Polluted Old Stars Suggest Earth-like Worlds May Be Common

Polluted Old Stars Suggest Earth-like Worlds May Be Common
An artist's impression of a massive asteroid belt in orbit around a star. The new work with SDSS data shows that similar rubble around many white dwarfs contaminates these stars with rocky material and water. (Image credit: NASA-JPL / Caltech / T. Pyle (SSC))

Earth-like planets should be a fairly common feature ofother solar systems in our galaxy, a new study of stellar senior citizenssuggests.

More than 90 percent of stars in the Milky Way, includingour own sun, endtheir lives as a white dwarfs. Traditionally, these dense stellar remainshaven't been the first place that astronomers look for signs of planetsoutside our own solar system. Instead, exoplanet searches have focused onstars like our own sun.

White dwarfs should essentially be composed of pure hydrogenand helium atmospheres. Any elements heavier than helium ("metals" inastronomical parlance) present in a white dwarf atmosphere have to bepollutants from some external source.

"But it turns out that [this explanation] doesn'treally fit the data," Fahiri told SPACE.com.

What's going on

Farihi has looked at white dwarfs with NASA's infraredSpitzer Space Telescope for five years, and thoseobservations showed that the white dwarfs "have dust right on top ofthem," Farihi said. "It's almost certainly raining down on theiratmospheres."

Farihi and his colleagues looked at the positions of thesewhite dwarfs within the Milky Way and estimated whether the impurities they sawin the stars' atmospheres could be explained by sweeping up the interstellarmedium.

"And the answer is a resounding 'No, it doesn't make sense,'"Farihi said.

They found that the types of metals seen in the stellaratmospheres, such as silicon, magnesium and iron, suggest a rocky origin. Theexact source of the rocky debris isn't known, but Farihi says there are twopossibilities: the debris could come from an asteroid belt similar to our own,which essential represents a planet that didn?t form, or the pieces of ashattered planet.

"The rocks that delivered the metals probably deliveredthe hydrogen," Farihi said. The hydrogen suggests that the minerals thatcontained the metals also contained water, an essential chemical for life as weknow it.

Join our Space Forums to keep talking space on the latest missions, night sky and more! And if you have a news tip, correction or comment, let us know at: community@space.com.

Andrea Thompson
Contributor

Andrea Thompson is an associate editor at Scientific American, where she covers sustainability, energy and the environment. Prior to that, she was a senior writer covering climate science at Climate Central and a reporter and editor at Live Science, where she primarily covered Earth science and the environment. She holds a graduate degree in science health and environmental reporting from New York University, as well as a bachelor of science and and masters of science in atmospheric chemistry from the Georgia Institute of Technology.