Wandering Planets

  • Released Thursday, May 26, 2016

Not every planet orbits a star, tethered by gravity like Earth to the sun. Outside our solar system, some planets roam free in the space between stars. Scientists estimate there may be billions of these cosmic nomads lurking in our Milky Way galaxy alone. To find them, NASA’s Kepler Space Telescope observes how these worlds temporarily intensify the light from distant stars. This effect, called microlensing, occurs because the gravity from massive objects in the universe warps the space around them. When a planet passes in front of a faraway star, its gravity bends the star’s light. That allows more light to briefly focus toward the telescope. From Kepler’s perspective, the star brightens and then dims over the course of the alignment. By staring at stars in a slice of our galaxy that extends to the heart of the Milky Way, Kepler will help scientists discover new worlds that are farther away than ever before. Watch the video to learn more.

When a planet passes in front of a distant star, its gravity bends and intensifies the star's light like a magnifying glass.

When a planet passes in front of a distant star, its gravity bends and intensifies the star's light like a magnifying glass.

To detect these worlds, scientists use Kepler to observe the short-term change in a star’s brightness.

To detect these worlds, scientists use Kepler to observe the short-term change in a star’s brightness.

Kepler is looking for new planets in our Milky Way galaxy located within a 20,000 light-year-long wedge of space (highlighted above).

Kepler is looking for new planets in our Milky Way galaxy located within a 20,000 light-year-long wedge of space (highlighted above).



Credits

Please give credit for this item to:
NASA's Goddard Space Flight Center
Video and images courtesy of NASA/Ames/JPL-Caltech

Release date

This page was originally published on Thursday, May 26, 2016.
This page was last updated on Wednesday, May 3, 2023 at 1:48 PM EDT.