Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 8790
| Start | March 13, 2510 at 03:16 AM UTC |
|---|---|
| End | April 9, 2510 at 10:41 AM UTC |
| Length (days) | 27.31 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 8785 | October 27, 2509 at 12:17 PM UTC | November 23, 2509 at 07:30 PM UTC | 27.30 |
| 8786 | November 23, 2509 at 07:30 PM UTC | December 21, 2509 at 03:05 AM UTC | 27.32 |
| 8787 | December 21, 2509 at 03:05 AM UTC | January 17, 2510 at 11:02 AM UTC | 27.33 |
| 8788 | January 17, 2510 at 11:02 AM UTC | February 13, 2510 at 07:13 PM UTC | 27.34 |
| 8789 | February 13, 2510 at 07:13 PM UTC | March 13, 2510 at 03:16 AM UTC | 27.34 |
| 8790 | March 13, 2510 at 03:16 AM UTC | April 9, 2510 at 10:41 AM UTC | 27.31 |
| 8791 | April 9, 2510 at 10:41 AM UTC | May 6, 2510 at 05:07 PM UTC | 27.27 |
| 8792 | May 6, 2510 at 05:07 PM UTC | June 2, 2510 at 10:32 PM UTC | 27.23 |
| 8793 | June 2, 2510 at 10:32 PM UTC | June 30, 2510 at 03:20 AM UTC | 27.20 |
| 8794 | June 30, 2510 at 03:20 AM UTC | July 27, 2510 at 08:08 AM UTC | 27.20 |
| 8795 | July 27, 2510 at 08:08 AM UTC | August 23, 2510 at 01:25 PM UTC | 27.22 |
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.