RC 700 - 28" Astrograph
The PlaneWave RC700,a 0.7 meter Alt/Az telescope system with Ritchey-Chrétien (RC) optics. PlaneWave have combined Ritchey-Chrétien optics with PlaneWave's direct-drive alt/az mount technology to set a new standard for research-class observatory telescopes.
PlaneWave's CDK astrographs have become the telescopes of choice for universities, industry, and astrophotographers around the world. Now PlaneWave offers the PW-RC series to meet the custom needs of the scientific community. More about the optical design (Verlinkung).
The PW700-RC in its native format (no field flattening lenses) uses only mirror with reflective coatings. This can be useful when making observations primarily on-axis and wide field imaging is not a concern.
With high-resolution encoders providing the feedback for the direct drive motors, not only will the telescope track without periodic error or have any backlash at all, but the mount will be able to counter against wind gusts. The direct drive motors can move the telescope at incredible speeds for tracking satellites or just to minimize target acquisition time.
Fused Silicia is a synthetic amorphous silica glass of the highest purity and one of the most transparent glasses made. The optical and thermal properties of fused silica are superior to other types of glass due to its purity. Its transmission and homogeneity exceed those of crystalline quartz without the problems of temperature instability inherent in the crystalline form. Fused Silica has a coefficient of thermal expansion six times lower than Borosilicate (Pyrex) glass, which means that as fused silica cools down, it preserves its shape to a high degree of accuracy. This translates into consistent optical performance and unchanging focus over temperature changes. With its high melting temperature ()~ 1.600 degree Celsius), a very low coefficient of thermal expansion and resistance to thermal shock, fused silica is the material of choice for professional observatories as well as various scientific applications.
- Pinpoint stars out to a 70mm image circle
- Direct-drive motors on each axis for smooth, fast, and virtually silent movement of the telescope. Direct Drive motors mean that there are no gears to cause backlash and periodic error
- High resolution encoders on each axis for precise positioning
- Incorporates PointXP mount modeling software by Dave Rowe All ASCOM compatible.
- Dual Nasmyth focus, allowing simultaneous mounting of two instruments or easy switching between visual and imaging use
- integrated rotator for the tertiary mirror, with magnetic locks to position the mirror precisely for either Nasmyth focus position. The rotator can move from one port to the other in under 10 seconds.
- Field de-rotator / rotational field framing
Benefits of Nasmyth Focus: The Nasmyth Focus is along the altitude axis so there are virtually no balancing issue as you change out equipment. Eyepieces remain at a constant wheelchair-accessible height, greatly simplifying access to the telescope for public observatories. The rotating tertiary mirror allows you to switch from one Nasmyth port to the other in just seconds, allowing observers to easily transition between imaging and visual use
Aperture 27.56 inch (700 mm) Focal Length 4540 mm Focal ratio 6.5 Central Obstruction 47% of the Primary Mirror Diameter Back Focus from Mounting Surface 309 mm (12.2 inch) Weight 1,200 lbs(544 kg) OTA Tube Dual truss structure with Nasmyth focus Dimensions 93.73" H x 43.25" W x 39" D Focus Position Nasmyth Focus
Fork Assembly Single piece U shaped fork arm assembly for maximum stiffness Azimuth Bearing 20 inch diameter thrust bearing Altitude Bearing 2 x 8.5 inch OD ball bearings Optical Tube Dual truss structure with Nasmyth focus
Motor Control Industrial grade Parker brushless motor control system and built in electronics Azimuth Motor Direct Drive 3 Phase Axial-Flux Torque Motor Altitude Motor Direct Drive 3 Phase Axial-Flux Torque Motor Encoder - Azimuth and Altitude 10 inch disk built into the azimuth and altitude axes with stainless steel encoder tape on the circumference with reader yields 16 million counts per revolution of the telescope. This translates to about 0.08 arcsecond resolution. Motor Torque Approximately 35 ft-lbs Drive Electronics Capable of controlling up to 4 high speed encoders, limit switch inputs, homing switch inputs, controls two additional motors for accessories, two brake outputs and 16 digital and 2 analog inputs Telescope Control Software Incorporates PointXP mount modeling software by Dave Rowe All ASCOM compatible.
Pointing Accuracy 10 arcsecond RMS with PointXP Model Pointing Precision 2 arcsecond Tracking Accuracy 1 arcsecond error over 3 minute period System Natural Frequency 10 Hz or greater Field De-Rotator Accuracy 3 microns of peak to peak error at 35mm off-axis over 1 hour of tracking (18 arc sec)
tr>Edge Thickness2.25 inchtr>Cell18 point
Radius of Curvature 4115mm Optical Diameter 700 mm (27.56 inch) Outer Diameter 714.38 mm (28.125 inch) Core Diameter 203mm (8 inch) Material Fused Silica
Radius of Curvature 2961 mm Optical Diameter 312.4 mm (12.3 inch) Outer Diameter 317.5 mm (12.5 inch) Material Fused Silica Thickness 25 mm Cell 3 point RTV
Optical Major Diameter 152.4 mm Material Fused Silica Thickness 25 mm
|Manufacturer SKU (#)||700125Q|
|Optical Design||Ritchey-Chrétien (RC)|
|Aperture (mm)||27.56" (700 mm)|
|Focal Length||4.540 mm (175.74 inch)|
|Back Focus Distance||12.2" (309 mm) from Mounting Surface|
|Central Obstruction||47% of the Primary Mirror Diameter|
|Optical Tube Weight||1200 lbs (544 kg)|
|Mount||No mount (OTA only)|