21–25 Oct 2025
Veras gräsmatta, Chalmers, Gothenburg
Europe/Stockholm timezone

Time-Resolving Sgr A* at 86 GHz via Low-Earth Orbit VLBI

24 Oct 2025, 11:55
20m
Veras gräsmatta, Chalmers, Gothenburg

Veras gräsmatta, Chalmers, Gothenburg

Stena Center Läraregatan 3 411 33 Göteborg Phone: +46 (0)31-797 20 70 Email: info@stenacenter.se
Talk Sessions

Speakers

Ms Amelia Frickey (Brown University)Mr Graham Neely (Brown University) Ref Bari (Brown University)

Description

T-REX (Time-Resolving Explorer) is a proposed SmallSat which seeks to time-resolve the accretion disk of Sgr A through direct radio interferometric imaging utilizing VLBI -- enabling the first constraints on black hole spin. T-REX will operate in Low-Earth Orbit (LEO) at 86 GHz (𝜆 ∼ 3.5𝑚𝑚) with a 𝑑 ∼ 2.5𝑚 antenna. It will co-observe with BHEX (Black Hole Explorer) in MEO and the EHT (Event Horizon Telescope) in a unique MEO-LEO-Ground "sandwich" configuration. If successful, T-REX would be the first demonstration of Space-Space VLBI (between BHEX and T-REX). Additionally, unlike BHEX which has only long baselines (> 20𝐺𝜆) which can reveal horizon- scale structure of Sgr 𝐴/M87 (but which is not as adept at observing larger-scale structure like jets), T-REX will benefit from both a long Space-Space Baseline (BHEX to T-REX) and a shorter, Space-Ground Baseline (T-REX to EHT). T-REX is thus uniquely positioned to access both horizon-scale and extended jet-structure morphology of low-accretion state black hole targets. T-REX’s primary science objective is to leverage this orbital structure to time-resolve Sgr A, effectively creating the first ever video of a black hole. In addition to this ambitious goal, T-REX plans to conduct an all-sky survey of ∼ 25 targets, potentially enabling multi-messenger astronomy on binary black hole systems, quasars, and black hole accretion disks.

Author

Ms Amelia Frickey (Brown University)

Co-author

Mr Graham Neely (Brown University)

Presentation materials

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