Researchers report a method to increase the sensitivity of gravitational-wave detectors such as LIGO by using an ordinary thermal imaging camera focused on the observatory’s mirrors. The approach addresses limitations caused by heat and thermal effects that influence the mirrors, helping detectors better account for or compensate these sources of noise. The work indicates the technique could improve LIGO’s next planned upgrade by up to about 31%, which would extend the detector’s effective reach for events such as neutron star collisions to significantly greater distances—tens of millions of light-years farther, according to the reports. The same sources also say the method is already incorporated into the design of Cosmic Explorer, a planned next-generation gravitational-wave observatory. Overall, the proposal is presented as a relatively straightforward, lower-complexity addition compared with developing entirely new detector hardware, relying instead on commercially available thermal camera technology aimed at existing components of the interferometer.