The Subaru Telescope is a large optical-infrared telescope located on Mauna Kea, Hawaii. It is operated by the National Astronomical Observatory of Japan and features an 8.2-meter primary mirror for detailed astronomical observations.
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The Subaru Telescope was inaugurated in 1999 and has been instrumental in numerous astronomical discoveries.
It utilizes advanced adaptive optics to correct distortions caused by Earth's atmosphere, resulting in clearer images.
Due to its location at 4,200 meters above sea level on Mauna Kea, it benefits from minimal light pollution and stable atmospheric conditions.
The telescope's instruments include the Hyper Suprime-Cam, which provides wide-field imaging capabilities.
Subaru collaborates with various international observatories, contributing significantly to global astronomical research.
Review Questions
What is the primary function of the Subaru Telescope?
How does the Subaru Telescope mitigate atmospheric distortions?
Why is the location of the Subaru Telescope advantageous for astronomical observations?
Related terms
Mauna Kea Observatories: A group of astronomical research facilities located on Mauna Kea, providing optimal observing conditions due to high altitude and low light pollution.
Adaptive Optics: Technology used in telescopes to reduce atmospheric distortion and produce clearer images.
Hyper Suprime-Cam: An instrument mounted on the Subaru Telescope that captures wide-field images with a high degree of detail.