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A black hole with the mass of a car would have a diameter of about 10 −24 m and take a nanosecond to evaporate, during which time it would briefly have a luminosity of more than 200 times that of the Sun. Lower-mass black holes are expected to evaporate even faster; for example, a black hole of mass 1 TeV/c 2 would take less than 10 −88 ...
Ultraman Orb (ウルトラマンオーブ, Urutoraman Ōbu) is a Japanese tokusatsu television series produced by Tsuburaya Productions and broadcast on TV Tokyo. it is the 28th entry to the Ultra Series and released to commemorate its 50th anniversary of the Ultra Series and is the first since Ultra Galaxy Mega Monster Battle: Never Ending Odyssey not to be a part of Ultraman Retsuden/New ...
Black Hole Blessings, which are gained from area bosses, or, optionally, at the run's start, have more powerful beneficial effects, but also a negative effect on the player. The player can sacrifice one of their hearts at shrines to gain a Blessing in return, or choose to recover their health instead.
In addition, Abell 85 has its velocity dispersion of dark matter halo at ~750 km/s, which could be explained only by a black hole with a mass greater than 150 billion M ☉, although Kormendy and Ho et al stated that "dark matter halos are scale-free, and the SMBH-dark matter coevolution is independent from the effects of baryons". [2]
Beyond the Black Hole is a game where the player is a scientific officer placed in charge of investigating some unusual phenomena. The player uses cartography orbs to examine objects in space, with two rebound fields on the left and right edges of the screen to reflect the orb back to the middle.
A blanet is a member of a hypothetical class of exoplanets that directly orbit black holes. [1]Blanets are fundamentally similar to other planets; they have enough mass to be rounded by their own gravity, but are not massive enough to start thermonuclear fusion and become stars.
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The no-hair theorem (which is a hypothesis) states that all stationary black hole solutions of the Einstein–Maxwell equations of gravitation and electromagnetism in general relativity can be completely characterized by only three independent externally observable classical parameters: mass, angular momentum, and electric charge.