Scientists have used a sophisticated simulation to reconstruct the brutal death of a star that wandered too close to a supermassive black hole and was shredded to bits.
The team, led by researchers from the Hebrew University of Jerusalem’s Racah Institute of Physics, retold the entire story of this so-called tidal disruption event (TDE) for the first time and saw an unknown type of shock wave occur during the gory process. They also found that the dissipation of these shock waves powered an exceptionally intense flare during the event’s brightest weeks.
In addition to explaining the brightest periods of these violent star-destroying events, the findings could help astronomers use TDEs to discover the properties of supermassive black holes, like their mass and rate of spin, and to test the limitations of Einstein’s theory of general relativity.
The findings were published Jan. 17 in the journal Nature.
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Black-hole-destroyed stars get a shock
TDEs happen when a star’s orbit approaches a supermassive black hole with a mass millions or billions of times greater than the mass of the sun. As the star draws close to the supermassive black hole, the black hole’s massive gravitational influence generates immense tidal forces within the star.
This is the result of the gravitational force at the closest hemisphere of the star to the black hole being much greater than that at the farther end. This tidal force causes the star to be stretched vertically while it is squeezed horizontally. This turns the star into a thin strand of stellar plasma in a process known as “spaghettification.”
This spaghettified plasma falls back toward the black hole, and as this happens, it is heated by a series of shock waves. This causes the plasma to fire off a highly luminous flare that can outshine the combined light of every star in the surrounding galaxy for weeks or even months.
The simulation created by Racah Institute of Physics scientists Elad Steinberg and Nicholas Stone gets deeper into TDEs, recreating for the first time the complete picture of these events, from the star being captured by the black hole, through the initial disruption of the star, until the peak of the TDE flare.
This event reconstruction was possible thanks to pioneering radiation-hydrodynamics simulation software developed by Steinberg.
The cosmic crime scene investigation revealed a previously unknown type of shock wave occurring during the TDE, showing that these events dissipate energy at a faster rate than scientists thought. This finding told the team that the brightest periods of the TDE are powered by these shock waves and the associated energy dissipation.
According to the researchers, astronomers could continue to explore the mechanics of these powerful shock waves using real-world observations of the violent encounters between supermassive black holes and doomed stars.