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Study confirms excellent astronomical potential of Muztagh Observation Station

New study confirms excellent astronomical potential of Muztagh Observation Station
Left: The 10-m tower at North-2 site. Right: The French DIMM and PC-4A environmental monitoring instrument. Credit: Monthly Notices of the Royal Astronomical Society (2025). DOI: 10.1093/mnras/staf1210

A new systematic study of the atmospheric conditions at the Muztagh Station in western China has revealed the site's unique suitability for optical observations. Researchers from the Xinjiang Astronomical Observatory of the Chinese Academy of Sciences reported that the location offers excellent "seeing" conditions, making it ideal for high-precision optical observations. The findings were in the Monthly Notices of the Royal Astronomical Society.

As starlight travels through Earth's atmosphere, it is affected by optical , which causes fluctuations in the and distorts the optical wavefront, thereby degrading a telescope's imaging quality. "Seeing" reflects the degree to which stellar images are blurred and jittered by atmospheric optical turbulence, and is one of the core indicators used to evaluate the quality of an site.

The study, led by Ph.D. candidate Gu Wenbo with his advisor Prof. Ali Esamdin and colleagues analyzed seeing and collected from 2018 to 2024 at the station's North-1 and North-2 points. Using a Differential Image Motion Monitor (DIMM), a 30-meter meteorological tower, and a PC-4A automatic weather system, the researchers measured key parameters for the Muztagh Observatory, including seeing, temperature, , and wind direction.

Results show that the seeing conditions at the Muztagh Station are excellent. The median seeing is 0.78 arcseconds at the North-2 point at a height of 10 meters, and 0.89 arcseconds at the North-1 point at a height of 6 meters. Simultaneously, the site has a small nighttime ground-surface temperature difference (about 2°C), moderate wind speed (median value of 5–6 m/s), and a stable, dominant wind direction (southwest).

The researchers also examined the relationship between wind dynamics and optical clarity. They found a significant "U-shaped" correlation between seeing and wind speed, where moderate wind speeds are most favorable for suppressing atmospheric turbulence and optimizing seeing. Airflow from the dominant wind direction usually brings better seeing, whereas strong vertical wind shear and short-term, drastic fluctuations in wind speed will significantly enhance atmospheric turbulence, leading to a deterioration in seeing.

With its excellent near-ground turbulence environment and seeing conditions, the Muztagh Station shows great potential to become an outstanding optical astronomical observatory site in western China.

More information: Wenbo Gu et al, Seeing and meteorological analysis at the North-1 and North-2 points of Muztagh-Ata site on the Pamir Plateau, Monthly Notices of the Royal Astronomical Society (2025).

Citation: Study confirms excellent astronomical potential of Muztagh Observation Station (2025, September 4) retrieved 8 September 2025 from /news/2025-09-excellent-astronomical-potential-muztagh-station.html
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