Until now, we thought about supermassive black holes like the immovable anchors of galaxies, being gravitational giants that keep everything in order from the center. But we were quite wrong, since the James Webb Space Telescope us has confirmed that, sometimes, these anchors break and are shot through intergalactic space as if they were real gun bullets.
The study. A team led by astronomer Pieter van Dokkum of Yale University has presented the first observational confirmation of a wandering supermassive black hole. It is called RBH-1 and its existence is the result of one of the most violent events that physics allows: being “kicked” out of your home by gravitational waves.
A scar. Detecting this is not easy, since black holes They cannot be seen with the naked eye, but the destruction they leave in their wake is analyzed. This is precisely what JWST saw when it detected a massive linear structure about 200,000 light years long (twice the diameter of the Milky Way), which connects a distant galaxy with a bright, fuzzy spot.
After trying to analyze this destruction in more detail, the telescope itself has revealed that it is a discontinuity. In layman’s terms: there is something extremely massive moving at an absurd speed of 954 km/s, which is equivalent to 3.4 million kilometers per hour. A speed that would allow us to travel from the Earth to the Moon in less than seven minutes.
How do we know? The question in this case seems obligatory: How do we know that it is a black hole and not a simple star formation? The answer lies in everything it leaves in its wake, since by moving at this type of high speed, the black hole It compresses the gas so violently that it generates a trail of hot plasma that can be measured, as well as the formation of new stars.
And now science has been able to confirm that this gas is not heated by the light emitted by stars, but by the brutal collision of a target that has at least 10 million times the mass of the Sun.
Why is he running away? The theory behind this phenomenon is not new, but has been predicted by general relativity for 50 years. But in order to understand what has happened here, we can see it in three different steps:
- The first thing that happened was the merger of two galaxies and their respective supermassive black holes that began to orbit each other.
- After this, a third galaxy arrives to join this party and its black hole interacts with the binary system formed before.
- Finally, a cosmic “kick” is given. In this case, the interaction of three bodies generates a great asymmetry in the gravitational waves that results in a black hole shooting out of the galaxy at a high speed.
It’s not the first. We already knew about wandering “stellar mass” black holes (a few times the mass of the Sun) roaming our own Milky Way, detected by gravitational microlensing effects by Hubble or the Gaia mission. However, finding a supermassive, what is the type of object that usually lives in the heart of galaxies, is a milestone on a different scale.
Why this matters. The confirmation of RBH-1 is not a simple curiosity for physicists, but validates models of galactic evolution that suggest that the universe is full of these ‘exiles’. And this shows that if supermassive black holes can be ejected so easily, it means that many galaxies could be “orphaned” of their central core, affecting how they grow and form stars.
Images | NASA Hubble Space Telescope
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