parsec
UK[ˈpɑːsɛk]US[ˈpɑːrsɛk]
n
A unit of astronomical distance equal to about 3.26 light years, based on the distance from Earth at which a star would have a parallax of one second of arc.
Morpheme Breakdown
par
sec
par
partial
sec
second
Etymology
The word 'parsec' is a modern scientific portmanteau, coined in 1913 by combining the first syllable of 'parallax' with the first syllable of 'second'. Its logic is entirely descriptive and literal, defining the unit by the method of its measurement: the distance corresponding to a PARallax of one SECond of arc. This construction bypasses ancient roots, directly fusing two established scientific terms from Greek ('parallaxis' meaning alteration) and Latin ('secundus') to create a precise, calculable standard for interstellar distances. It represents a 20th-century method of word formation, where technical clarity takes precedence over etymological evolution from a single classical language.
Analysis
Structure: par (partial) + sec (second)
- par: A clipping of 'parallax', from Greek 'parallaxis' (alternation, change), indicating a shift in apparent position. In this word, it functions as the core concept.
- sec: A clipping of 'second' (of arc), from Latin 'secundus' (following, next). In this word, it specifies the precise angular measurement.
Examples
The nearest star to the Sun, Proxima Centauri, is approximately 1.3 parsecs away.
Astronomers often measure galactic distances in units of kiloparsecs.
The concept of a parsec is fundamental to the field of astrometry.