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Thinking outside the Goldilocks zone: Earth scientists reimagine the sweet spot for habitable planets.

Just how fantastical a planet can be and still support recognizable life isn't just a question for science fiction. Astronomers are searching the stars for otherworldly inhabitants, and they need a road map. Which planets are most likely to harbor life? That's where geoscientists' imaginations come in. Applying their knowledge of how our world works and what allows life to flourish, they are envisioning what kind of other planetary configurations could sustain thriving biospheres.

You don't necessarily need an Earth-like planet to support Earth-like life, new research suggests. For decades, thinking about the best way to search for extraterrestrials has centered on a "Goldilocks" zone where temperatures are "just right" for liquid water, a key ingredient for life, to wet the surface of an Earth doppelganger. But now it's time to think outside the Goldilocks zone, some scientists say. Unearthly mechanisms could keep greenhouse gas levels in check and warm planets in the coldest outer reaches of a solar system. Life itself could even play a starring role in a planet's enduring habitability.

"It's an exciting time," says Harvard planetary scientist Robin Wordsworth. "There's still a ton for us to learn about the way different planets behave. The Goldilocks zone is just a very rough guide, and we need to keep an open mind."

Currency of life

When it comes to habitable planets, water continues to be the currency of life. Too close to a star and all the water on a planet evaporates; too far and the planet is an icy snowball. The Goldilocks zone marks the region between those two extremes, where water can stay liquid. Every known organism requires liquid water at some point during its life cycle. Extraterrestrial life could be completely unlike anything seen on Earth, of course, but "we've got to start looking somewhere," says Colin Goldblatt, a planetary scientist at the University of Victoria in Canada. "At least we know what Earth life looks like."

With the assumption that water is king, astronomers search for wet planets using powerful telescopes (see Page 32). The search is limited by what the telescopes can see in a planet's atmosphere, however. Life-supporting liquid water could hide under the surface, for example, inside Jupiter's icy moon Europa (SN: 10/4/14, p. 10). And any subterranean life, which typically wouldn't alter the atmosphere, would probably be undetectable. Even with rovers roaming Mars, scientists can't tell for certain whether Martian groundwater hosts life (SN: 12/26/15, p. 26). For alien life to be observable from afar, liquid water would have to be at the surface, not just concealed belowground.

With liquid surface water as a must-have for hunting extraterrestrials, astronomers estimated the extent of the habitable region more than 50 years ago. Early research confined the Goldilocks zone for our own solar system to a narrow band--one estimate placed it from 0.95 times to 1.01 times Earth's average distance from the sun. But then scientists realized the surprising influence of Earth's built-in temperature control system: the carbon cycle, the process by which carbon travels from the atmosphere into the Earth and back out to the atmosphere.

The carbon cycle controls how much heat-trapping carbon dioxide is in the atmosphere. Rainfall weathers exposed rocks, causing a chemical reaction that pulls C[O.sub.2] from the air and into the oceans and eventually underground via plate tectonics. Volcanoes, meanwhile, spew C[O.sub.2] into the atmosphere. This cycle keeps the planet's temperatures from getting too extreme.

If the climate ever gets too cold, the carbon cycle could boost C[O.sub.2] to compensate. For instance, if temperatures drop and rainfall slows, the lack of weathering will allow C[O.sub.2] to build up in the atmosphere. And as volcanoes continue belching up additional C[O.sub.2], temperatures will rise and rainfall will rise. And if things get so hot that glaciers melt and rainfall increases, the planet will cool as weathering accelerates and draws down more C[O.sub.2] from the atmosphere. Plants and other organisms also play roles in drawing in C[O.sub.2] or releasing it into the air.

This balancing act could help keep planets within a comfortable range for life, expanding the habitable zone to as wide as 0.5 to 2.0 times Earth's distance from the sun, though these numbers are hotly contested. Thanks to the carbon cycle, Earth might still be habitable even if pushed out to Mars' orbit, says Penn State geoscientist James Kasting.

Rocky recycling

Not every planet tucked safely inside the habitable zone is necessarily life-friendly. Venus and Mars are within the habitable zone by some definitions, but neither boasts a livable surface climate. More than location is at play. Other factors such as plate tectonics may make a planet right or wrong for life. Plate tectonics is an important piece in the temperature-controlling carbon cycle, as the shifting and sinking plates that cover Earth's surface carry carbon into Earth's interior that later erupts from volcanoes. Some scientists propose that planets akin to Venus and Mars that lack the conditions for plate tectonics should be crossed off the "explore list" (SN: 1/23/16, p. 8).

Lindy Elkins-Tanton, a planetary scientist at Arizona State University in Tempe, disagrees. On exoplanets, other processes could do the job of plate tectonics, she said last December at an American Geophysical Union meeting in San Francisco. "We're too Earth-centric in our notion of how you can create a planetary carbon cycle," she says. "What else can we consider?"

One alternative could be the churning of a planet's outer layers in a way that doesn't require giant shifting slabs. The deepest part of a terrestrial planet's outermost shell becomes denser as pressures increase with depth. Rising molten rock from the planet's hot interior can also add density and heat to the bottom of the shell, making the rock runnier and denser. Even just a 1 percent density change could produce globs of material dense enough to sink deeper into the planet, carrying carbon along for the ride, Elkins-Tanton proposes.

As the material sinks, it releases some water like a squeezed sponge. This carbon-containing water then seeps back toward the surface. Water loosens the bonds that hold rocks together, which lowers a rock's melting point. If enough water accumulates, molten magma pools form and fuel volcanic eruptions. Together, these mechanisms could substitute for plate tectonics in the carbon cycle, Elkins-Tanton says. True, the process would be much slower than plate tectonics, but it could keep some planets' climates livable, her simulations show.

Hot air

Of course, the carbon cycle matters only if C[O.sub.2] is the main driver of the atmospheric blanket that keeps a planet cozy enough for life-sustaining liquid water. Plenty of other greenhouse gases, such as ozone or nitrous oxide, could keep exoplanets temperate. One, however, would be particularly potent: hydrogen.

Earth used to have a lot more hydrogen in its atmosphere. In 2013, Wordsworth and planetary scientist Raymond Pierrehumbert, now at the University of Oxford, proposed that hydrogen could have kept Earth warm back when the sun was cool. They were attempting to resolve the faint young sun paradox (SN: 5/4/13, p. 30).

Early in Earth's history, about 3.8 billion years ago, the sun shined 20 to 30 percent less brightly than it does now. Keeping the young planet warm posed a problem. Wordsworth and Pierrehumbert proposed that hydrogen, when combined with abundant nitrogen in the atmosphere, could serve as a paradox-resolving greenhouse gas. When hydrogen and nitrogen molecules collide in the air, the hydrogen molecules start wobbling differently. This wobbling increases the range of light wavelengths that hydrogen molecules absorb, amplifying the greenhouse effect. Hydrogen escaped from Earth's atmosphere over time. But on larger rocky planets with stronger gravitational pulls, that hydrogen would stick around, Wordsworth says.

With enough hydrogen and nitrogen, a planet can keep warm far outside of the C[O.sub.2]-based Goldilocks zone, Wordsworth says. Planets as far away from their sun as Pluto is to ours could stay above freezing. Even rogue planets alone in the cosmos with no parent star might keep warm enough to support life (SN: 4/4/15, p. 22).

The problem, however, is that these planets would need something akin to a carbon cycle to fine-tune hydrogen concentrations and prevent temperatures from getting too hot or too cold. Worse yet, at least on Earth, enterprising microbes feast on any available hydrogen for energy. Emerging lifeforms could gorge on an exoplanet's hydrogen, essentially eating the very thing keeping the planet warm enough for life. Those planets therefore might not stay habitable long enough for advanced life to evolve, Wordsworth says.

The inhabitance paradox

The hungry microbes might actually be good for hydrogen-wrapped planets, planetary scientist Dorian Abbot of the University of Chicago proposed at the AGU meeting in December. Higher temperatures make enzymes work faster and microbes more active. If temperatures rose, the hydrogen-chomping microbes would draw more hydrogen from the atmosphere and cool the planet. And if temperatures fell too far, microbe activity would fall and hydrogen levels would stabilize.

The ability of life, like those microbes, to fundamentally alter the climate and chemistry of its home planet poses a new paradox, Goldblatt said at the same meeting. Whether or not a planet is habitable could sometimes depend on whether life has already made itself at home there. He calls it the inhabitance paradox; the idea is an extension of the Gaia hypothesis, the proposal that organisms alter their surroundings to maintain a habitable environment. In other words, life could be a requirement for life.

The paradox showcases just how complex the hunt for habitable planets has become, Goldblatt says. "There are many other ways to support life--we just don't know what they are yet," he says. "Our imagination is limited to our experience. We're going to observe other planets and see things we never have imagined."

Explore more

* Lindy Elkins-Tanton. "What makes a habitable planet?" Eos. April 16, 2013.

Swing shifts

The Goldilocks zone marks the boundary where planets can exist without permanently slipping into a frigid or scorching wasteland. But even in the zone, extreme temperatures can happen, Kristen Menou proposed last year in Earth and Planetary Science Letters. While some scientists say life could exist outside the habitable zone, he thinks the habitable zone itself isn't entirely life-friendly.

Menou, an astrophysicist at the University of Toronto, ran climate simulations mimicking the conditions on hypothetical exoplanets just within the outer edge of the habitable zone. The planets receiving slightly less solar heat than Earth were vulnerable to extreme climate swings. Within tens of millions of years, these planets can cycle between frigid temperatures as low as around -63[degrees] Celsius and blistering heat of about 57[degrees] C. While such worlds briefly host liquid surface water, they spend as much as 99.2 percent of their time frozen. Unstable planets start appearing farther than about 1.25 times Earth's distance from the sun, the simulations show.

These capricious planets could eventually stabilize to have a habitable climate, but only if advanced plant life emerges first, Menou says. Plants boost the carbon cycle by absorbing and releasing C[O.sub.2], a process that helps regulate temperatures. Unfortunately, swinging climates would be inhospitable for the long-term evolution required to develop advanced plants, Menou says. "For complex life, these planets would look very threatening." Plants may never evolve, making the planets unlikely candidates for complex life.--Thomas Sumner

Caption: Where to look? The hunt for extraterrestrial life has long focused on planets at a just-right distance from alien stars. where liquid water can exist on a planet's surface.

Caption: Drop the base Geologic forces can churn a planet's outer layers without plate tectonics, research suggests. Density changes can cause large drops of carbon-carrying material to fall deeper into a planet's interior, releasing water that fuels volcanism, sending carbon back into the planet's atmosphere.

Caption: Hot hydrogen Collisions between hydrogen and nitrogen molecules in early Earth's atmosphere could have allowed hydrogen molecules to absorb a wider variety of light wavelengths ([H.sub.2]-[N.sub.2]). This effect would curb the amount of heat lost, warming the planet, new research suggests.


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Title Annotation:IN SEARCH OF ALIENS
Author:Sumner, Thomas
Publication:Science News
Date:Apr 30, 2016
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