Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 6354
| Start | April 13, 2328 at 05:00 PM UTC |
|---|---|
| End | May 10, 2328 at 11:08 PM UTC |
| Length (days) | 27.26 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 6349 | November 29, 2327 at 01:59 AM UTC | December 26, 2327 at 09:40 AM UTC | 27.32 |
| 6350 | December 26, 2327 at 09:40 AM UTC | January 22, 2328 at 05:42 PM UTC | 27.33 |
| 6351 | January 22, 2328 at 05:42 PM UTC | February 19, 2328 at 01:54 AM UTC | 27.34 |
| 6352 | February 19, 2328 at 01:54 AM UTC | March 17, 2328 at 09:50 AM UTC | 27.33 |
| 6353 | March 17, 2328 at 09:50 AM UTC | April 13, 2328 at 05:00 PM UTC | 27.30 |
| 6354 | April 13, 2328 at 05:00 PM UTC | May 10, 2328 at 11:08 PM UTC | 27.26 |
| 6355 | May 10, 2328 at 11:08 PM UTC | June 7, 2328 at 04:19 AM UTC | 27.22 |
| 6356 | June 7, 2328 at 04:19 AM UTC | July 4, 2328 at 09:04 AM UTC | 27.20 |
| 6357 | July 4, 2328 at 09:04 AM UTC | July 31, 2328 at 01:57 PM UTC | 27.20 |
| 6358 | July 31, 2328 at 01:57 PM UTC | August 27, 2328 at 07:26 PM UTC | 27.23 |
| 6359 | August 27, 2328 at 07:26 PM UTC | September 24, 2328 at 01:37 AM UTC | 27.26 |
About this tool
A Carrington rotation is the time the Sun takes to turn once on its axis as seen from the Earth: 27.2753 days on average. The count was defined by the English astronomer Richard Carrington, who studied sunspots in the 1850s; rotation 1 began on 9 November 1853, and the numbering has run without interruption since.
Explorer computes the start of each rotation with the formula given by Jean Meeus in Astronomical Algorithms (chapter 29), implemented in its own astronomy library and checked against published dates. A rotation begins when the Carrington longitude L₀ of the central meridian passes through 0°; because the Earth moves along its orbit, the synodic period varies slightly around the mean, hence lengths of 27.2 to 27.3 days.
Observers use the rotation number as a calendar for the Sun: an active region that crosses the disc reappears about one rotation later, and the community activity heatmap shows one row per rotation so that returning regions line up. Enter a date to find its rotation, or a number to get the UTC start and end dates and the neighbouring rotations.