Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 6865
| Start | June 11, 2366 at 06:20 AM UTC |
|---|---|
| End | July 8, 2366 at 11:04 AM UTC |
| Length (days) | 27.20 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 6860 | January 25, 2366 at 08:07 PM UTC | February 22, 2366 at 04:18 AM UTC | 27.34 |
| 6861 | February 22, 2366 at 04:18 AM UTC | March 21, 2366 at 12:10 PM UTC | 27.33 |
| 6862 | March 21, 2366 at 12:10 PM UTC | April 17, 2366 at 07:14 PM UTC | 27.29 |
| 6863 | April 17, 2366 at 07:14 PM UTC | May 15, 2366 at 01:14 AM UTC | 27.25 |
| 6864 | May 15, 2366 at 01:14 AM UTC | June 11, 2366 at 06:20 AM UTC | 27.21 |
| 6865 | June 11, 2366 at 06:20 AM UTC | July 8, 2366 at 11:04 AM UTC | 27.20 |
| 6866 | July 8, 2366 at 11:04 AM UTC | August 4, 2366 at 04:01 PM UTC | 27.21 |
| 6867 | August 4, 2366 at 04:01 PM UTC | August 31, 2366 at 09:35 PM UTC | 27.23 |
| 6868 | August 31, 2366 at 09:35 PM UTC | September 28, 2366 at 03:50 AM UTC | 27.26 |
| 6869 | September 28, 2366 at 03:50 AM UTC | October 25, 2366 at 10:39 AM UTC | 27.28 |
| 6870 | October 25, 2366 at 10:39 AM UTC | November 21, 2366 at 05:52 PM UTC | 27.30 |
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.