also wind up in what is thought to be the habitable zone, looking to exoplanet hunters like Earth-like worlds. "It sounds like what we're looking for," he said. "But is it an Earth twin, or a 'habitable-zone' Venus?"

For the smallest red dwarfs, Barnes added, tidal heating could reduce the habitable zone by about 50% of present estimates, but brighter suns have farther-flung habitable zones where this is no longer an important factor. "At one-quarter of solar mass, the effect goes away," Barnes says.

But even for planets not ‘sterilized’ by the process, there can be major effects. "This is a source of energy that doesn’t exist on Earth," he says.

If the effect is strong, it could produce a planet-sized Io. Or, if the planet would otherwise be frozen, tidal heating could maintain a liquid ocean beneath a planet-girdling ice cap, like a planet-sized version of Jupiter's moon Europa, which has an ocean beneath a thick layer of ice, kept liquid by tidal heat.

"Nobody's put serious work into this before," says Douglas Hamilton, an astronomer at the University of Maryland in College Park.

The next step, adds Sylvio Ferraz Mello, an astronomer at the University of Sao Paulo, Brazil, is to look at the geological consequences of comparatively mild tidal heating on otherwise Earth-like worlds — a factor that could have unknown, but possibly major ramifications for plate tectonics.

Hamilton warns, however, that his findings are still theoretical. And even if there are ways to determine whether a terrestrial planet circling in the habitable zone of an M-class star is an Earth twin or a tidal Venus, he adds, "that's well beyond any [space telescope] missions we have on the drawing board."


Related links

Related links

Related links in Nature Research

Planetary science: In search of biosignatures 2012-Feb-29

Three tiny exoplanets suggest Solar System not so special 2012-Jan-11

Kepler scores potentially habitable planet 2011-Dec-05

Related external links

Rory Barnes

Rights and permissions

Reprints and Permissions

About this article

Cite this article

Lovett, R. Tidal heating shrinks the 'goldilocks zone'. Nature (2012).

Download citation

  • Published:

  • DOI:


Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing