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  2. Superluminal motion - Wikipedia

    en.wikipedia.org/wiki/Superluminal_motion

    Superluminal motion is most often observed in two opposing jets emanating from the core of a star or black hole. In this case, one jet is moving away from and one towards the Earth. If Doppler shifts are observed in both sources, the velocity and the distance can be determined independently of other observations.

  3. Hypernova - Wikipedia

    en.wikipedia.org/wiki/Hypernova

    In this case, a massive star (>30 solar masses) collapses to form a rotating black hole emitting twin astrophysical jets and surrounded by an accretion disk. It is a type of stellar explosion that ejects material with an unusually high kinetic energy , an order of magnitude higher than most supernovae, with a luminosity at least 10 times greater.

  4. Superluminous supernova - Wikipedia

    en.wikipedia.org/wiki/Superluminous_supernova

    The collapsar model is a type of superluminous supernova that produces a gravitationally collapsed object, or black hole. The word "collapsar", short for "collapsed star", was formerly used to refer to the end product of stellar gravitational collapse, a stellar-mass black hole. The word is now sometimes used to refer to a specific model for ...

  5. List of star extremes - Wikipedia

    en.wikipedia.org/wiki/List_of_star_extremes

    A star is a massive luminous spheroid astronomical object made of plasma that is held together by its own gravity.Stars exhibit great diversity in their properties (such as mass, volume, velocity, stage in stellar evolution, and distance from Earth) and some of the outliers are so disproportionate in comparison with the general population that they are considered extreme.

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  7. Galaxy rotation curve - Wikipedia

    en.wikipedia.org/wiki/Galaxy_rotation_curve

    The rotation curve of a disc galaxy (also called a velocity curve) is a plot of the orbital speeds of visible stars or gas in that galaxy versus their radial distance from that galaxy's centre. It is typically rendered graphically as a plot , and the data observed from each side of a spiral galaxy are generally asymmetric, so that data from ...

  8. Supermassive black hole - Wikipedia

    en.wikipedia.org/wiki/Supermassive_black_hole

    If black holes evaporate via Hawking radiation, a non-rotating and uncharged stupendously large black hole with a mass of 1 × 10 11 M ☉ will evaporate in around 2.1 × 10 100 years. [ 89 ] [ 18 ] Black holes formed during the predicted collapse of superclusters of galaxies in the far future with 1 × 10 14 M ☉ would evaporate over a ...

  9. Barycenter (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Barycenter_(astronomy)

    If the four giant planets were on a straight line on the same side of the Sun, the combined center of mass would lie at about 1.17 solar radii, or just over 810,000 km, above the Sun's surface. [ 7 ] The calculations above are based on the mean distance between the bodies and yield the mean value r 1 .

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