Focal Length Formula:
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The focal length of a telescope is the distance (in millimeters) between the telescope's primary lens or mirror and the point where the light rays come together in focus. It determines the telescope's magnification capabilities and field of view.
The calculator uses the focal length formula:
Where:
Explanation: The focal length is simply the product of the aperture size and the f-ratio of the telescope.
Details: Focal length affects magnification (longer focal length = higher magnification) and field of view (shorter focal length = wider field). It's crucial for determining what eyepieces to use and what objects you can observe effectively.
Tips: Enter the aperture in millimeters (common sizes are 70mm, 100mm, 150mm, etc.) and the f-ratio (common values are f/5, f/10, etc.). Both values must be positive numbers.
Q1: What's a typical focal length for beginner telescopes?
A: Beginner telescopes often have focal lengths between 400mm and 1000mm, depending on their design and intended use.
Q2: How does focal length affect magnification?
A: Magnification is calculated as (telescope focal length) / (eyepiece focal length). Longer telescope focal lengths provide higher magnification with the same eyepiece.
Q3: What's better - short or long focal length?
A: It depends on what you want to observe. Short focal lengths are better for wide-field views (galaxies, nebulae), while long focal lengths are better for planetary observation.
Q4: Can I change my telescope's focal length?
A: The native focal length is fixed, but you can effectively change it using focal reducers (to decrease) or Barlow lenses (to increase).
Q5: How does focal length relate to f-ratio?
A: F-ratio is the focal length divided by the aperture. Fast telescopes (low f-ratio) are better for photography, while slow telescopes (high f-ratio) often provide better visual contrast.