astrophotometry
|as-tro-pho-tom-e-try|
🇺🇸
/ˌæstroʊfoʊˈtɑmətri/
🇬🇧
/ˌæstrəʊfəˈtɒmɪtri/
measure brightness of celestial objects
Etymology
'astrophotometry' originates from modern English, formed from the Greek-derived prefix 'astro-' (from Greek 'astron' meaning 'star'), 'photo-' (from Greek 'phōs/phot-' meaning 'light'), and the suffix '-metry' (from Greek 'metron' meaning 'measure').
'astrophotometry' developed as a compound by adding the prefix 'astro-' to 'photometry' (the latter coming via New/Modern Latin and Greek roots for 'light' and 'measure') during the late 19th to 20th century, as photographic and electronic techniques in astronomy became established; the combined term entered English usage in the 20th century.
Initially the root elements referred broadly to 'measurement of light'; over time the compounded term came to mean specifically the measurement of the brightness of celestial objects.
Meanings by Part of Speech
Noun 1
the measurement of the brightness (intensity) of astronomical objects (stars, galaxies, nebulae, etc.), typically using photographic or electronic detectors and photometric techniques.
Astrophotometry is used to determine the light curves of variable stars and to measure the brightness of distant galaxies.
Synonyms
Last updated: 2025/11/08 19:20
