Terminal Configuration and Performance Specifications
Optical section main technical parameters
One, Tube Lens
1. Primary Optical System: Apochromatic High-Resolution Refractive Optical System
Objective lens
Effective Bore Size:Φ310 mm
Effective Focal Length: 3000mm
Resolution: 0.38 arcseconds
Maximum Magnification: 2250x
Extinction Magnitude: 17th magnitude star
(2) Eyepieces: Five Sets (Advanced PL Eyepieces)
(3) Attachment:
Solar Light Filters: Used for visual and photographic observations of the sun.
Solar Projection System: Used for projecting and observing the sun, as well as depicting sunspots.
2. Apochromatic refractor telescope: high-resolution achromatic refractive optical system
Objective lens
Effective Bore Size:Φ100 Baomai
Equivalent Focal Length: 1200 meters
Resolution: 1.16 arcseconds
Maximum Magnification: 600x
(1) Eyepieces: (Five sets of eyepieces are compatible with the main scope eyepiece assembly)
Wide-Angle Eyepiece: f=40mm (equipped with crosshair reticle)
(2) Attachment:
Solar Light Filters: Used for visual and photographic observations of the sun.
3. Starfinder Telescope: Achromatic High-Resolution Refractive Optical System
Objective lens
Effective Bore Size:Φ80 mm
Effective Focal Length: 500mm
Resolution: 1.45 arcseconds
Maximum Magnification: 100x
(2) Eyepieces: (The eyepieces are interchangeable with the five eyepiece groups of the main scope)
Wide-angle eyepiece: f=40mm (equipped with crosshair reticle)
(3) Attachment:
Solar Light Filters: Used for visual and photographic observations of the sun.
Main Technical Parameters of Mechanical Parts
Rack
1. Rack: Equipped with an advanced German equatorial mount system, the base and equatorial mount can be disassembled separately for easy transportation and installation.
2. Equatorial Mount Dynamic Range:
Equatorial Axis: 0h-24h Declination Axis: ±90
The observed azimuth angle points to a scale with reading indicators.
Section 3: Electrical Control Drive System
The equatorial mount's right ascension and declination axes are controlled by a dual-motor dual-servo computer single board program.
(1) The driving speed in the right ascension direction during tracking observation is:
Tracking Speed (Constant Motion) = 15'/minute
(2) Both the right ascension axis and the declination axis are equipped with three-speed controls: rapid search, slow fine-tuning, and micro-motion fine-tuning.
Quick Search: ±(30°-60°)/minute
Slow Motion Fine Adjustment: ±(1°- 3°)/minute
Micro Adjustment: Soil (1)-3/min
To ensure the observer can quickly locate celestial targets and accurately track them.
IV. Automatic Tracking System:
Programmable control system designed based on the varying motion trajectories of celestial bodies, automatically drives the main optical path system (main tube), achieving automated tracking of celestial bodies.
V. Automatic Star Tracking System:
The Automatic Star Finder System is specifically designed for beginners to quickly locate celestial bodies. Its advantages include an operating system with human-machine dialogue, featuring a microcomputer installed in the automatic star-finding control box, controlled manually.
The Chinese star chart on the box, by clicking on a celestial body in the star chart, you can automatically find its coordinates. Follow this method to control the telescope, aiming it at the celestial body you wish to observe. Simple operations can capture the boundless starry sky.
