A planet that lies in the "habitable zone" of a star has no guarantee of being "habitable." But a planet in the habitable zone receives enough radiation from its parent star (or stars) that the temperature on its surface could be right for hosting liquid water on its surface, an essential ingredient for life as we know it. Too much heat and liquid water evaporate; too little heat and the water would freeze.
The habitable zone is a good starting place to search for habitable worlds, but planets in this region could very easily be unfit for life.
For a planet to have liquid water on its surface, it has to have a surface, which means it has to be rocky, like Earth, not a gas giant like Jupiter or Saturn. The planet also has to have an atmosphere, but that atmosphere has to be moderate — Venus' atmospheremakes the planet's surface far too hot for water to remain a liquid, but that may not have always been the case. And scientists think it's likely that many planets migrate through their solar system, so they could move out of the habitable zone, killing off any life that might have emerged there. Most stars experience a change in their radiation output near the beginning of their lifetimes, which could have the same effect.
"When we talk about 'the habitable zone,' we're really just talking about a crude sample selection technique," Tasker said. "It is not a quantitative measurement of a planet's habitability."
Tasker also mentioned that there are multiple scenarios in which life might survive outside the habitable zone. Take, for example, a moon orbiting a very large, hot planet around a star. The moon not only receives heat from the star, but may also receive heat from the planet. In addition, if the moon has an eccentric orbit (meaning not circular), it could experience extreme tidal heating (wherein the gravity of a planet pulls on the interior of a moon, creating a potential internal heat source for the moon). In that case, the moon might be too hot if it lies in the habitable zone of the parent star, but could be perfectly habitable if it lies just outside the habitable zone.
In total, researchers have identified thousands of alien planets, and there are new instruments coming online that will identify even more. Advanced instruments, like the James Webb Space Telescope (JWST), set to launch in 2019, will allow scientists to study those known planets in more detail, and search for complex "biosignatures" in the exoplanet atmospheres, or chemical combinations that are typically produced by life-forms. The upcoming Wide-Field Infrared Survey Explorer (WFIRST), set to launch in the mid-2020s, and the proposed Large UV/ Optical/Infrared Survey (LUVOIR), could also search for signs of habitability on exoplanets.
"I personally think this is perhaps the most exciting time for our field," Tasker said during her presentation. "I think, perhaps, in the next 10 years we're going to be able to really start talking about habitability on another planet.
"Now whether we will discover — conclusively — life, I think that's more questionable, but the amount of information we're going to get from things like JWST or WFIRST or LUVOIR is going to be game changing," she said. "It's going to be amazing."
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- Original article on Space.com.


Animation Tool Helps Alien-Hunting Scientists Track a Planet's Habitable Zone

























