6m telescope
The 6-m telescope (BTA - Big Telescope Alt-azimuthal)
has the status of a national instrument. SAO
ensures the telescope being operative and carries out continuous
work to provide BTA with modern techniques of astrophysical data
accumulation and processing. The telescope is located near
Mt. Pastukhova at an altitude of 2070 m above sea level, the
coordinates of the site:
longitude 41o26'30",
latitude +43o 39'12".
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Main mirror diameter |
6 m |
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Focal length |
24 m |
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Light collecting area |
26 sq.m |
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Wavelength range |
0.3 - 10 mkm |
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Angular resolution |
0.6 arcsec |
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- with the application of speckle |
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interferometry techniques |
0.02 arcsec |
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Mass of the main mirror |
42 tons |
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Total telescope mass |
850 tons |
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Telescope height |
42 m |
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Dome height |
53 m |
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Limiting stellar magnitude (1994) |
26 |
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Optical scheme of the telescope
The main mirror (MM) is parabolic in shape and has a focal length
of 24 meters. The diameter of the main mirror is 605 cm, the
diameter of the cilindrical prime focus cage, where optical
devices and the mechanisms of input/output of the lens corrector
and hyperbolic secondary focus mirror are located, is 2 m. From
the laboratory tests the concentration of energy in a circle 0.8"
in diameter is 90%. The image diameter is
determined first of all by the microclimat in the dome and by thermal
conditions of the mirror. Under favorable conditions (temperature
difference between the MM, air inside the dome and outside of it)
the seeing is limited by atmosphere turbulence and amounts to
FWHM ~1" for 20% of observational nights.
The optical scheme of the telescope provides for working at the
prime focus (f/4) and two Nasmith foci (f/30). To correct for
field aberrations, when working at the prime focus, a Rosse
corrector is used, which is made of K type glass (the short-wave
bandwidth is 3800
).
The field of view with coma and astigmatism
corrected at a level of <0.5" is about 14'. The
time to switch on the beam from one focus to the other is 3-4
minutes, which makes it possible to conduct different observing
programs during a night.
Any questions to
webmaster
Last update: 26/12/2008
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