Chile. The TAO Project (Atacama Observatory of the University of Tokyo) was built to explore the depths of the universe from one of the highest points on the planet and in the process redefined the limits of modern astronomy.
The result of a solid international collaboration led by the Institute of Astronomy of the University of Tokyo and involving Japanese institutions such as the National Astronomical Observatory and ISAS/JAXA, as well as the Department of Astronomy of the University of Chile, the TAO Project represents a success in the exploration of the universe from the top of the Andes mountain range.
After more than two decades of development, this 6.5-meter-diameter telescope is now strategically located on Chajnantor Hill, allowing astronomical observations without significant interference.
Contribution of the Mayekawa Group
One of the most important challenges for the construction of the TAO telescope was to control the temperature of the so-called primary mirror.
Therefore, and to ensure accurate observations while minimizing thermal distortions, it was decided to install the N2K cooler, developed by the company Mayekawa.
This advanced terrestrial cooling system maintains the thermal stability of the space, which also optimizes performance, allowing high-precision astronomical investigations to be carried out.
With industrial refrigeration solutions such as the N2K Chiller, Project TAO ensures ideal conditions for your operations.
Scientific objectives
The telescope consists of two scientific instruments designed to explore the universe in the infrared: Swims and Mimizuku. Swims focuses on photographing galaxies, investigating their formation, while Mimizuku is dedicated to the study of primordial disks around the stars where planets are born. Both instruments have the potential to revolutionize the understanding of the cosmos, offering unique perspectives on invisible regions of space.
Impact and potential
The TAO Project in the field represents a technological and scientific breakthrough, as well as an example of international cooperation and excellence in astronomical research. Its strategic location on Cerro Chajnantor in Chile, combined with an advanced cooling system for the primary mirror, stands out as a significant achievement in the search for high-precision astronomical observations, free of thermal distortions that could compromise the quality of the data collected.
"We are proud to contribute to this innovative project and excited about the future revelations they will bring to humanity," said the Mayekawa Group.
