Distant planets tell all: A new analysis uses alien worlds' orbital treks to peek inside their stars.

NASA's ever-watchful Kepler space telescope has identified thousands of exoplanets by noting the tiny brightness dips caused when these worlds "transit," or cross the face of, their host stars. The length between dimmings tells scientists how long the planet takes to orbit—how long its year is—and the level of dimming shows how much smaller the planet is than the star.

And now, the speed of the planet's passing can also divine the star's density. [Wildest Alien Planet Discoveries of 2016]

"It's really weird that a planet that's orbiting far away from the star can tell us anything about the star's interior—I think that's really bizarre but cool," said Emily Sandford, an astronomer at Columbia University in New York and lead author on the new work. 

"Basically, by measuring very precisely the shape of those dimmings, the amount of light that's missing over time when a planet passes in front, you can measure the density of the star the planet's orbiting," she told Space.com.

Using a method first derived by astrophysicsts Sara Seager and Gabriela Mallen-Ornelas in 2003, Sandford and co-author David Kipping, also of Columbia, analyzed data on 66 Kepler stars to determine their densities. Their precision rivalled that of asteroseismology, a technique used on bright stars that uses oscillations in their shine to reconstruct their interior properties. While asteroseismology requires very precise brightness measurements, Sandford said, the new calculation needs less pristine data.

Essentially, the process works because how long a planet spends in front of its star is tied to the star's density. Planets that are far away from their stars spend less time in front of them—imagine a planet right at the star's surface, which would spend half of its orbit in front of it, versus one that is very far away, and only crosses in front for a quick part of its orbit, Sandford said. But at the same time, a planet has to move at a certain speed to maintain a steady orbit based on how massive the star is—if the planet is going too slowly, it will fall into the star, and if it's going too fast, it will fly away.

"We can then use that knowledge of [proportionally] how far the planet is from its star, combined with the duration of the transit, to solve for the stellar density," Sandford said. "If a planet is far away and yet takes a long time to transit, we know that the star must be big, puffy, and low-density; if a planet is close-in and yet transits quickly, we know that the star must be small, compact, and high-density."