File:KPD 0005+5106.jpg

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Captions

Jupiter-like planet is lossing mass to its neighboring white dwarf.

Summary

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Description
English: A team of scientists used NASA's Chandra X-ray Observatory and ESA's XMM-Newton to investigate some unusual X-ray activity of a white dwarf star, as reported in our latest press release. The data suggest this white dwarf is blasting a companion object, which is either a low-mass star or planet, with waves of heat and radiation while pulling it apart through gravitational force.

Most stars, including the Sun, will become "white dwarfs" after they begin to run out of fuel, expand and cool into a red giant, and then lose their outer layers. This evolution leaves behind a stellar nub that slowly fades for billions of years. An artist's illustration shows a white dwarf as the blue-white sphere near the center.

Astronomers have observed that the white dwarf KPD 0005+5106, located about 1,300 light years from Earth, emits high-energy X-ray emission that regularly increases and decreases in X-ray brightness every 4.7 hours. This recurring ebb and flow of X-rays indicates that KPD 0005+5106 has an object in orbit around it — either a very low mass star or a planet — depicted in the illustration by the brown and red object on the right-hand side. The white dwarf pulls the material from the companion into a disk around itself, which the artist shows in orange, before it slams into its north and south poles.

The concentration of material hitting the white dwarf's poles is creating two bright spots of high-energy X-ray emission. As the white dwarf and its companion orbit around each other the hot spot facing more towards Earth would go in and out of view, causing the high-energy X-rays to regularly increase and decrease that Chandra observed.

The researchers looked at what would happen if this object was a planet with the mass about that of Jupiter, a possibility that agrees with the data more readily than a dim star or a brown dwarf. In their models, the white dwarf would pull material from the planet onto the white dwarf, a process that the planet could only survive for a few hundred million years before eventually being destroyed. This stolen material swirls around the white dwarf, which glows in X-rays that Chandra can detect.
Date
Source https://chandra.si.edu/photo/2021/kpd0005/
Author Illustration: NASA/CXC/M. Weiss; X-ray: NASA/CXC/ASIAA/Y.-H. Chu, et al.

Licensing

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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