Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 2746
| Start | November 5, 2058 at 09:39 AM UTC |
|---|---|
| End | December 2, 2058 at 05:06 PM UTC |
| Length (days) | 27.31 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 2741 | June 22, 2058 at 03:51 AM UTC | July 19, 2058 at 08:40 AM UTC | 27.20 |
| 2742 | July 19, 2058 at 08:40 AM UTC | August 15, 2058 at 01:58 PM UTC | 27.22 |
| 2743 | August 15, 2058 at 01:58 PM UTC | September 11, 2058 at 07:58 PM UTC | 27.25 |
| 2744 | September 11, 2058 at 07:58 PM UTC | October 9, 2058 at 02:35 AM UTC | 27.28 |
| 2745 | October 9, 2058 at 02:35 AM UTC | November 5, 2058 at 09:39 AM UTC | 27.29 |
| 2746 | November 5, 2058 at 09:39 AM UTC | December 2, 2058 at 05:06 PM UTC | 27.31 |
| 2747 | December 2, 2058 at 05:06 PM UTC | December 30, 2058 at 12:55 AM UTC | 27.33 |
| 2748 | December 30, 2058 at 12:55 AM UTC | January 26, 2059 at 09:02 AM UTC | 27.34 |
| 2749 | January 26, 2059 at 09:02 AM UTC | February 22, 2059 at 05:12 PM UTC | 27.34 |
| 2750 | February 22, 2059 at 05:12 PM UTC | March 22, 2059 at 12:55 AM UTC | 27.32 |
| 2751 | March 22, 2059 at 12:55 AM UTC | April 18, 2059 at 07:44 AM UTC | 27.28 |
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.