Exploring Outer Worlds

  • Released Tuesday, December 17, 2013
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Since the early 1990s, astronomers have known that distant planets orbit stars light-years from Earth. Although most of these alien worlds, called exoplanets, are too far away to be imaged directly, scientists have made detailed observations of their size and composition. One method of study involves watching a planet as it transits its host star. By measuring how the brightness and color of a star changes when a planet crosses in front of its disk, astronomers can indirectly determine the mass of the planet and the proximity of its orbit. Similar measurements can provide other key information, like the chemical makeup of a planet's atmosphere. Watch the video to learn more.

When a planet crosses in front of a star, some of the star's light is absorbed, and some is transmitted, passing through the planet's atmosphere.

When a planet crosses in front of a star, some of the star's light is absorbed, and some is transmitted, passing through the planet's atmosphere.

During a transit, a planet’s size can be determined by measuring the observed decrease in brightness of its star.

During a transit, a planet’s size can be determined by measuring the observed decrease in brightness of its star.

Scientists can identify which chemicals are present in a planet’s atmosphere by separating transmitted light into a spectrum of colors.

Scientists can identify which chemicals are present in a planet’s atmosphere by separating transmitted light into a spectrum of colors.



Credits

Please give credit for this item to:
NASA's Goddard Space Flight Center
Cover image courtesy of ESA/Hubble

Release date

This page was originally published on Tuesday, December 17, 2013.
This page was last updated on Wednesday, May 3, 2023 at 1:51 PM EDT.