TMT

E297491

TMT is a planned next-generation ground-based optical and infrared observatory featuring a 30-meter primary mirror for extremely high-resolution astronomical observations.

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TMT canonical 2

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Statements (52)

Predicate Object
instanceOf astronomical observatory
ground-based optical telescope
infrared telescope
abbreviationFor Thirty Meter Telescope
alternativeProposedSite Roque de los Muchachos Observatory, La Palma, Canary Islands, Spain
apertureClass extremely large telescope
comparedTo European Extremely Large Telescope
Giant Magellan Telescope
fullName Thirty Meter Telescope
governingOrganization TMT International Observatory LLC
hasInstrument Infrared Imaging Spectrograph
Infrared Imaging Spectrograph (IRIS)
Infrared Multi-Slit Spectrometer
Infrared Multi-Slit Spectrometer (IRMS)
Mid-Infrared Camera and High-disperser Spectrograph
Mid-Infrared Camera and High-disperser Spectrograph (MICHI)
Planet Formation Instrument
Planet Formation Instrument (PFI)
Wide Field Optical Spectrometer
Wide Field Optical Spectrometer (WFOS)
hasTechnology active optics
adaptive optics
laser guide star system
mirrorType segmented primary mirror
numberOfPrimaryMirrorSegments 492
partner California Institute of Technology
Canada
China
India
Japan
United States
University of California
plannedLocation Mauna Kea, Hawaii, United States
linked to: Mauna Kea
primaryMirrorDiameter 30 meters
scienceCaseIncludes direct imaging of exoplanets
precision cosmology measurements
probing conditions near supermassive black holes
spectroscopy of faint high-redshift galaxies
scienceGoals extremely high angular resolution imaging
high-resolution spectroscopy
study of black holes
study of dark matter and dark energy
study of exoplanets
study of galaxy formation and evolution
study of stellar populations
study of the early universe
status planned
telescopeDesign Ritchey–Chrétien
telescopeType reflecting telescope
wavelengthRange mid-infrared
near-infrared
optical

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