The finding tracks the star - about the size of our Sun - as it shifts from its customary path, slips into the gravitational pull of a super massive black hole and is sucked in, said Sjoert van Velzen, a Hubble fellow at the Johns Hopkins University in US.
"It's the first time we see everything from the stellar destruction followed by the launch of a conical outflow, also called a jet, and we watched it unfold over several months," van Velzen said.
Astrophysicists had predicted that when a black hole is force-fed a large amount of gas, in this case a whole star, then a fast-moving jet of plasma - elementary particles in a magnetic field - can escape from near the black hole rim.
This study suggests this prediction was correct, the scientists said.
Super massive black holes, the largest of black holes, are believed to exist at the centre of most massive galaxies.
The first observation of the star being destroyed was made in December last year. Researchers used radio telescopes to follow up as fast as possible. They were just in time to catch the action.
By the time it was done, the team had data from satellites and ground-based telescopes that gathered X-ray, radio and optical signals, providing a stunning "multi-wavelength" portrait of this event.
It helped that the galaxy in question is closer to Earth than those studied previously in hopes of tracking a jet emerging after the destruction of a star.
The first step for the international team was to rule out the possibility that the light was from a pre-existing expansive swirling mass called an "accretion disk" that forms when a black hole is sucking in matter from space.
That helped to confirm that the sudden increase of light from the galaxy was due to a newly trapped star.
"From our observations, we learn the streams of stellar debris can organise and make a jet rather quickly, which is valuable input for constructing a complete theory of these events," van Velzen said.
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