The application discloses a low-tolerance and high-sensitivity large-view-field main-focus astronomical optical
system, which comprises a main mirror, a correcting mirror A, a correcting mirror B, a correcting mirror C, a correcting mirror D, a correcting mirror E, a correcting mirror F and a focal plane; wherein light is reflected by the main mirror, and then sequentially passes through the correcting mirror A, the correcting mirror B, the correcting correcting mirror C, the correcting mirror D, the correcting mirror E and the correcting mirror F to reach the focal plane; the main mirror is a concave aspheric mirror, and the
surface shape is a quadratic
hyperboloid or a high-order aspheric surface. The application realizes low
machining and assembling tolerance sensitivity while ensuring excellent large-view-field imaging of the main-focus optical
system; through analyzing the distribution of aberration on each
optical surface, the position and structure parameters of special glass materials and the
optical power of optical elements are optimized, the average of the contribution of each
optical surface aberration is realized, and thus the
machining and assembling tolerance sensitivity is reduced.