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Basics

UT1 (Universal Time 1)

ut1

Definition

UT1 (Universal Time 1) is a timescale derived from the observed rotation angle of the Earth. It is determined through Very Long Baseline Interferometry (VLBI) observations of distant quasars, which precisely measure the Earth's rotational orientation. Because UT1 directly reflects all irregular variations in the Earth's spin, including the effects of tidal friction, crustal movements, and atmospheric circulation, the length of a UT1 day is never exactly 86,400 SI seconds.

Relationship to UTC

UTC is a uniform timescale based on atomic clocks, whereas UT1 is a non-uniform timescale tied to the Earth's rotation. The difference between them (DUT1 = UT1 - UTC) is kept within 0.9 seconds by inserting leap seconds. The International Earth Rotation and Reference Systems Service (IERS) monitors DUT1 and announces upcoming leap seconds via Bulletin C. The 2022 resolution of the General Conference on Weights and Measures (CGPM) decided to widen this permitted difference by 2035, although the new limit and its implementation date were still undecided as of September 2026. Once the wider limit takes effect, leap second insertions will effectively stop and DUT1 will be allowed to gradually accumulate without correction.

Practical Use

UT1 is essential in astronomy (celestial position calculations), geodesy (determining Earth's orientation), and precision satellite orbit determination. For everyday life and IT systems, UTC is sufficient, but observatory software and precision satellite-tracking systems require the DUT1 correction. IERS publishes the current DUT1 value weekly in Bulletin A.

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