Neil deGrass Tyson "Orbital Erosion"

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SUMMARY

Neil deGrasse Tyson referenced "orbital erosion" in the context of two black holes orbiting each other, which relates to the phenomenon of orbital decay due to gravitational waves. In classical mechanics, two bodies in orbit are stable; however, general relativity introduces the concept that gravitational waves can carry away energy and angular momentum, leading to a gradual spiral towards each other. This effect is negligible in systems like the Earth-Sun but significant in binary black hole or neutron star systems, providing strong evidence for gravitational waves.

PREREQUISITES
  • Understanding of general relativity
  • Knowledge of gravitational waves
  • Familiarity with orbital mechanics
  • Basic concepts of black hole physics
NEXT STEPS
  • Research gravitational wave detection methods, such as LIGO
  • Study the PSR B1913+16 pulsar-neutron star binary as a case study
  • Explore the implications of orbital decay in astrophysical systems
  • Learn about the effects of tidal forces on celestial bodies
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Astronomers, astrophysicists, and students interested in gravitational physics and the dynamics of binary systems will benefit from this discussion.

mgkii
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I listened to one of NDT's lectures on a podcast this morning and he made a passing reference to two black holes orbiting each other that would eventually "spiral into each other due to orbital erosion" (his words)

I'm familiar with orbital decay for satellites in orbit around the Earth due to friction, emf etc; and I'm familiar with planet and moon orbits expanding from tidal forces, energy lost to gravitational waves etc. However I'm struggling to understand Neil's reference to orbital erosion in relation to Black holes (although from the context of his comment I don't think his comments were specific to Black holes), my understanding until now has been that two bodies orbiting each other would be stable unless other forces act inn them?

Can anyone enlighten me as to what Neil may have been referring to?

Thanks
Matt
 
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Two bodies orbiting each other will be stable forever in classical mechanics, but when you introduce general relativity, the picture changes somewhat. Gravitational waves will carry away energy/angular momentum from the system, resulting in the two bodies spiralling into each other. In the Earth-Sun system, this effect is absolutely negligible (1/300th of a hydrogen atom each year), but in orbiting black holes or neutron stars, this effect can be significant. In fact, observations the orbital decay of a pulsar-neutron star binary is considered some of the strongest evidence for gravitational waves. https://en.wikipedia.org/wiki/PSR_B1913+16

You can read more about how gravitational waves result in orbital decay here:
https://en.wikipedia.org/wiki/Gravitational_wave#Orbital_decay_from_gravitational_radiation
 
Fantastic reply. Many thanks indeed.
 
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