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Observational Astronomy Lab
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A radio astronomy lab that explores the distant universe with a terahertz telescope in Antarctica.

AboutAbout the lab
Building a telescope in Antarctica to observe the distant universe
The Observational Astronomy Lab studies the structure of the Milky Way, star-forming regions, external galaxies, supermassive black holes, and distant galaxies through telescope observations.
The lab aims to build a 10 m-class terahertz telescope in the interior of Antarctica, the best site on Earth for observation, to observe objects such as distant "dark galaxies" that cannot be seen in visible light.
The lab also uses the ALMA radio interferometer, the Nobeyama 45 m telescope, and the James Webb Space Telescope.
Key terms
- Terahertz waves
- A wavelength range for observing the universe, alongside submillimeter waves and infrared. In the interior of Antarctica, where there is little water vapor, they pass through the atmosphere more easily
- ALMA
- The world's largest radio interferometer, observing at millimeter to submillimeter wavelengths. Its 66 antennas are arranged over an area up to 10 km across
- Molecular gas
- The part of the gas filling a galaxy that is closely involved in star formation. The other part is atomic gas
NewsLab news
A master's student received the Physics Degree Program Leader Award
A master's student received the Meikeikai Award
An undergraduate student received the College of Physics English Award (Score Improvement category)
An undergraduate student received the Best Presentation Award for graduation research
ResearchResearch themes
The Observational Astronomy Lab observes the universe in radio waves, terahertz waves, and other wavelengths to study galaxies, star formation, and supermassive black holes. While advancing a plan to build a telescope in Antarctica, it also uses telescopes such as ALMA and the Nobeyama 45 m telescope.
*Illustrative imageAntarctic Terahertz Telescope Project
The interior of Antarctica has extremely little water vapor, making it the best site on Earth for submillimeter, terahertz, and infrared observations of the universe. Working with institutions such as the National Institute of Polar Research and the National Astronomical Observatory of Japan, the lab is advancing a plan to install a 10 m-class telescope there.
*Illustrative imageExploring galaxies and the distant universe with ALMA
Using ALMA, which observes at millimeter to submillimeter wavelengths, the lab observes mass accretion onto active galactic nuclei and the formation and evolution of galaxies in the distant universe.
*Illustrative imageObserving gas and star formation in galaxies
Because stars are born from gas, the lab observes molecular gas in spiral galaxies and other galaxies using telescopes such as the Nobeyama 45 m radio telescope. It studies the structure of galaxies, the motion of gas, and active galactic nuclei.
MembersFaculty
The members of the Observational Astronomy Lab are faculty members, visiting faculty members, postdoctoral researchers, doctoral, master's, and undergraduate students, research students, and administrative assistants.As of 2026
- ProfessorNario Kuno
- Assistant ProfessorTakuya Hashimoto
- Assistant Professor (Tenure Track)Shunsuke Honda
- Assistant Professor (Tenure Track)Yuri Nishimura
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Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “Eyes on the Skies (beletsky alma 15-cc2)” ESO/Y. Beletsky / CC BY 4.0 (cropped)
- Antarctic Terahertz Telescope Project: “The HEAT telescope (ann14031b)” Craig Kulesa / CC BY 4.0 (cropped)
- Exploring galaxies and the distant universe with ALMA: “ALMA Antennas on Chajnantor” Iztok Bončina/ESO / CC BY 4.0 (cropped)
- Observing gas and star formation in galaxies: “Hubble2005-01-barred-spiral-galaxy-NGC1300” NASA, ESA, and The Hubble Heritage Team STScI/AURA) / Public domain (cropped)
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