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Astronomy: Laser Telescope Boosts Viewing Power

Astronomy: Laser Telescope Boosts Viewing Power

November 11, 2025 Lisa Park Tech

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Main topic: Improvements to ‌the Very large Telescope Interferometer ‍(VLTI) using laser guide stars and adaptive optics, specifically thru the GRAVITY+ project.

Key Points:

* Laser Guide Stars: Four new lasers have been implemented at the VLTI.These lasers create artificial “reference stars” in the‌ sky by‍ stimulating sodium⁢ atoms in the upper atmosphere (90km altitude).
*​ Adaptive Optics: these artificial⁢ stars are used by adaptive optics systems to measure and⁤ correct for atmospheric turbulence. This⁢ results in significantly sharper‍ astronomical images.
* Expanded Observational Range: Previously, atmospheric correction relied on naturally shining stars near the target. The laser guide stars allow for observations​ of any region of the sky, greatly expanding ‌the ‍VLTI’s capabilities.
* GRAVITY+ Project: The project ‍responsible for these improvements is called GRAVITY+.
* First Results: The system was tested on a cluster ⁤of massive stars‌ in a neighboring galaxy. It revealed that a previously thought single star is actually a binary star system.
* Interferometry: The VLTI​ uses interferometry, combining data ⁣from multiple telescopes to achieve higher resolution. this is similar to techniques used in radio​ astronomy but more challenging in the optical spectrum.
* Previous Success: Interferometry was successfully used in 2021 to image stars orbiting the‍ Milky Way’s⁣ central black hole.

In essence: The​ VLTI has been significantly upgraded with laser guide star technology,enabling sharper images and a wider range of observable targets. ‍This advancement, driven by the GRAVITY+ project, promises to unlock new discoveries in astronomy.

Image Description:

The image shows a double star system ‍within the Tarantula Nebula, detected using the GRAVITY+ instrument. The image is credited to the ​ESO/GRAVITY+ Collaboration, with background images from various sources (ESO/IDA/Danish 1.5 m/R. Gendler, C. C. Thöne, C. Féron, and J.-E. Ovaldsen/P. Crowther/C.J. Evans). The image is available in different resolutions‌ (696w,1008w,1392w).

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