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  2. Rotating black hole - Wikipedia

    en.wikipedia.org/wiki/Rotating_black_hole

    In late 2006, astronomers reported estimates of the spin rates of black holes in The Astrophysical Journal. A black hole in the Milky Way, GRS 1915+105, may rotate 1,150 times per second, [6] approaching the theoretical upper limit.

  3. Galaxy rotation curve - Wikipedia

    en.wikipedia.org/wiki/Galaxy_rotation_curve

    The rotational/orbital speeds of galaxies/stars do not follow the rules found in other orbital systems such as stars/planets and planets/moons that have most of their mass at the centre. Stars revolve around their galaxy's centre at equal or increasing speed over a large range of distances.

  4. Galactic orientation - Wikipedia

    en.wikipedia.org/wiki/Galactic_orientation

    Spiral galaxies range from S0, the lenticular galaxies, to Sb, which have a bar across the nucleus, to Sc galaxies which have strong spiral arms. In total count, ellipticals amount to 13%, S0 to 22%, Sa, b, c galaxies to 61%, irregulars to 3.5%, and peculiars to 0.9%. At the center of most galaxies is a high concentration of older stars.

  5. Astrophysical jet - Wikipedia

    en.wikipedia.org/wiki/Astrophysical_jet

    Two early theories have been used to explain how energy can be transferred from a black hole into an astrophysical jet: Blandford–Znajek process. [15] This theory explains the extraction of energy from magnetic fields around an accretion disk, which are dragged and twisted by the spin of the black hole.

  6. Density wave theory - Wikipedia

    en.wikipedia.org/wiki/Density_wave_theory

    The density wave theory also explains a number of other observations that have been made about spiral galaxies. For example, "the ordering of H I clouds and dust bands on the inner edges of spiral arms, the existence of young, massive stars and H II regions throughout the arms, and an abundance of old, red stars in the remainder of the disk".

  7. Differential rotation - Wikipedia

    en.wikipedia.org/wiki/Differential_rotation

    The reciprocal of the rotational shear is the lap time, i.e. the time it takes for the equator to do a full lap more than the poles. The relative differential rotation rate is the ratio of the rotational shear to the rotation rate at the equator: α = Δ Ω Ω 0 {\displaystyle \alpha ={\frac {\Delta \Omega }{\Omega _{0}}}}

  8. Spin-flip - Wikipedia

    en.wikipedia.org/wiki/Spin-flip

    A black hole spin-flip occurs when the spin axis of a rotating black hole undergoes a sudden change in orientation due to absorption of a second (smaller) black hole. Spin-flips are believed to be a consequence of galaxy mergers , when two supermassive black holes form a bound pair at the center of the merged galaxy and coalesce after emitting ...

  9. Hubble's law - Wikipedia

    en.wikipedia.org/wiki/Hubble's_law

    The mathematical derivation of an idealized Hubble's law for a uniformly expanding universe is a fairly elementary theorem of geometry in 3-dimensional Cartesian/Newtonian coordinate space, which, considered as a metric space, is entirely homogeneous and isotropic (properties do not vary with location or direction). Simply stated, the theorem ...