![]() Where one fails to solve a given image, another might succeed. The reason for this is that while most plate solving software is quite good, none are infallible. will prompt if the Blind Solver should be used to solve the image. There clicking on the play button a new image will be captured and solved based on the given parameters. To manual trigger plate solve of an image you need to use the Plate Solving tool in the image panel. This includes the focal length of the telescope itself and any focal length-affecting devices such as reducers, telecompressors, or barlows. will usually be able to detect the sensor's pixel size, but the user will need to inform the software of the effective focal length of the optical path. The two important settings are the camera's sensor pixel size and the focal length of the telescope. Plate solving requires that your camera and telescope settings are correct. ![]()
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