There are different ways to find the distance to the moon in an image in Matlab, but one way is to use the known size of the moon and its angular diameter.
First, you need to estimate the angular diameter of the moon in the image. You can use imtool
or imshow
to display the image and manually measure the diameter using a ruler tool. Alternatively, you can use image processing techniques to automatically detect the moon and estimate its diameter. For example, you can use the imfindcircles
function to detect a circle in the image that corresponds to the moon and estimate its radius.
Once you have the angular diameter of the moon, you can compute the distance to the moon using the formula:
distance = size / 2 * tan(alpha)
where size
is the known size of the moon (e.g., its average radius), and alpha
is the estimated angular diameter of the moon in radians.
Note that this formula assumes that the moon is at the zenith (i.e., directly overhead). If the moon is at an angle, you need to adjust the formula accordingly.
Here's an example code snippet that demonstrates how to estimate the distance to the moon in an image:
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Note that the focalLength
parameter needs to be calibrated for your specific camera and lens setup. You can measure it by taking a photo of an object with a known size and distance, and then computing the focal length from the resulting image. For example:
main.m532 chars17 lines
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