When searching for potentially habitable exoplanets, one of the key factors to take into consideration is the habitable zone, the region around a star where temperatures could allow liquid water to exist on the surface of any rocky planets that may orbit them.
In general, this region is neither too hot nor too cold, although other characteristics that could affect the surface temperature of a planet such as cloud cover must also be taken into consideration when estimating a planet’s possible habitability.
The “classic” habitable zone model has remained unchanged for some time, but now yesterday a group of astronomers have announced some modifications that will affect how many discovered exoplanets are considered to be in their stars’ habitable zones.
The astronomers, from Penn State and also collaborators with the Planetary Habitability Laboratory, have concluded that, overall, the habitable zones are a bit farther out from their stars than previously thought.
“This has implications for finding other planets with life on them,” according to Ravi Kumar Kopparapu, a lead investigator with the new study.
Just how does this affect the potentially habitable exoplanets already discovered? It means that some of them may not be in the newly-defined habitable zone after all, but also that some exoplanets previously considered to be outside the habitable zone will now be in it.
In our solar system, the “old” habitable zone extended from just inside the orbit of Venus to outside the orbit of Mars. Under the new definition, Earth would now reside very close to the inner edge of the habitable zone instead of Venus. Interesting, considering that Earth flourishes with life, even though it is now barely inside our Sun’s habitable zone.
The original press release is here.
There will also be a related update to the Habitable Exoplanets Catalog on February 18, 2013.
This article was first published on Examiner.com.