TKS Ephemeris · Laboratory · sidereal frame

Ayanāṃśa comparison — one engine, several definitions

An ayanāṃśa is the offset between the tropical (sāyana) and sidereal (nirayana) zodiac. Every school fixes it differently, and the choice moves every sidereal longitude, nakṣatra and rāśi. This page quantifies the differences with our own engine only — the same ICRS → true-ecliptic-of-date chain (IAU-2006-style precession + nutation) and the Hipparcos position of Spicā (α Vir, Chitrā) with its real proper motion. Nothing here is imported from an almanac: tropical longitudes come from our chain, and each ayanāṃśa definition is applied to them.

The four things compared

1 · Zero-point years and modern values

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2 · The decisive test — Spicā’s nirayana longitude under each system

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Under true Chitrāpakṣa this is 180° by construction (that is what the definition says). Any fixed-offset system makes Spicā creep away from 180° with time — the numbers below are exactly that creep, in arc-seconds. A system that keeps a fixed ayanāṃśa-rate can never hold a star fixed for millennia.

3 · Curves and differences (arc-seconds)

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4 · Table (step-wise)

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Method, accuracy and limits

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