NAOJ Nobeyama Radio Observatory NOBEYAMA

Nobeyama
Radio Observatory

“Holy Place” of Japanese Radio Astronomy
Japanese radio astronomy that was born immediately after the war,
has remarkably developed into a global level in Nobeyama
with solar radio observations and cosmic radio observations
by 45-m radio telescope and so on.

Photo by Atsushi Hayashi

News

Latest Reserch Results

Apr. 18. 2024 Discovery of the origin of the streamer feeding the material of the young star Per-emb-2
Feb. 16. 2023 “Tadpole” Molecular Cloud Discovered near the Center of the Milky Way －Interacting with a Black Hole?－
May. 10. 2021 Star Formation Triggered by Cloud-Cloud Collisions
Apr. 16. 2021 Surprise Twist Suggests Stars Grow Competitively
Feb. 24. 2021 "Carbon Chain Factories" around massive young stellar objects ---Discovery of a new "Carbon Chain Chemistry" in hot-core regions
Aug. 25. 2020 Large Amount of Spinning-top-like Organic Molecules Found in Sagittarius
Aug. 04. 2020 Completion of a catalog of locations for near-future star birth in the Orion constellation---Discovery of Mysterious double-eye structure toward a baby star--
Jun. 11. 2020 New Method to Study Barred Spiral Galaxies
Mar. 23. 2020 Star Formation Project Maps Nearby Interstellar Clouds
Jan. 09. 2020 PASJ Special Issue "Nobeyama 45 m telescope: Legacy Projects and Receiver FOREST" was published

Telescopes of Nobeyama

Photo by Toshinari Hidaka

Photo by Atsushi Nakazawa

45-m telescope

The 45-m telescope is one of the world's largest radio telescopes that observes in the millimeter (1mm-10mm) wavelengths. Using its large 45-m diameter aperture,the 45-m telescope is capable of collecting extremely weak signal from distant terrestrial objects.

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Nobeyama Radio Polarimeters

Nobeyama Radio Polarimeters are observing the Sun with multiple frequencies in the microwave range. It is capable to obtain the total incoming flux and the circular-polarization degree.

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Photo by Hirokuni Tsuchiya

Nobeyama Millimeter Array

The Nobeyama Millimeter Array (NMA) is a telescope array that consists of six parabolic antennas. Its ability to produce high spatial resolution images is equivalent to a 600-m diameter parabola,and it has pictured details of numerous celestial objects.

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Photo by Atsushi Nakazawa

Nobeyama Radioheliograph (Nagoya University)

Nobeyama Radioheliograph is a radio telescope dedicated to observe the Sun. It consists of 84 parabolic antennas each with 80 cm diameter, sitting on lines of 490m long in the east/west and of 220m long in the north/south.

  • Detail

45-m Telescope

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