Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 376
| Start | November 11, 1881 at 02:43 AM UTC |
|---|---|
| End | December 8, 1881 at 10:16 AM UTC |
| Length (days) | 27.31 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 371 | June 27, 1881 at 08:05 PM UTC | July 25, 1881 at 01:00 AM UTC | 27.20 |
| 372 | July 25, 1881 at 01:00 AM UTC | August 21, 1881 at 06:31 AM UTC | 27.23 |
| 373 | August 21, 1881 at 06:31 AM UTC | September 17, 1881 at 12:44 PM UTC | 27.26 |
| 374 | September 17, 1881 at 12:44 PM UTC | October 14, 1881 at 07:31 PM UTC | 27.28 |
| 375 | October 14, 1881 at 07:31 PM UTC | November 11, 1881 at 02:43 AM UTC | 27.30 |
| 376 | November 11, 1881 at 02:43 AM UTC | December 8, 1881 at 10:16 AM UTC | 27.31 |
| 377 | December 8, 1881 at 10:16 AM UTC | January 4, 1882 at 06:12 PM UTC | 27.33 |
| 378 | January 4, 1882 at 06:12 PM UTC | February 1, 1882 at 02:22 AM UTC | 27.34 |
| 379 | February 1, 1882 at 02:22 AM UTC | February 28, 1882 at 10:27 AM UTC | 27.34 |
| 380 | February 28, 1882 at 10:27 AM UTC | March 27, 1882 at 05:55 PM UTC | 27.31 |
| 381 | March 27, 1882 at 05:55 PM UTC | April 24, 1882 at 12:24 AM 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.