Faceonmerger_frame_watermarked

Simluation of a black hole merger with asymmetric masses and orbital precession, consistent with GW190412

A still image from a numerical simulation of a black-hole binary merger with asymmetric masses and orbital precession. Credit: N. Fischer, H. Pfeiffer, A. Buonanno (Max Planck Institute for Gravitational Physics), Simulating eXtreme Spacetimes (SXS) Collaboration.