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TopicAllAryabhata Earth Diameter · 1Aryabhata Earth Rotation · 1Aryabhata Eclipse Geometry · 1Aryabhata Ecliptic Obliquity · 1Aryabhata Kalpa Billion Years · 1Aryabhata Moon Reflected Sunlight · 1Aryabhata Sidereal Day · 1Panchasiddhantika Graphical Computation · 1Panchasiddhantika Vedanga Yuga · 1Surya Siddhanta Armillary Sphere · 1Surya Siddhanta Earth Globe · 1Surya Siddhanta Eclipse Duration · 1Surya Siddhanta Gnomon Observatory · 1Surya Siddhanta Mars Period · 1Surya Siddhanta Moon Earth Ratio · 1Surya Siddhanta Moon Sidereal · 1Surya Siddhanta Precession · 1Surya Siddhanta Saturn Sidereal · 1Surya Siddhanta Sidereal Year · 1Varahamihira Romaka Siddhanta · 1Varahamihira Solstice Shift · 1

1 claim.

  • AstronomyT1

    Pañcasiddhāntikā III.21 (505 CE) states that the summer solstice once turned from the middle of Āśleṣā — "then the ayana was right" — but at present begins from Punarvasu: a shift of about 23°, roughly 1,700 years of equinoctial precession separating the old record from current observation. Hipparchus discovered precession c. 130 BCE; this verse documents the Indian tradition registering the same drift by checking its inherited solstice positions against the sky.

    The Panchasiddhantika: The Astronomical Work of Varaha Mihira · tr. G. Thibaut & Sudhakara Dvivedi, 1889

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