Stellar pancaking is a phenomenon that occurs when a star's orbit around a black hole becomes highly eccentric, causing the star to become stretched and flattened, resembling a pancake.
Stellar pancaking is caused by the intense gravitational pull of a black hole. The black hole's gravitational force distorts the star's orbit, causing it to become highly elongated and flattened.
Yes, stellar pancaking can be observed using telescopes that are sensitive to X-rays. As the star is stretched and flattened, it emits X-rays that can be detected by these telescopes.
Stellar pancaking is not dangerous for humans, as it occurs in distant galaxies. However, it can be dangerous for the star itself, as it can lead to the star being eventually torn apart by the black hole's gravitational pull.
Stellar pancaking can affect the black hole by providing it with additional material to feed on. As the star is stretched and flattened, its outer layers can be pulled into the black hole, increasing its mass and energy.