An artist’s portrayal of a Warm Jupiter gas-giant planet in orbit around its parent star, along with smaller companion planets.

An artist’s portrayal of a Warm Jupiter gas-giant planet (right) in orbit around its parent star, along with smaller companion planets. Credit: Detlev Van Ravenswaay/Science Photo Library

After analyzing four years of Kepler space telescope observations, astronomers from the University of Toronto have given the clearest understanding yet of a class of exoplanets called “warm Jupiters,” showing that many have unexpected planetary companions.

The team’s analysis, published July 10 in the Astrophysical Journal, provides strong evidence of the existence of two distinct types of warm Jupiters, each with their own formation and dynamical history.

The two types include those that have companions and thus, likely formed where we find them today; and those with no companions that likely migrated to their current positions.

According to lead author Chelsea Huang, a Dunlap Fellow at University of Toronto's Dunlap Institute for Astronomy & Astrophysics, “Our findings suggest that a big fraction of warm Jupiters cannot have migrated to their current positions dynamically and that it would be a good idea to consider more seriously that they formed where we find them.”

An artist's impression shows Jupiter migrating in toward the sun and Earth.
Answering the question of whether warm Jupiters form close to their stars or migrate in will tell us more about the history of our own Jupiter and our solar system. Credit: NASA / ESA / STScI

Warm Jupiters are large, gas-giant exoplanets—planets found around stars other than the sun. They are comparable in size to the gas-giants in our solar system. But unlike the sun’s family of giant planets, warm Jupiters orbit their parent stars at roughly the same distance that Mercury, Venus and the Earth circle the Sun. They take 10 to two hundred days to complete a single orbit.

Because of their proximity to their parent stars, they are warmer than our system’s cold gas giants—though not as hot as hot Jupiters, which are typically closer to their parent stars than Mercury.

It has generally been thought that warm Jupiters didn’t form where we find them today; they are too close to their parent stars to have accumulated large, gas-giant-like atmospheres. So, it appeared likely that they formed in the outer reaches of their planetary systems and migrated inward to their current positions, and might in fact continue their inward journey to become hot Jupiters. On such a migration, the gravity of any warm Jupiter would have disturbed neighbouring or companion planets, ejecting them from the system.

But, instead of finding “lonely,” companion-less warm Jupiters, the team found that 11 of the 27 targets they studied have companions ranging in size from Earth-like to Neptune-like.

“And when we take into account that there is more analysis to come,” says Huang, “the number of warm Jupiters with smaller neighbours may be even higher. We may find that more than half have companions.”

NASA’s Ames Research Center in Moffett Field, California, manages the Kepler and K2 missions for NASA’s Science Mission Directorate. NASA’s Jet Propulsion Laboratory in Pasadena, California, managed Kepler mission development. Ball Aerospace & Technologies Corporation operates the flight system with support from the Laboratory for Atmospheric and Space Physics at the University of Colorado at Boulder.

To read the paper “Warm Jupiters are less lonely than hot Jupiters”, visit: