Reflective telescope with wide field of view
Systems and methods for providing a wider FOV for a telescope system are disclosed. In one embodiment, a telescope includes a primary mirror having an orifice, where an optical path originates from an object positioned in front of the primary mirror and reflects off the primary mirror. A secondary mirror is disposed adjacent to the primary mirror, where the optical path reflects off the secondary mirror and passes through the orifice in the primary mirror. The telescope includes a set of extended field corrector optics disposed along the optical path, the extended field corrector optics positioned to reflect light incident from the secondary mirror, where the set of extended field corrector optics includes two corrector mirrors. A tertiary mirror is disposed along the optical path and adjacent to the extended field corrector optics, the tertiary mirror positioned to reflect the light incident from the extended field corrector optics.
1. A telescope comprising:
a primary mirror having an orifice, wherein light propagating along an optical path originates from an object positioned in front of the primary mirror and reflects off the primary mirror;
a secondary mirror disposed adjacent to the primary mirror, wherein the light propagating along the optical path reflects off the secondary mirror and passes through the orifice in the primary mirror;
a set of extended field corrector optics disposed along the optical path, the set of extended field corrector optics positioned to reflect light incident from the secondary mirror, wherein the set of extended field corrector optics comprises two corrector mirrors; and
a tertiary mirror disposed along the optical path and adjacent to the set of extended field corrector optics, wherein the tertiary mirror is positioned to:
receive light incident on the tertiary mirror from the set of extended field corrector optics, wherein the light incident on the tertiary mirror is propagating from the set of extended field corrector optics toward the primary mirror; and
reflect the light incident from the set of extended field corrector optics.
2. The telescope of claim 1 wherein the tertiary mirror is positioned adjacent to the primary mirror.
3. The telescope of claim 1 further comprising a fold mirror disposed along the optical path and adjacent to the set of extended field corrector optics, the fold mirror positioned to reflect light incident from the tertiary mirror.
4. The telescope of claim 1 wherein the tertiary mirror has an optical power suitable to collimate the light received from the set of extended field corrector optics.
5. The telescope of claim 1 wherein the set of extended field corrector optics are optically centered.
6. The telescope of claim 1 wherein a fold mirror and the tertiary mirror are on opposite sides of the set of extended field corrector optics.
7. The telescope of claim 1 wherein the primary mirror has a center, and the orifice is offset from the center.
8. The telescope of claim 1 wherein the set of extended field corrector optics has substantially no net paraxial optical power.
9. The telescope of claim 1 wherein the set of extended field corrector optics comprise a convex mirror and a concave mirror.
10. The telescope of claim 9 wherein each of three sets of light rays comprises individual light rays that intersect at a crossover plane substantially equidistant between the convex mirror and the concave mirror.
11. The telescope of claim 10 wherein the convex mirror and the concave mirror are disposed on opposite sides of an intermediate image.
12. The telescope of claim 11 wherein the intermediate image is an accessible intermediate image.
13. The telescope of claim 12 wherein the intermediate image is disposed equal distances away from the convex mirror and the concave mirror.
14. The telescope of claim 9 wherein the two corrector mirrors are both aspheric.
15. The telescope of claim 9 wherein the convex mirror is more aspheric than the concave mirror.