Measuring an asteroid’s mass is difficult, yet it is central to assessing potential impact consequences and estimating available resources. Current approaches typically rely on optical observations and then infer density from spectral characteristics, which introduces uncertainty. Two outlets report on a new concept that aims to address this by repurposing ideas from the Laser Interferometer Space Antenna (LISA) flagship mission. The proposal suggests that LISA’s laser-based sensing could be used to derive highly accurate mass estimates for nearby asteroids without changing LISA’s hardware. The core idea is to use laser interferometry in a way that links the asteroid’s gravitational effect (or related interaction with the measurement) to its mass, providing a more direct measurement than density inferred from spectra. As described in the reports, the method would apply to comparatively close asteroids, where the signal effect on LISA measurements could be detectable. The proposal focuses on asteroid characterization and emphasizes that it would leverage LISA technology rather than requiring additional instruments or modifications to the mission.