Why do Astronomers Use Lasers in Observations

When observing the universe from Earth, astronomers face a major challenge: Earth’s atmosphere. Turbulence in the atmosphere causes incoming light from stars and galaxies to bend slightly in random ways, making celestial objects appear blurred or to “twinkle.” To overcome this problem, many modern observatories use lasers as part of adaptive optics systems to sharpen astronomical images.

On 26 April 2016, an event at ESO’s Paranal Observatory in Chile marked the brilliant first light for the four powerful lasers that form a crucial part of the adaptive optics systems on ESO’s Very Large Telescope. Attendees were treated to a spectacular display of cutting-edge laser technology against the majestic skies of Paranal. These are the most powerful laser guide stars ever used for astronomy and mark the first use of multiple laser guide stars at ESO. This image shows the four beams emerging from the new laser system on Unit Telescope 4 of the VLT.
ESO’s Paranal Observatory in Chile

Astronomers fire a powerful yellow laser beam into the sky to create an artificial reference point known as a laser guide star. The laser excites a thin layer of sodium atoms about 90 km above Earth in the mesosphere. These atoms absorb the laser light and re-emit it, producing a glowing spot in the sky that acts like an artificial star.

Because this “star” is created by the telescope itself, astronomers always know its exact position. Once the artificial star is created, the telescope measures how its light is distorted by atmospheric turbulence. A computer then calculates how the atmosphere is bending the light and sends commands to a deformable mirror inside the telescope. This mirror changes its shape hundreds or even thousands of times per second, canceling out the distortion.

As a result, the telescope can produce much sharper images, approaching the clarity of space telescopes.

Improving Ground-Based Telescopes

Without adaptive optics and laser guide stars, ground-based telescopes would suffer from blurred images caused by atmospheric effects. By using lasers, astronomers can achieve near space-quality resolution while operating from Earth’s surface. This technique allows scientists to study distant galaxies, observe stars forming in nebulae, and even image exoplanets around nearby stars.

By creating artificial guide stars and enabling adaptive optics systems, Lasers allow telescopes on Earth to overcome atmospheric distortion and observe the universe with remarkable precision. This technology helps astronomers capture clearer images and make more accurate measurements of distant cosmic objects.

Tsiyon Hone

Tsiyon Hone

Tsiyon is an aspiring astrophysicist and lover of the night sky. She strives to blending science and communication in the global scientific community . She has a deep interest in explosion of binary stars and supernovae.

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