Variable Earth's Rotation Speed in the 14th to 16th Centuries: New {\Delta}T Constraints from Chinese Eclipse Records
Hisashi Hayakawa, Mitsuru S\^oma, Naiqi Li

TL;DR
This study refines historical Earth's rotation speed variability during the 14th to 16th centuries by analyzing Chinese eclipse records, providing new constraints on { extDelta}T and improving previous models.
Contribution
It introduces new { extDelta}T constraints from Chinese records during the Ming Dynasty, revises existing data, and enhances understanding of Earth's rotational changes in that period.
Findings
Revised { extDelta}T constraints for 1361, 1514, 1542, and 1575.
Most existing { extDelta}T constraints in the 14th-16th centuries were updated.
Results indicate a steeper decrease in { extDelta}T between 1514 and 1567.
Abstract
Total solar eclipses are not only astronomical spectacles but also great astrophysical laboratories. Their historical records are particularly helpful for assessing the past variability of the Earth's rotation speed. Chinese records played a key role for such analyses. However, Chinese eclipse records from the M\'ing period have not been used for {\Delta}T reconstructions, partially because most of the contemporaneous eclipse reports are found not in official histories but in local treatises. This study examines eclipse records in the (quasi-)contemporaneous local treatises, concentrating on what explicitly mentioned eclipse totality on the day of a total solar eclipse and what were compiled during the M\'ing Dynasty. On their basis, our study revised the {\Delta}T constraint in 1361 to -408 s =< {\Delta}T =< 601 s and set new {\Delta}T constraints of 277 s =< {\Delta}T =< 890 s in…
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