![ESO on Twitter: "2/ The new images zoom in 20 times more than what was possible before the VLTI and have helped astronomers find a never-before-seen star close to the black hole: ESO on Twitter: "2/ The new images zoom in 20 times more than what was possible before the VLTI and have helped astronomers find a never-before-seen star close to the black hole:](https://pbs.twimg.com/media/FGkXXyFWYAk7eqn.jpg:large)
ESO on Twitter: "2/ The new images zoom in 20 times more than what was possible before the VLTI and have helped astronomers find a never-before-seen star close to the black hole:
![Gravity model (ratio of the number of VLT sites and males 19–44 years... | Download Scientific Diagram Gravity model (ratio of the number of VLT sites and males 19–44 years... | Download Scientific Diagram](https://www.researchgate.net/publication/5645545/figure/fig10/AS:213927616094237@1428015726710/Gravity-model-ratio-of-the-number-of-VLT-sites-and-males-19-44-years-of-age-The.png)
Gravity model (ratio of the number of VLT sites and males 19–44 years... | Download Scientific Diagram
![First wavefront sensor for GRAVITY installed at Paranal Observatory | Max-Planck-Institut für Astronomie First wavefront sensor for GRAVITY installed at Paranal Observatory | Max-Planck-Institut für Astronomie](https://www.mpia.de/4492923/original-1518438505.jpg?t=eyJ3aWR0aCI6MzQxLCJmaWxlX2V4dGVuc2lvbiI6ImpwZyIsIm9ial9pZCI6NDQ5MjkyM30%3D--579ca1adf7dec51cae77b2eab5879801f83130ad)
First wavefront sensor for GRAVITY installed at Paranal Observatory | Max-Planck-Institut für Astronomie
![Mass distribution in the Galactic Center based on interferometric astrometry of multiple stellar orbits - CERN Document Server Mass distribution in the Galactic Center based on interferometric astrometry of multiple stellar orbits - CERN Document Server](https://cds.cern.ch/record/2806198/files/figure1.png)