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Astronomers have discovered a new main sequence star that’s the fastest of its kind ever found in the Milky Way. It’s hurtling through the galaxy at an eye-popping speed of around 1,700 kilometres per second, and it’s racing away from the centre of the galaxy.
This also makes it the first star that astronomers can confidently identify as having been ejected from the galactic centre. That means it was probably booted out by an interaction with the supermassive black hole therein, the colossus Sagittarius A* (Sgr A*).
S5-HVS1, as researchers have named the star, is pretty interesting. It’s a main-sequence, or “living” star that is still undergoing hydrogen fusion in its core; in fact, it’s relatively young, up to just 500 million years old.
It’s an A-type star around 2.35 times the mass of the Sun, and shining quite brightly. These characteristics make it a real oddball, as stars go.
That’s because these fast-moving stars – known as hypervelocity stars, or HSVs – are quite rare, but according to a 2015 analysis, those in the main sequence tend towards O- and B-type stars: very hot and massive ‘live fast and die young’ stars that don’t live more than a few tens of millions of years.
There are also hypervelocity ‘dead’ stars, or neutron stars, like the previous speed record-holder, RX J0822−4300, with an apparent velocity over 1,500 kilometres per second – a record speed when it was first calculated in 2006.
But those stars have a clearer origin: when a dying star goes supernova, the explosion can be asymmetrical, ejecting the star itself out into space at insane speeds. For the white dwarfs, a double detonation, where both stars go kaboom, is believed to be responsible.
Before S5-HVS1 (the discovery of which is still awaiting peer review), the current undisputed fastest known main sequence star in the galaxy was US 708, at 1,200 kilometres per second. It’s an O-type. S5-HVS1 blows it out of the water.
But without an explosion, how do main sequence stars get kicked into such insane speeds? Well, that’s where the black holes come in.
Astronomers think that the hypervelocity main sequence stars identified to date could have been ejected into space via three-body exchange interactions, where one of the bodies is a black hole, and the other two are stars in a binary system.
(Take a breather and watch this beautiful animation of a three-body system set to sound.)
“Three-body exchange interactions among stars and a massive black hole inevitably unbinds stars from a galaxy,” wrote astronomer Warren Brown of the Harvard Smithsonian Centre for Astrophysics in 2015.
“Because stars have finite sizes, only a massive compact object can explain stars ejected at 1,000-km s−1 velocities.”
S5-HVS1’s position, roughly 29,000 light-years away from Earth, and the speed with which it’s moving, indicates it was kicked out of the galactic centre about 4.8 million years ago. It’s been hurtling across space ever since – but the mechanism that kicked it out is a little less clear.
For a three-body exchange interaction to have occurred, according to the paper, one of the stars would have had to have been relatively low mass, less than the mass of the Sun, locked in a short-period orbit with S5-HVS1 – lasting between 3 and 40 days.
Although these binaries would be rare, they are possible. An accretion event a few million years ago could have kicked off star formation in the galactic centre, producing the S5-HSV1 binary. Its trajectory is curiously aligned with a disc of these stars, which could indicate that’s where it originated.
It’s also possible that Sgr A* gobbled up one of the stars, ejecting S5-HVS1 out into the galaxy at a velocity of around 1,800 kilometres per second.
Still another possibility is that an intermediate black hole in the galactic centre merged with Sgr A* a few million years ago. The dynamical friction at the last stages of its inspiral could have kicked a bunch of stars out of the galactic centre.
Although there is little evidence of such an event, it could be investigated by searching for more hypervelocity stars ejected at the same time as S5-HVS1.
There’s also still more to learn about the star itself. A new release of Gaia data – a project to map the galaxy in three dimensions at the highest level of accuracy and detail ever – is expected at the end of 2021.
This will provide more information on S5-HVS1’s velocity and trajectory, give us more precise measurements and refining our understanding of its strange history.
The research has been submitted to the Monthly Notices of the Royal Astronomical Society, and is available on the pre-print website arXiv.