How 'Giant' Planets Impact Neighbors' Habitability

The habitable zone is the region around a star where a planet with an Earth-like atmosphere on a circular orbit can support liquid water on its surface.

Studying 147 extrasolar planetary systems with giant planets (with the parameters of these systems taken from NASA’s exoplanet archive), Georgakarakos and colleagues found that, in most cases, the presence of “giant neighbors” would reduce a terrestrial planet’s chances to remain habitable, even when the terrestrial planet is on a stable orbit. A stable orbit means that the terrestrial planet is not ejected from the system, or pushed to the outskirts. It is important that the complex gravitational interactions between the star, the terrestrial planet, and its ”giant neighbor” result in a stable orbit for the Earth-like planet as the development and evolution of life on a planet requires long timescales.

“While in the majority of investigated systems the presence of the gas ‘giants’ shrank the habitable zone, they still left sufficient room for habitable Earth-like planets to be there,” said Georgakarakos. “This is an important insight to inform follow-up investigations. It would not make sense to search for Earth 2.0 in a system where a giant planet stirs the orbit of any neighboring terrestrial planet in the habitable zone so much that its climate collapses.”

Added Siegfried Eggl, associate researcher at JPL: “Perhaps most surprisingly, our findings suggest that, under certain conditions, the presence of a giant planet can actually increase the size of the habitable zone, which is the area where your terrestrial planet receives the right amount of light in order to support liquid water on its surface. This is quite remarkable since the continuous gravitational pull of giant planets on their terrestrial neighbors mostly spells trouble for habitability.”

By providing specific constraints on when precisely giant planets become “bad neighbors,” Georgakarakos, Eggl, and Ian Dobbs-Dixon, NYUAD assistant professor of physics, were able to identify prime targets in the ongoing search for a “second Earth.” “The general idea is the farther away the giant planet is from the habitable zone, the better. For planets that are similar to our Earth that is actually true. What we showed, however, is that this may not necessarily be the case for Earth-like planets with a climate less sensitive to changes in the incoming radiation,” Georgakarakos said.

 Contacts and sources:
Adam Pockriss
Rubenstein (for NYU Abu Dhabi)

Calla Cofield
NASA Jet Propulsion Laboratory