Abstract: A method and apparatus is disclosed for aligning an optical instrument with respect to a celestial coordinate system, the optical instrument having a field of view and an optical instrument coordinate system, the celestial coordinate system having a plurality of objects each having celestial coordinates. The method includes the steps of receiving a plurality of captured optical instrument positions in the optical instrument coordinate system along with a plurality of associated capture times; calculating, for each associated capture time in the plurality of associated capture times, coordinates in the optical instrument coordinate system for the plurality of objects to create a plurality of calculated object positions for each associated capture time; and, determining, for each associated capture time, a match for each captured optical instrument position in the plurality of captured optical instrument positions with the plurality of calculated object positions to create a list of actual alignment objects.

Abstract: A tripod/telescope assembly including a tripod structure and optical tube-fork-base structure removably connected to one another by a conical central opening formed in an upper structure of the tripod and a complementary conical structure extending from a lower portion of the optical tube-fork-base. The tripod has three equally spaced legs pivotally extending downward from the upper structure of the tripod head. The tripod structure and optical tube-fork-base structure are disassembled and reassembled by a hand knob that has a central threaded fastening shaft extending through the complementary conical structures. The hand knob and complementary conical structures establish a stable, rotatable platform and allow the tube-fork-base structure of the telescope to be quickly separable from the tripod structure for transportation purposes.