A newly discovered distant planetary system features multiple planets that orbit at a severe tilt to their host star.
Such tilted orbits had been found in planetary systems featuring a “hot Jupiter,” a giant planet in a close orbit to its host star. But, until now, they hadn’t been observed in multiplanetary systems without such a big interloping planet.
“This is a new level of detail about the architecture of a planetary system outside our solar system,” says Steve Kawaler, professor of physics and astronomy at Iowa State University and a leader of the Kepler Asteroseismic Investigation.
“These studies allow us to draw a detailed picture of a distant system that provides a new and critical test of our understanding of how these very alien solar systems are structured.”
Kawaler is part of the research team that studied regular changes in the brightness of the host star, Kepler-56, an aging red giant star with two planets in close orbits and a massive third planet in a distant orbit. By measuring those oscillation frequencies and using spectroscopy data about the star’s temperature and chemistry, researchers measured the star’s diameter and other properties.
The paper, published in Science, reports Kepler-56 is more than four times the radius of our sun. Its mass is also 30 percent greater than our sun. It is about 3,000 light years from Earth.
Kawaler says he was also part of the team that used studies of the changes in brightness to help determine the tilt of the rotation axis of Kepler-56. That axis is tilted 45 degrees to the line of sight from Earth.
Generally, Kawaler says, the simplest way for a planetary system to develop is with the orbits in the same plane as the host star’s equator. That typically indicates the planets formed from a thin disk of dust and gas surrounding the host star. The planets in our solar system all orbit within 7 degrees of the plane of the sun’s equator.
A planet orbit that tilts away from other planets or from the host star’s equator can mean the planet had a traumatic youth, Kawaler says. It may have been pulled into a different plane after encountering another planet or planets. That’s generally the case with migrating hot Jupiters. They change their orbits after encounters with other planets and material, and therefore have a higher chance of tilted orbits.
In the case of Kepler-56, however, the more massive outer planet seems to be maintaining the tilted orbits of the two inner planets.
“It issues a continuous tug on the orbit of the smaller ones, pulling them into their inclined orbits,” Kawaler says.
All of those Kepler-56 observations, the researchers note, add up to firm evidence that tilted planetary orbits are possible even in systems that don’t contain a hot Jupiter.
Lead author of the study is Daniel Huber of NASA’s Ames Research Center in Mountain View, California.
Source: Iowa State University