Artificial Stars in the Atacama
A striking new photograph released by the European Southern Observatory captures one of modern astronomy's most visually arresting technologies in action: powerful laser beams lancing upward from the Very Large Telescope at the Paranal Observatory in Chile, creating glowing artificial stars in the upper atmosphere against the sweeping backdrop of the Milky Way. The image, captured by Chilean astrophotographer Alexis Trigo, has been selected as Space Photo of the Day for February 17, 2026, and it offers a vivid illustration of how ground-based observatories are overcoming the fundamental limitation that has challenged astronomers since Galileo first turned a telescope skyward.
The photograph shows multiple orange-yellow laser beams projecting from the telescope units into the clear desert sky, each one terminating in a tiny bright point high in the atmosphere. These artificial guide stars, created by exciting sodium atoms in a layer of the atmosphere roughly 90 kilometers above the Earth's surface, serve as reference points for an adaptive optics system that corrects for the constant blurring caused by atmospheric turbulence.
How Laser Guide Stars Work
The principle behind laser guide stars is elegant in its conception if technically demanding in its execution. Earth's atmosphere, while essential for life, is a persistent nuisance for astronomers. Pockets of air at different temperatures and densities constantly shift and swirl above any telescope, bending light rays in slightly different directions from moment to moment. This atmospheric turbulence is what makes stars appear to twinkle to the naked eye, a phenomenon that is charming for casual stargazers but devastating for precise astronomical imaging.
To counteract this effect, the Very Large Telescope projects sodium laser beams into the sky, targeting a thin layer of sodium atoms that exists at an altitude of approximately 90 kilometers. These sodium atoms are remnants of meteors that have burned up in the atmosphere, leaving behind a persistent metallic layer. When the laser light hits these atoms, they fluoresce, creating a bright point source that functions as an artificial star.
The adaptive optics system then monitors this artificial star hundreds of times per second, measuring exactly how the atmosphere is distorting its light at any given instant. A computer processes these measurements in real-time and sends commands to a deformable mirror, a flexible mirror that can change its shape many times per second to compensate for the atmospheric distortion. The result is images with a level of sharpness that approaches what could be achieved from space, effectively removing the atmosphere from the equation.
- The photograph was captured by astrophotographer Alexis Trigo at the Paranal Observatory in Chile's Atacama Desert
- Laser guide stars work by exciting sodium atoms at approximately 90 kilometers altitude, remnants of burned-up meteors
- Adaptive optics systems measure atmospheric distortion hundreds of times per second and correct it in real-time
- Three additional Unit Telescopes received laser upgrades in December 2025 to support the VLTI and GRAVITY+ instruments
- The technology allows ground-based telescopes to achieve image clarity approaching that of space-based observatories








