General relativity predicts that black hole images ought to display a bright, thin (and as-of-yet-unresolved) ring. This "photon ring" is produced by photons that explore the strong gravity of the black hole, flowing along trajectories that experience extreme light bending within a few Schwarzschild radii of the horizon before escaping. The shape of the photon ring is largely insensitive to the precise details of the emission from the astronomical source surrounding the black hole and therefore provides a direct probe of the Kerr geometry and its parameters. The Black Hole Explorer (BHEX) is a proposed space-based experiment targeting the supermassive black holes M87* and Sgr A* with radio-interferometric observations at frequencies of 100 GHz through 300 GHz and from an orbital distance of ~30,000 km. This design will enable measurements of the photon rings around both M87* and Sgr A*, confirming the Kerr nature of these sources and delivering sharp estimates of their masses and spins.
@article{arxiv.2406.09498,
title = {The Black Hole Explorer: Photon Ring Science, Detection and Shape Measurement},
author = {Alexandru Lupsasca and Alejandro Cárdenas-Avendaño and Daniel C. M. Palumbo and Michael D. Johnson and Samuel E. Gralla and Daniel P. Marrone and Peter Galison and Paul Tiede and Lennox Keeble},
journal= {arXiv preprint arXiv:2406.09498},
year = {2024}
}
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Submitted to SPIE Space Telescopes & Instrumentation