Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 8417
| Start | May 4, 2482 at 12:03 PM UTC |
|---|---|
| End | May 31, 2482 at 05:30 PM UTC |
| Length (days) | 27.23 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 8412 | December 18, 2481 at 09:58 PM UTC | January 15, 2482 at 05:54 AM UTC | 27.33 |
| 8413 | January 15, 2482 at 05:54 AM UTC | February 11, 2482 at 02:04 PM UTC | 27.34 |
| 8414 | February 11, 2482 at 02:04 PM UTC | March 10, 2482 at 10:08 PM UTC | 27.34 |
| 8415 | March 10, 2482 at 10:08 PM UTC | April 7, 2482 at 05:35 AM UTC | 27.31 |
| 8416 | April 7, 2482 at 05:35 AM UTC | May 4, 2482 at 12:03 PM UTC | 27.27 |
| 8417 | May 4, 2482 at 12:03 PM UTC | May 31, 2482 at 05:30 PM UTC | 27.23 |
| 8418 | May 31, 2482 at 05:30 PM UTC | June 27, 2482 at 10:19 PM UTC | 27.20 |
| 8419 | June 27, 2482 at 10:19 PM UTC | July 25, 2482 at 03:06 AM UTC | 27.20 |
| 8420 | July 25, 2482 at 03:06 AM UTC | August 21, 2482 at 08:22 AM UTC | 27.22 |
| 8421 | August 21, 2482 at 08:22 AM UTC | September 17, 2482 at 02:20 PM UTC | 27.25 |
| 8422 | September 17, 2482 at 02:20 PM UTC | October 14, 2482 at 08:56 PM UTC | 27.27 |
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.