A white dwarf may seem like it would be a calm, dying star, but scientists say such stars can pack a gravitational punch so strong that they can tear a passing planet apart.

Scientists using several telescopes, including NASA's Chandra X-ray Observatory, found evidence that a planet in an ancient cluster of stars on the edge of the Milky Way drifted too close to a white dwarf star and was ripped apart. NASA officials explained the discovery in a video on the planet's death by white dwarf.

White dwarf stars start out as any normal star about the size of the sun, but eventually swell into red giants while they burn up the hydrogen in their core and fuse it into helium. When all the hydrogen is gone, only the star's core is left —a dense sphere with a radius about one hundredth the size of the original star, but with almost the same mass.

The dead stars' density creates a strong gravitational pull, more than 10,000 times stronger than the gravitational force at the surface of the sun, according to NASA officials.

That force, and its associated tides, could have the power to pull apart a planet that passes too close, astronomers said. They estimate the destroyed planet had about a third of the mass of Earth and the white dwarf has approximately 1.4 times the mass of the sun.

Researchers using the European Space Agency's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) discovered the possibility that a white dwarf tore a planet apart when they found an unexpected source of X-ray radiation in globular star cluster NGC 6388. They initially thought the radiation was due to hot gas swirling toward an intermediate-mass black hole thought to be at the center of the cluster.

The globular cluster NGC 6388 shines purple in this X-ray view from NASA's Chandra X-Ray Observatory.
The globular cluster NGC 6388 shines purple in this X-ray view from NASA's Chandra X-Ray Observatory.
Credit: X-ray: NASA/CXC/IASF Palermo/M.Del Santo et al; Optical: NASA/STScI

A second look with Chandra X-ray Observatory, however, revealed that the X-rays were actually coming from a point off to the side of the cluster's possible black hole center. Scientists continued to monitor the radiation for 200 days with the X-ray telescope on board NASA's Swift gamma-ray burst observatory, an international mission that aims to solve the mystery of what causes brief and intense flashes of gamma-ray radiation in space.

As scientists monitored the X-rays, the radiation dimmed at a rate that agrees with current theories of how a planet ripped apart by the gravitational tidal forces of a white dwarf would react. These theories predict the debris from a planet shredded by a white dwarf would be heated and glow in X-rays as it falls onto the white dwarf.

"While the case for the tidal disruption of a planet is not iron-clad, the argument for it was strengthened when astronomers used data from the multiple telescopes to help eliminate other possible explanations for the detected X-rays," NASA officials wrote in a statement.    

The research was detailed in an October 2014 issue of the Monthly Notices of the Royal Astronomical Society.

Follow Kasandra Brabaw on Twitter at @KassieBrabaw. Follow us @Spacedotcom, Facebook and Google+. Original article on Space.com.