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

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
Dec. 12. 2019 Trial of "Radio Fingerprint Authentication" on galaxies ~ Molecular catalog on the three nearby galaxies was completed ! ~
Nov. 21. 2019 Eggs of stars sleeping in Cygnus region, the largest cradle in Milky Way.
Jul. 24. 2019 Production Sites of Stars are Rare
Jun. 05. 2019 Can we judge the efficiency of star formation by galaxy morphologies?
Mar. 08. 2019 Revealing the chemical composition and its evolution in high-mass star-forming regions
Feb. 28. 2019 Hiding Black Hole Found
- A stray black hole that swirls gas clouds -
Apr. 09. 2018 Evidence of Past Explosions at the Center of the Milky Way
-Is It Another Super Massive Star Cluster ?-
Jan. 25. 2018 FUGIN Project: Large-scale Exploration of the Invisible Milky Way
- Making the Most Detailed Radio Map of the Milky Way
Nov. 17. 2017 "Solar Minimum Surprisingly Constant"
More than Half a Century of Observation yields New Discovery
Feb. 02. 2017 Tail of Stray Black Hole hiding in the Milky Way
Jan. 15, 2016 Signs of Second Largest Black Hole in the Milky Way -Possible Missing Link in Black Hole Evolution
Feb. 26, 2015 ALMA Revealed Surprisingly Mild Environment around a Supermassive Black Hole
May. 19, 2014 Unveiling a Structure of a Protoplanetary Disk

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.

  • Detail

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.

  • Detail

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.

  • Detail

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

Web site