'Thirty Meter Telescope'| Organizations | Caltech, the University of California, and ACURA |
|---|
| Logo | |
|---|
| Wavelength regime | Infrared, Visible light (0.31-28 µm) |
|---|
| Location | Still to be determined; sites considered are in Mexico, Chile, and Hawaii. |
|---|
| Completion | 2014 |
|---|
| Webpage | http://www.tmt.org/ |
|---|
| Physical Characteristics |
|---|
| Telescope Style | Ritchey-Chrétien |
|---|---|
| Diameter | 30 m |
|---|
| Collecting Area | ~650 m2 |
|---|
| Focal Length | 450 m |
|---|
| Primary Mirror | Consists of 492 hexagonal segments each about ~1.4 m in diameter |
|---|
The 'Thirty meter telescope (TMT)' (formerly called the 'California Extremely Large Telescope (CELT)') is a future large
segmented-mirror optical and
infrared extremely large telescope, proposed and run by a consortium made up by
Caltech, the
University of California, and
ACURA. Completion is scheduled for November 2014.
The 'TMT' is an
extremely large telescope design first proposed in the 1990s by a consortium of Californian Universities under the name ''California Extremely Large Telescope'', but this name was changed when additional institutions from outside California joined the project. The design is for a segmented 30m diameter astronomical telescope.
The optical design for the TMT is a
Ritchey-Chretien two mirror system. This rather naturally provides a large, 20 arc minute
field of view (15 arc minute unvignetted) with under 0.5
arcsecond images (100% enclosed energy). This focus is free of coma and only suffers from
astigmatism, which
grows quadratically with field angle. The primary will be 30 m in diameter, and for compactness, the primary
f-ratio will be f/1.5. The final focus will be f/15, delivering a final focus with about 2 mm/ arc second as its plate scale. Such a giant telescope produces very large seeing-limited images, a challenge for the design of seeing-limited scientific instruments. The 20
arcminute field is 2.6 m in diameter.
The telescope will have a simplified design in order to minimize the cost. Thus there will be no prime focus, nor a
Cassegrain focus. All scientific work is expected to be done at the bent Cassegrain and Nasmyth foci.
See also
★
List of optical telescopes
★
Giant Magellan Telescope
★
Overwhelmingly Large Telescope
External links
★
Project web site
★
Caltech web site
★
Old CELT website
★
New Lick Observatory TMT site