An astronomical telescope is an optical instrument used for observing celestial objects. It collects and focuses light, enabling us to observe celestial bodies that are far away from the Earth, such as stars, planets, galaxies, and nebulae.
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Features & Benefits
Objective: The objective is one of the most important components of a telescope, located at the front of the optical path. It is a large lens or mirror responsible for collecting and focusing light to form an image of celestial objects.
Eyepiece: The eyepiece is located at the rear of the optical path, close to the eye. It magnifies the image formed by the objective, allowing us to observe celestial objects with greater clarity and detail.
Focuser: The focuser enables us to adjust the telescope's focal length to obtain a clear image. By rotating the focuser, we can achieve sharp focus to accommodate different observation distances.
Magnification Adjuster: Some astronomical telescopes are equipped with a magnification adjuster, which allows us to change the magnification during observations. By adjusting the magnification, we can alter the size of the observed celestial objects.
Mount or Tripod: Telescopes are typically placed on a stable mount or tripod to maintain stability during observations. This helps reduce shaking and vibrations caused by hand movements, ensuring a steady view.
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Specification
How to Use
Rotate the left and right body of the laser ranging telescope, and at the same time, the left and right eyes observe the target through the left and right eyeglasses of the telescope until the left and right eyes observe a circular image.
Observe the distant target with the left and right eyes, and rotate the left and right eyeglasses until the target is the clearest.
If you wear glasses and use a laser range finder, you can unscrew the left and right eyepiece rubber goggles and observe.
