a unit of distance equal to that required to cause a heliocentric parallax of one second of an arc, equivalent to 206,265 times the distance from the earth to the sun, or 3.26 light-years.
par·sec (pär'sěk') n. A unit of astronomical length based on the distance from Earth at which stellar parallax is one second of arc and equal to 3.258 light-years, 3.086 × 1013 kilometers, or 1.918 × 1013 miles.
1913, from par(allax) sec(ond). It is the distance at which an object has parallax (viewed from Earth) of one second of arc, or about 3.26 light years.