The 2000 Array
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This is the STU (Scope Transport
Unit) with arrays Left: 16" f/4.5 (obsolete); Right: 10" f/6
The 2000 array consists of two reflectors; a 10" and a belly-slung 4-1/2". The HPS Unit (High-Power Scan) is a 10" f/6, a 69-inch-long Newtonian. It has a 57.8" f/l. The mount used is a custom-made altazimuth yoke on a three-wheeled trailer. The pan & tilt head was constructed from the old 16" scope tube. The Scope Transport Unit or STU is a actually a mobile support with three 14" pneumatic tires and the scope/DOB Driver II mount. The STU has a 30" turret with a 10-gauge steel yoke that forms the scope mount. The upper turret rotates over the lower plate and provides the azimuth control. A drive wheel on the yoke is the elevation control. The DOB Driver II is a computerized remote control system. Another item needed to operate the STU are a site monitor, which can select any of the images from the three cameras.
The protective cover allows
set-up in 30-minutes
The Umbilical Harness which is a 50' long, 8-cable spool that is reeled out each session. It contains RG-59U coax cables to and from all cameras, a 110 VAC power cord and multiple plug-in receptacle, and a modular line from the DOB Driver II pendant control.
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Left: Cast aluminum
NOVAK 9-point flotation mirror mounting cell as used on The Lunascan
Project's 10" f/6 Newtonian. Shown here are a 16" in the foreground
with the 10" on the right. Right: 10" f/6 Cassegrain mirror in the
Novack cell.
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2.1" secondary diagonal mirror,
holder, and spider.
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The FinderCam
The Finder Cam is used to help locate and track the Moon, using the DOB Driver II computer located in the Control Room, and is a Panasonic WV-450 vidicon camera with a wide-angle TV lens, attached to a quickmount bracket for fast deployment and rapid takedown.
The Lunascan Project's
New MPS Unit Configuration
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The 4.5" f/8 mirror. The MPS Unit's CCD camera
is mounted in the eyepiece holder in the upper left.
The MPS Unit is a 900-mm, 4-1/2", f/8, Newtonian-reflector.
The Medium Power Scanning system is used to scan & videotape
a larger section of the Moon, but at lower power than the HPS unit. The
6" tube is 37" long. Will resolve to 1.5 arc-secs.
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The CCD-camera & T-C Adaptor
configuration.
The end on the right is placed vertically
in the focusser and has a 26-mm eyepiece inside for high-power scanning
of the Moon at 320 power, without Barlow.
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Lower part of east wall
unit in Control Room
The east wall unit in the Control Room houses
the six monitors and the datarecorder used there, plus stores equipment
not in use that can't be stored with the STU. Also stored in the Control
Room is main scope when not in use.
The Main Monitor is a 19" color
television.
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