The Canada-France-Hawaii Telescope (CFHT), operational since 1979, is a 3.6-meter diameter astronomical instrument located at an altitude of 4204 meters on the Mauna Kea volcano in Hawaii. The result of a collaboration between Canada, France, and the University of Hawaii, it embodies an example of international scientific cooperation in astronomy. The choice of Mauna Kea is not random: its atmospheric conditions—stability, low humidity, absence of light pollution—make it one of the best astronomical observation sites in the world.
Equipped with a 3.6-meter hyperbolic primary mirror, the CFHT was one of the first telescopes to fully exploit the technique of active optics, ensuring the stability of its surface to within a few tens of nanometers. Thanks to a thermally very stable dome and a compact structure, it significantly reduces internal turbulence. It is equipped with several cutting-edge instruments, including:
The CFHT has played a fundamental role in several key areas:
The operation of the CFHT takes place in a sensitive cultural and environmental context. Mauna Kea is a sacred site for Hawaiians, and strict protocols aim to minimize the impact of scientific infrastructure on the ecosystem and local traditions. The CFHT is thus part of an approach of respectful science, attentive to the human and natural dimensions of its environment.
For over four decades, the CFHT has contributed to major scientific breakthroughs in astronomy.
Thanks to the stability of its instruments, its exceptional sky, and the longevity of its observation programs, the CFHT remains one of the most prolific telescopes in the fields of cosmology, stellar physics, and planetary formation.
Scheduled for conversion in the coming years, the CFHT is expected to evolve into the MSE (Maunakea Spectroscopic Explorer) project: an 11-meter spectroscopic telescope dedicated to the study of the large structures of the universe. This transition, supported by the international scientific community, will make it possible to take advantage of the existing infrastructure while pushing the limits of multi-object spectroscopy.
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