The 65cm Refractor Telescope
About the 65cm refractor telescope.
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This telescope was constructed in April 1972, and is still the largest refractor telescope in the East Asia.
This telescope has two advantages that make it ideal for studying planets
and/or the nuclei of comets: 1. its long focal lenght, and 2.
the stable and clear observing conditions
at Hida observatory.
The telescope observes storms and clouds on Mars,
and seasonal variations in its atmosphere.
In 2001, the 15m dome was repaired. This telescope is also
used for the education of under graduate and graduate students.
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The view of the telescope inside the dome.
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One of the main objectives of this telescope is to investigate the
variation of the Martian atmosphere and clouds. The following
figures show Martian clouds taken with different filters. The
use of different filters enables us to study the
clouds in detail. (Top: with blue filters. Bottom: with red filters)
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Clouds of Mars on 5th March, 1997.
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The variation of the clouds from March through April, 1997.
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Instrument performance
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Apature | 650mm |
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Manufactured by | Carl Zeiss Co. Ltd. |
Focal length | 10,500mm |
F/ratio | 16 |
Resolution | 0".18 |
Light gathering power | 8,600 |
Limitting visual magnitude | 16.2 |
Tracking accuracy | 0.1"/9' |
Size of the housing | 930mm(diameter)x11,500mm |
Total weight | 17 ton |
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CCD camera | Spectrasource Instruments Co. Ltd. | HPC-1S |
| CCD chip | Kodak KAF1600-IUV |
| Chip size | 9 micro meter |
| Pixel number | 1522 x 1032 |
| Bit depth | 16 bits |
Controlling PC | Gateway 2000 | P5-133 |
Filters (For Mars) | Nihon Shinku Kogaku Co. Ltd. | |
| Blue filter | 436.2nm / 15.6nm |
| Yellow Filter | 588.3nm / 12.6nm |
| Red Filter | 647.2nm / 10.1nm |
| (Central wavelength / Band width) |
Filters (For Jupiter) | Nihon Shinku Kogaku Co. Ltd. | |
| Methane band | 890nm / 10nm |
| Continuum | 750nm / ---- |
Recent topics
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The "Hida Observatory Polarimetry System (HOPS)" is currently an on-going
project to install a "Two-dimensional polarization imager" on the
65cm telescope. The present objective of this project is to
investigate the polar hayes of
Jupiter.
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Recent work
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Martian north polar cap 1996-1997.
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K. Iwasaki, D. Parker, L. Larson, and T. Akabane.
Icarus 138, 20-24 (1999).
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Diurnal variation of Martian water-ice clouds in Tharsis
region of the low latitude cloud belt: Observations in 1995-1999.
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T.
Akabane, T. Nakakushi, K. Iwasaki, S. M. Larson.
A & A 384, 678-688 (2002).
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Mars: The cloud effect on the blue clearing in the Syrtis Major region.
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T. Nakakushi, T. Akabane, K. Iwasaki, S. M. Larson.
J. Geophys. Res. 106, 5043-5056 (2001).
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