The Herald (South Africa)

Astronomer­s identify second-largest known Milky Way black hole

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Astronomer­s have discovered a black hole with a mass about 33 times greater than our sun, the biggest one known in the Milky Way aside from the supermassi­ve black hole lurking at the centre of our galaxy.

The newly identified black hole was located about 2,000 light-years from Earth — relatively close in cosmic terms — in the constellat­ion Aquila, and had a companion star orbiting it, researcher­s said on Tuesday.

A light year is the distance light travels in a year, 9.5-trillion kilometres.

Black holes are extraordin­arily dense objects with gravity so strong that not even light can escape, making it difficult to spot them.

This one was identified through observatio­ns made in the European Space Agency’s Gaia mission, which is creating a huge stellar census, because it caused a wobbling motion in its companion star.

Data from the European Southern Observator­y’s Chilebased Very Large Telescope and other ground-based observator­ies were used to verify the black hole’s mass.

“This black hole is not only very huge, it is also very peculiar in many aspects. It is really something we never expected to see,” said Pasquale Panuzzo, a research engineer at the French agency CNRS working at the Observatoi­re de Paris and lead author of the study published in the journal Astronomy & Astrophysi­cs.

For instance, the black hole, called Gaia BH3, and its companion are travelling within the galaxy in the opposite direction of how stars typically orbit in the Milky Way.

Gaia BH3 probably formed after the death of a star more than 40 times as huge as the sun, the researcher­s said.

Black holes that result from the collapse of a single star are called stellar black holes.

Gaia BH3 is the largestkno­wn stellar black hole, according to astronomer and study co-author Tsevi Mazeh of the Tel Aviv University in Israel.

Stellar black holes are dwarfed in size by the supermassi­ve black holes inhabiting the centre of most galaxies.

One such black hole, Sagittariu­s A* or Sgr A*, is located at the heart of the Milky Way.

It possesses four-million times the mass of our sun and is located about 26,000 lightyears from Earth.

Gaia BH3’s progenitor star was composed almost entirely of hydrogen and helium.

Stars in the early universe had such a chemical compositio­n, known as low metallicit­y.

This star had formed relatively early in the universe’s history — perhaps two-billion years after the Big Bang event.

When that star exploded at the end of its lifespan — called a supernova — it blasted some material into space while the remnant violently collapsed to form a black hole.

The discovery of Gaia BH3, according to Panuzzo, supports stellar evolution models showing that huge stellar black holes can be produced only by a low metallicit­y star like this one’s progenitor star.

Gaia BH3’s companion star, just as old as the other one was, is about 76% of the mass of the sun and a bit colder, but about 10 times more luminous.

It orbits the black hole on an elliptical path at a distance varying between about 4.5 times the distance between Earth and the sun.

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