The Event Horizon Telescope (EHT) captured the first image of a black hole in 2019, providing direct confirmation of the existence of black holes. BHEX Mini (Black Hole Explorer Mini) is a satellite mission which seeks to take the next leap: Capturing the first video of a black hole. BHEX Mini will be an 87 kg, $25 milion radio satellite in low-earth orbit operating at 86 GHz. It will conduct a targeted survey of >25 secondary science targets, enabling population studies of supermassive black hole masses, spins, and luminosities. By virtue of orbiting in LEO, BHEX Mini would enable rapid and dense interferometric coverage for Sgr A* & M87 at 86 GHz, advancing direct imaging of the photon ring. If successful, BHEX Mini would also be the first satellite to achieve Space-Space VLBI by co-observing targets with BHEX in MEO.
Simulations created by the BHEX Mini team to constrain SWaPC requirements and the feasibility of Primary Science Objectives. All of our code is open-source.
Using Ben Hudson's SpaceVLBI library to simulate (u,v) coverage for BHEX Mini at 86 GHz. Currently supports only Space-Ground baselines and single-frequency observations.
Using Aditya Tamar's approach to simulate the impact of ISM scattering on BHEX Mini's observations of Sgr A* at 86 GHz.
Determining Duty Cycle of BHEX Mini given Quantization Scheme (1-bit or 2-bit), and amount of ground contact during LEO orbit.
This notebook calculates the visibility amplitude for 25 Secondary Science Targets (SSTs), the Thermal Noise Constraint on the Space-Space & Space-Ground baseline, and the Antenna Diameter.
Calculates Minimum Integration Time for BHEX Mini, given a target thermal noise floor and SEFD (System Equivalent Flux Density).
Simulates the amount of time required for BHEX Mini to rotate by an angle θ to point at a new radio target, given the maximum spin rate, moment of inertia, and net torque.