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AntonZensusZhao, Guang-YaoGuang-YaoZhaoZhao, Shan-ShanShan-ShanZhao2022-03-242022-03-2420212397-3366http://hdl.handle.net/20.500.12386/31827Very-long-baseline interferometry (VLBI) observations of active galactic nuclei at millimetre wavelengths have the power to reveal the launching and initial collimation region of extragalactic radio jets, down to 10-100 gravitational radii (r<SUB>g</SUB> ≡ GM/c<SUP>2</SUP>) scales in nearby sources<SUP>1</SUP>. Centaurus A is the closest radio-loud source to Earth<SUP>2</SUP>. It bridges the gap in mass and accretion rate between the supermassive black holes (SMBHs) in Messier 87 and our Galactic Centre. A large southern declination of −43° has, however, prevented VLBI imaging of Centaurus A below a wavelength of 1 cm thus far. Here we show the millimetre VLBI image of the source, which we obtained with the Event Horizon Telescope at 228 GHz. Compared with previous observations<SUP>3</SUP>, we image the jet of Centaurus A at a tenfold higher frequency and sixteen times sharper resolution and thereby probe sub-lightday structures. We reveal a highly collimated, asymmetrically edge-brightened jet as well as the fainter counterjet. We find that the source structure of Centaurus A resembles the jet in Messier 87 on ~500 r<SUB>g</SUB> scales remarkably well. Furthermore, we identify the location of Centaurus A's SMBH with respect to its resolved jet core at a wavelength of 1.3 mm and conclude that the source's event horizon shadow<SUP>4</SUP> should be visible at terahertz frequencies. This location further supports the universal scale invariance of black holes over a wide range of masses<SUP>5,6</SUP>.ELETTRONICOenEvent Horizon Telescope observations of the jet launching and collimation in Centaurus AArticle10.1038/s41550-021-01417-w2-s2.0-85113880625https://www.nature.com/articles/s41550-021-01417-whttps://api.elsevier.com/content/abstract/scopus_id/851138806252021NatAs...5.1017JFIS/05 - ASTRONOMIA E ASTROFISICA