Don't Look Up! We got you!
Sunday, November 8, 2026 · UTC
Missions & Science

World's timekeepers vote to end the leap second from May 2027

Atomic time and Earth-rotation time may now drift up to an hour apart; the same meeting began work on a common time scale for the Moon.

Asteroid & Near-Earth Object Reporter
Share on X
Stands on 15 placed sources from 3 publishers.
Timekeepers vote to end leap second, allowing Earth time to drift from atomic time.
Timekeepers vote to end leap second, allowing Earth time to drift from atomic time. AI illustrationhow this picture was made
VERSAILLES, France, Oct. 15, 2026 - The world's timekeepers voted on 15 October to end the leap second.[1] Under Resolution 5, adopted at the 28th General Conference on Weights and Measures (CGPM) in Versailles,[2] Coordinated Universal Time (UTC) will run on without leap-second jumps[3] from 20 May 2027.[4] Since 1972, leap seconds have kept atomic UTC in step with UT1, the time set by Earth's rotation,[5] and 27 were added between 1972 and 2016.[6] From now on the two may drift up to one hour apart before any correction.[7] Scientists expect such a "leap hour" will not be needed for more than 1,000 years,[8] and timeanddate.com reports that no correction should be needed for several thousand years.[9] The change comes as Earth's rotation has sped up in recent years.[10] Under the old rules there was a 30% chance that the first-ever negative leap second would be needed within 10 years,[11] and removing a second could disrupt digital infrastructure.[12] The conference also looked beyond Earth. Resolution 6 addresses an international time scale for the Moon[13] and encourages space agencies to share their lunar timekeeping experience.[14] Resolution 4 lays the groundwork for a new definition of the second, to be adopted in 2030.[15] Impact Insight. Atomic clocks count the steady vibrations of atoms, while Earth's spin speeds up and slows down with tides, winds and shifts deep inside the planet, so the two kinds of time slowly drift apart. Precise time matters for planetary defense: predicting where an asteroid will be, and pointing radars and telescopes at it, depends on knowing both atomic time and Earth's exact orientation, so astronomers will keep tracking Earth's rotation closely even after civil clocks stop jumping.
Proof15 sources · 3 publishers · signed
What this stands on
  1. CGPM approved ending leap seconds on 2026-10-15. · timeanddate.com
  2. The 28th CGPM meeting was held 15 October 2026 in Versailles, France. · bipm.org
  3. Resolution 5 eliminates leap second discontinuities for UTC continuity. · bipm.org
  4. Continuous UTC will take effect on 20 May 2027 per Resolution 5. · bipm.org
  5. Leap seconds kept UTC and UT1 in sync since 1972. · timeanddate.com
  6. 27 leap seconds were added between 1972 and 2016. · timeanddate.com
  7. Resolution 5 sets a one hour maximum limit for UTC and UT1 difference. · bipm.org
  8. A leap hour will not be needed for over 1000 years. · yahoo.com
  9. No leap seconds will be needed for several thousand years. · timeanddate.com
  10. Earth's rotation speed has increased in recent years. · timeanddate.com
  11. There was 30% chance of negative leap second in 10 years under old rules. · timeanddate.com
  12. A negative leap second could disrupt digital infrastructure. · yahoo.com
  13. Resolution 6 addresses creation of an international lunar reference time scale. · bipm.org
  14. Resolution 6 encourages space agencies to share lunar timekeeping experience. · bipm.org
  15. Resolution 4 lays groundwork for a new second definition for 2030 CGPM adoption. · bipm.org
We could not place any of them by their address. None is an official body: that part stands on reporting, not on the underlying document or transcript.