Planetary cores can broadcast for over 100 million years and as long as a billion years after their stars have burnt up their nuclear fuel.

Astronomers have turned their focus on cores of exoplanets around white dwarf stars. They are “tuning in” to the radio waves they emit.

Research led by Dr. Dimitri Veras from the Department of Physics assesses the survivability of planets that orbit stars which have burnt all of their fuel and shed their outer layers, destroying nearby objects and removing the outer layers of planets. The researchers have determined they could detect the cores which result from this destruction and those cores could survive for long enough to be found from Earth.

Co-author Professor Alexander Wolszczan from Pennsylvania State University discovered the first exoplanet confirmed to exist orbiting a pulsar, in the 1990s. He did that using a method that detects radio waves emitted from the star. The researchers plan to observe white dwarfs in a similar part of the electromagnetic spectrum. Therefore, they hope to achieve another breakthrough.

The magnetic field between a white dwarf and an orbiting planetary core can form a unipolar inductor circuit, with the core acting as a conductor due to its metallic constituents. Radiation from that circuit is emitted as radio waves which researchers can then detect with radio telescopes on Earth. The effect can also be detected from Jupiter and its moon Io, which form a circuit of their own.

However, the scientists needed to determine how long those cores can survive after being stripped of their outer layers. They found that planetary cores can survive for over 100 million years and as long as a billion years.

The astronomers plan to use the results of the new research in proposals for observation time on telescopes such as Arecibo in Puerto Rico and the Green Bank Telescope in West Virginia to try to find planetary cores around white dwarfs.

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“There is a sweet spot for detecting these planetary cores: a core too close to the white dwarf would be destroyed by tidal forces, and a core too far away would not be detectable,” says lead author Dimitri Veras from the physics department at the University of Warwick.

“Also, if the magnetic field is too strong, it would push the core into the white dwarf, destroying it. Hence, we should only look for planets around those white dwarfs with weaker magnetic fields at a separation between about 3 solar radii and the Mercury-Sun distance.

“Nobody has ever found just the bare core of a major planet before, nor a major planet only through monitoring magnetic signatures, nor a major planet around a white dwarf. Therefore, a discovery here would represent ‘firsts’ in three different senses for planetary systems.”

“We will use the results of this work as guidelines for designs of radio searches for planetary cores around white dwarfs,” Wolszczan says. “Given the existing evidence for a presence of planetary debris around many of them, we think that our chances for exciting discoveries are quite good.”

“A discovery would also help reveal the history of these star systems because for a core to have reached that stage it would have been violently stripped of its atmosphere and mantle at some point and then thrown towards the white dwarf,” Veras adds. “Such a core might also provide a glimpse into our own distant future, and how the solar system will eventually evolve.”

The research appears in the Monthly Notices of the Royal Astronomical Society.

Source: University of Warwick

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