Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 726
| Start | January 1, 1908 at 12:40 PM UTC |
|---|---|
| End | January 28, 1908 at 08:49 PM UTC |
| Length (days) | 27.34 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 721 | August 18, 1907 at 01:24 AM UTC | September 14, 1907 at 07:30 AM UTC | 27.25 |
| 722 | September 14, 1907 at 07:30 AM UTC | October 11, 1907 at 02:11 PM UTC | 27.28 |
| 723 | October 11, 1907 at 02:11 PM UTC | November 7, 1907 at 09:19 PM UTC | 27.30 |
| 724 | November 7, 1907 at 09:19 PM UTC | December 5, 1907 at 04:48 AM UTC | 27.31 |
| 725 | December 5, 1907 at 04:48 AM UTC | January 1, 1908 at 12:40 PM UTC | 27.33 |
| 726 | January 1, 1908 at 12:40 PM UTC | January 28, 1908 at 08:49 PM UTC | 27.34 |
| 727 | January 28, 1908 at 08:49 PM UTC | February 25, 1908 at 04:56 AM UTC | 27.34 |
| 728 | February 25, 1908 at 04:56 AM UTC | March 23, 1908 at 12:34 PM UTC | 27.32 |
| 729 | March 23, 1908 at 12:34 PM UTC | April 19, 1908 at 07:15 PM UTC | 27.28 |
| 730 | April 19, 1908 at 07:15 PM UTC | May 17, 1908 at 12:53 AM UTC | 27.23 |
| 731 | May 17, 1908 at 12:53 AM UTC | June 13, 1908 at 05:47 AM UTC | 27.20 |
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.