combat-ready black holes are surrounded by disks of material and can spewpowerful jets . These jets , in number , can liberate powerful X - rays . And some of those XTC - rays will shine downwards towards the black hole and disk . In the disk they can get reflected , create anechothat uranologist call X - ray reverberation . Such a signal can be used to do some pretty astonishing science .

Basically , astronomers are looking at the direct photon give off by the super C and then looking at how the same light is reflected off the disc . This reverberation does n’t happen all at the same time because the focal ratio of brightness level is finite . So the reflexion will start in the inmost part of the disk , and the signal will ripple outwards as the tenner - rays from the jet need more prison term to reach the outer parts of theaccretion saucer .

“ imagine of it as a lamppost suspended some distance above the black hollow . This lamppost flash and sends photons out in all direction . Those directly emitted ace will reach us before the ones that spring off the disc to get through us . This is just due to a unlike way of life distance , ” research worker Dr Patrick O’Neill , from the University of Newcastle , distinguish IFLScience .

Schematic of the reflection process in the black hole Cygnus X-1. The light emitted from the jet is shown in blue, which we say originates from a point source some distance above the black hole. The X-rays following path a) are observed directly by our telescopes. The light that follows paths (labelled b & c), reflect off the disc and follow the green trajectories to reach us. Light travelling along a) follows the shortest path to reach us, whereas the light travelling along path c) takes the longest path, and therefore takes the longest time to reach us.

The X-rays from the jet can reach us directly or be reflected off the disk on paths of different lengths.Image credit: Patrick O’Neill. Background image: NASA/JPL-Caltech

“ But the record is not itself a undivided point , it ’s in reality get some width to it . So not only is this signal lagging behind the direct photons , they are lagging behind as a function of how far it needs to move to the disk to be ponder . ”

The attack is a manner to independently measure out the mass and the aloofness of the contraband hole and it is not affected by the dusty regions in the centre of attention of galaxies , as X - irradiation wing right through them without being absorb . The technique was tested successfully onCygnus X-1 , the first ex - ray source to be recognise as a sinister cakehole .

There are two exciting things that this can be used for . A circumstances of astronomical disastrous hole are get hold above the planets of the Milky Way , as it is easy to spot them where it is not crowded , standardised to the oldest stars . But the pitch-black holes that are there are the lighter ones , those that were given a rush by companion star go supernova . Heavier black trap are to be regain around the center of the Milky Way and by front at theseechoes , the team hopes to recover them .

And stellar - sized black holes do not only exist in the Milky Way . The power to measure distance and mass , without having to vex about the detritus in the room , is also appealing for the field of supermassive black maw at the center of distant galaxies .

“ This   can   be   applied   to   supermassive   pitch-dark   kettle of fish   really ,   really   far   away   and   we   can   apply   that   to   probe the   elaboration   of   the   universe   in   a   unlike   way , ” Dr O’Neill continued .

There is currently amajor tensionin the estimate for the expansion rate of the creation . If you use the cosmic microwave oven background knowledge ( CMB ) , the utmost light that can be keep in the universe , you get one number . If you practice supernovae as standard candles to mensurate the distance of much close – but still aloof – galaxies , you get another bit .

“ This is a new set of standard taper that we can use to probe the Hubble constant that does n’t rely on supernovae or temperature wavering from the CMB , ” Dr O’Neill told IFLScience .

The research was present at theNational Astronomical Meeting 2023 .