Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 3187
| Start | October 11, 2091 at 06:16 PM UTC |
|---|---|
| End | November 8, 2091 at 01:22 AM UTC |
| Length (days) | 27.30 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 3182 | May 28, 2091 at 02:35 PM UTC | June 24, 2091 at 07:22 PM UTC | 27.20 |
| 3183 | June 24, 2091 at 07:22 PM UTC | July 22, 2091 at 12:12 AM UTC | 27.20 |
| 3184 | July 22, 2091 at 12:12 AM UTC | August 18, 2091 at 05:33 AM UTC | 27.22 |
| 3185 | August 18, 2091 at 05:33 AM UTC | September 14, 2091 at 11:36 AM UTC | 27.25 |
| 3186 | September 14, 2091 at 11:36 AM UTC | October 11, 2091 at 06:16 PM UTC | 27.28 |
| 3187 | October 11, 2091 at 06:16 PM UTC | November 8, 2091 at 01:22 AM UTC | 27.30 |
| 3188 | November 8, 2091 at 01:22 AM UTC | December 5, 2091 at 08:50 AM UTC | 27.31 |
| 3189 | December 5, 2091 at 08:50 AM UTC | January 1, 2092 at 04:41 PM UTC | 27.33 |
| 3190 | January 1, 2092 at 04:41 PM UTC | January 29, 2092 at 12:49 AM UTC | 27.34 |
| 3191 | January 29, 2092 at 12:49 AM UTC | February 25, 2092 at 08:57 AM UTC | 27.34 |
| 3192 | February 25, 2092 at 08:57 AM UTC | March 23, 2092 at 04:37 PM UTC | 27.32 |
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.