A star transit is the passage of a star across the field of view of a telescope eyepiece.
The precise observation of star transits is the basis of many methods in astronomy and in geodesy. The measurements can be done in different ways:
- visually (mostly up to 1990): accuracy 0,1" to 2" (depending on the instrument); timing with digital clocks about 0,05–0,2 seconds;
- by CCD and other electro-optical sensors: as above, time often better;
- semi automatic instruments: photography or "impersonal micrometer", ca. 2 times better than No. 1;
- by scanning methods: astrometry satellites like Hipparcos about 0,01".
