Subaru Telescope
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Features of the Subaru Telescope

The Subaru Telescope itself

Regular maintenance of the primary mirror

To maintain the mirror's reflective performance, the aluminum coating (the reflective layer) is reapplied every few years.

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The Subaru Telescope itself
  • The primary mirror has an aperture of 8.2m.
  • Surface precision of 0.014µm
  • Active-optics technology using 261actuators
  • Regular cleaning of the primary mirror
  • Four foci
  • Main unit 22.2m in height and weighing 555t
Instruments of the Subaru Telescope
  • 43m-high cylindrical dome
  • Seven instruments
  • Vapor deposition of the primary mirror
  • A highly efficient system for switching observational instruments
The environment surrounding the Subaru Telescope
  • 6,500km from Japan
  • Low population density of about 19 people per square kilometer
  • Latitude N 19° 49’ 43”
  • Elevation of 4,207m
  • Clear weather on the peak of Mauna Kea over 80% of the year
  • Razor-sharp astronomical imaging available nowhere else on Earth

Regular maintenance of the primary mirror

■ The primary mirror with its aluminum coating removed

The various equipment required to repeat vapor deposition of aluminum on the primary mirror is housed under the dome.

■ Electroplated primary mirror

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Subaru Telescope National Astronomical Observatory of JapanSubaru Telescope National Astronomical Observatory of Japan
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© 1999 National Astronomical Observatory of Japan
This project is supported by "Project to Promote Large Scientific Frontiers" of MEXT.

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