Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 3410
| Start | June 7, 2108 at 08:04 AM UTC |
|---|---|
| End | July 4, 2108 at 12:48 PM UTC |
| Length (days) | 27.20 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 3405 | January 22, 2108 at 09:59 PM UTC | February 19, 2108 at 06:10 AM UTC | 27.34 |
| 3406 | February 19, 2108 at 06:10 AM UTC | March 17, 2108 at 02:00 PM UTC | 27.33 |
| 3407 | March 17, 2108 at 02:00 PM UTC | April 13, 2108 at 09:01 PM UTC | 27.29 |
| 3408 | April 13, 2108 at 09:01 PM UTC | May 11, 2108 at 02:59 AM UTC | 27.25 |
| 3409 | May 11, 2108 at 02:59 AM UTC | June 7, 2108 at 08:04 AM UTC | 27.21 |
| 3410 | June 7, 2108 at 08:04 AM UTC | July 4, 2108 at 12:48 PM UTC | 27.20 |
| 3411 | July 4, 2108 at 12:48 PM UTC | July 31, 2108 at 05:45 PM UTC | 27.21 |
| 3412 | July 31, 2108 at 05:45 PM UTC | August 27, 2108 at 11:21 PM UTC | 27.23 |
| 3413 | August 27, 2108 at 11:21 PM UTC | September 24, 2108 at 05:38 AM UTC | 27.26 |
| 3414 | September 24, 2108 at 05:38 AM UTC | October 21, 2108 at 12:27 PM UTC | 27.28 |
| 3415 | October 21, 2108 at 12:27 PM UTC | November 17, 2108 at 07:41 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.