Telescope FOV Equation:
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The telescope field of view (FOV) is the angular size of the area visible through your telescope. It depends on both the eyepiece's apparent field of view and the magnification being used.
The calculator uses the telescope FOV equation:
Where:
Explanation: The true field of view narrows as magnification increases, following this simple inverse relationship.
Details: Knowing your telescope's FOV helps in locating celestial objects and understanding what will fit in your view. It's essential for planning observations and astrophotography.
Tips: Enter the eyepiece's apparent field of view (typically 50°-82° for most eyepieces) and your telescope's current magnification. Both values must be positive numbers.
Q1: What's a typical eyepiece FOV?
A: Standard Plössl eyepieces have about 50° FOV, while wide-angle designs can reach 82° or more.
Q2: How does magnification affect FOV?
A: Higher magnification results in a narrower field of view, making it harder to locate objects but providing more detail.
Q3: What's a good FOV for deep-sky observing?
A: For large deep-sky objects, a wider FOV (1° or more) is preferable. For planets, a narrower FOV is acceptable.
Q4: Can I calculate magnification from FOV?
A: Yes, you can rearrange the formula: Magnification = Eyepiece FOV / Telescope FOV.
Q5: Does telescope focal length affect FOV?
A: Indirectly, as focal length determines magnification with a given eyepiece: Magnification = Telescope FL / Eyepiece FL.