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This sequence of images, taken with the GRAVITY instrument at ESO’s Very Large Telescope Interferometer (VLTI), show several stars orbiting Sagittarius A*, the supermassive black hole at the centre of our galaxy. One of these stars, known as S301, was recently found to pass much closer to the black hole than any other known star. S301 orbits Sagittarius A* every 8.7 years. At its closest approach — similar to the distance between the Sun and Saturn — the star moves at more than 8% the speed of light. The size of Neptune’s orbit is shown as a reference. S301 passes so close to Sagittarius A* that its orbit could be affected by the rotation of the black hole, which twists space-time around it. The effect is small, but could be potentially measured in the next few years with the VLTI and ESO’s Extremely Large Telescope (ELT), currently under construction. The orbit of S301 is displayed here with an elliptical curve. In each frame, the solid curve shows the path that the star has already completed up to that point, whereas the dashed one marks the path it will follow afterwards.