Evolution of planetary system around a white dwarf

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SUMMARY

The discussion centers on the findings regarding the white dwarf G238-44, located 86 light-years from Earth, which is currently accreting material from its surrounding planetary system. Lead researcher Ted Johnson from UCLA highlights that this is the first observation of both types of objects accreting onto a white dwarf simultaneously. The research utilizes archival data from the Hubble Space Telescope and other NASA observatories to analyze the chaotic evolution of planetary systems as stars transition from red giants to white dwarfs, leading to significant orbital disruptions.

PREREQUISITES
  • Understanding of white dwarf characteristics and formation
  • Familiarity with planetary system dynamics and evolution
  • Knowledge of astronomical observation techniques, particularly using the Hubble Space Telescope
  • Basic concepts of stellar evolution, including red giants and nuclear fusion
NEXT STEPS
  • Research the process of stellar evolution from red giant to white dwarf
  • Explore the implications of white dwarf accretion on planetary system stability
  • Investigate the role of NASA's Hubble Space Telescope in astronomical discoveries
  • Study the dynamics of planetary orbits in the context of stellar death
USEFUL FOR

Astronomers, astrophysicists, and students interested in stellar evolution and planetary system dynamics will benefit from this discussion, particularly those focusing on the fate of solar systems around dying stars.

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An article came up on Phys.org about a white dwarf drawing in material from the planetary system surrounding it. Is this the ultimate fate of our solar system?

https://phys.org/news/2022-06-dead-star-cannibalism-planetary-far-reaching.html

"We have never seen both of these kinds of objects accreting onto a white dwarf at the same time," said lead researcher Ted Johnson, a physics and astronomy major at UCLA who graduated last week. "By studying these white dwarfs, we hope to gain a better understanding of planetary systems that are still intact."

The findings are based on an analysis of materials captured by the atmosphere of G238-44, a white dwarf some 86 light-years from Earth, using archival data from the Hubble Space Telescope and additional NASA satellites and observatories. A white dwarf is the burned-out core that remains after a star like our sun sheds its outer layers and stops burning fuel through nuclear fusion.

Theories of planetary-system evolution describe the demise of a star as a turbulent, chaotic event, one that begins when it first balloons exponentially into what is known as a red giant and then quickly loses its outer layers, collapsing into a white dwarf—a super-dense star about the size of Earth, with a mass of our sun. The process dramatically disrupts the remaining planets' orbits, and smaller objects—asteroids, comets, moons—that venture too close to them can be scattered like pinballs and sent hurtling toward the white dwarf.

https://www.nasa.gov/feature/goddard/2022/hubble-dead-star-caught-ripping-up-planetary-system

The findings are based on analyzing material captured by the atmosphere of the nearby white dwarf star G238-44. A white dwarf is what remains of a star like our Sun after it sheds its outer layers and stops burning fuel though nuclear fusion. "We have never seen both of these kinds of objects accreting onto a white dwarf at the same time," said Ted Johnson, the lead researcher and recent University of California, Los Angeles (UCLA) bachelor's graduate. "By studying these white dwarfs, we hope to gain a better understanding of planetary systems that are still intact."
 
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