An accretion disk may form a variety of celestial objects, primarily through the gravitational attraction of material falling toward a central mass, such as a star or a black hole. As this material spirals inward, it loses angular momentum and heats up, emitting radiation. This process can lead to the formation of a new star, a planet, or even a binary star system, depending on the mass and dynamics involved. Additionally, in the case of black holes, the accretion disk can contribute to the growth of the black hole itself.
When a nebula is disturbed by an outside explosion, it may form an accretion disc.
When a nebula is disturbed by an outside explosion, it may form an accretion disc.
When a nebula is disturbed by an outside explosion, it may form an accretion disc.
solar system Material that is in orbit around a massive central body is an accretion disk. This disk can eventually turn into a white dwarf star. An accretion disc may eventually form planets such as the ones in our solar system.
Solar system
accretion disk
When a nebula is disturbed by an outside explosion, it may form an accretion disc.
When a nebula is disturbed by an outside explosion, it may form an accretion disc.
When a nebula is disturbed by an outside explosion, it may form an accretion disc.
nebula
solar system Material that is in orbit around a massive central body is an accretion disk. This disk can eventually turn into a white dwarf star. An accretion disc may eventually form planets such as the ones in our solar system.
This description describes a nebula.