Gravitational Wave Observations

Blanets: Worlds around Black Holes

blanet

Introduction

  • In Christopher Nolan’s 2014 sci-fi masterpiece Interstellar, three planets (aside from Earth) captivate viewers with their extreme environments.
  • Surprisingly, these worlds, technically termed Blanets, may not be purely fictional and could exist in reality.

What are Blanets?

  • Formation Theory: In 2019, Japanese scientists proposed a theory suggesting that planets could form within massive dust and gas clouds surrounding supermassive black holes.
  • Unique Characteristics: Blanets, unlike Earth, are not expected to resemble habitable worlds due to their formation near black holes.
  • Surrounding Environment: Black holes are encircled by colossal discs of gas and dust, influenced by the black hole’s gravitational pull and heating effects.
  • Galactic Presence: Nearly every galaxy is believed to harbor a supermassive black hole at its center, acting as a gravitational nucleus around which stars organize.

Formation Process

  • Similar Mechanism: Planets near young stars form from the collision and aggregation of dust and gas particles in swirling disks. A comparable process could occur near supermassive black holes.
  • Blanet Characteristics: Blanets are anticipated to be approximately 3,000 times larger than Earth and must orbit the black hole at a distance of about 100 trillion km to avoid gravitational disruption during their formation.

Implications and Speculations

  • Extreme Environments: Blanets represent worlds of extremes, vastly different from habitable planets like Earth.
  • Scientific Inquiry: The study of blanets offers insights into the dynamic interactions between black holes and their surrounding environments, pushing the boundaries of astrophysical understanding.

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