Documents / Official release
This is a preliminary transcript of the Gemini 7 technical debriefing, dated December 23, 1965, from the National Aeronautics and Space Administration. It was made from tape recordings of the crew debriefing held December 19 to 21, 1965 at the Crew Quarters, Cape Kennedy, Florida. In it, Frank Borman and Jim Lovell go through countdown, powered flight, insertion, station keeping with the booster, systems, experiments and training. The table of contents also lists a section on visual sightings during orbital flight.
From the source:Release of 2026-06-12 Incident: December 19-21, 1965, Cape Kennedy, Florida. This document is a preliminary transcript derived from voice recordings of the Gemini 7 flight crew debriefing conducted December 19-21, 1965, at the Crew Quarters, Cape Kennedy, Florida. Lights and flashes are mentioned and there is discussion about having proper illumination for vehicle docking. Borman and Lovell discuss celestial and terrestrial observational anomalies and note sightings of Mercury, meteors, aurora, and lightning. They also discuss not being able to see any stars once the Sun comes up.
“Coast to Coast AM”2 pages
149 was fine , the stop watch was an excellent idea. The lighting on the sextant angle reading was too bright . It was a whi te bri ght light. Everytime you read the sextant out you lost your dark adaptation because we were looking at this whi te light. And al l it had to be,since the spacecraft is dark anyway if you are l ooking a t stars, is red, or dimmer l i ght to read the angle out . The r eticle was f i n e during the f irst pa.rt of the flight, and then f or some reason it became a double i mage . I found out that I never used the reticle during the full M.oo.n or eve.n at hal f Moon I could see the dark lines without having to light up the retic l e. One of t he big things about the sextant, the mechanical aspects , was t he fact that the l ight was not spli t 50- 50 between the upper prism and the lower telescope. It was a 20-80 split and therefore one image woul d be bright and the other one dim. This was fine if you went from the start of the horizon where you would have a bright star a.nd a dim hori zon. You had a contro l , but if you went from, say, two stars to measure the angle between two stars to check the al i gn ment of a sextant, (because the angl es are already known) one star woul d be bright and the other star rea l dim if you got them within a certain angl e of each other. But as soon as you got that other dim star, then the bright
Official release, from the pursue collection. The PDF is mirrored here; the original link is above. 222 pages are in the text index: search them above, or from the library's search.