Which structure around Cygnus X-1 is directly involved in feeding matter toward the black hole?

Prepare for the NOVA Black Hole Apocalypse Astronomy Test with flashcards and multiple choice questions. Each question offers hints and explanations. Get ready for your exam!

Multiple Choice

Which structure around Cygnus X-1 is directly involved in feeding matter toward the black hole?

Explanation:
Feeding matter toward a black hole happens through an accretion disk, a rotating disk of gas that spirals inward as viscosity allows angular momentum to be transported outward and gravitational energy to be converted into heat. In Cygnus X-1, material drawn from the companion star forms this disk and becomes extremely hot, emitting strong X-rays as it loses energy while moving closer to the black hole. The event horizon is the boundary beyond which nothing can escape, not a structure that channels matter inward. The corona is a hot, tenuous region above the disk that produces high-energy photons through scattering processes, but it’s not the channel that feeds matter. A dust torus is a broader, often larger-scale ring found in some active galaxies, not the main feeding feature in this stellar-mass black hole system. Therefore, the accretion disk is the structure directly involved in feeding matter toward the black hole.

Feeding matter toward a black hole happens through an accretion disk, a rotating disk of gas that spirals inward as viscosity allows angular momentum to be transported outward and gravitational energy to be converted into heat. In Cygnus X-1, material drawn from the companion star forms this disk and becomes extremely hot, emitting strong X-rays as it loses energy while moving closer to the black hole. The event horizon is the boundary beyond which nothing can escape, not a structure that channels matter inward. The corona is a hot, tenuous region above the disk that produces high-energy photons through scattering processes, but it’s not the channel that feeds matter. A dust torus is a broader, often larger-scale ring found in some active galaxies, not the main feeding feature in this stellar-mass black hole system. Therefore, the accretion disk is the structure directly involved in feeding matter toward the black hole.

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