Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 942
| Start | February 18, 1924 at 02:09 AM UTC |
|---|---|
| End | March 16, 1924 at 09:57 AM UTC |
| Length (days) | 27.33 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 937 | October 4, 1923 at 11:42 AM UTC | October 31, 1923 at 06:43 PM UTC | 27.29 |
| 938 | October 31, 1923 at 06:43 PM UTC | November 28, 1923 at 02:07 AM UTC | 27.31 |
| 939 | November 28, 1923 at 02:07 AM UTC | December 25, 1923 at 09:53 AM UTC | 27.32 |
| 940 | December 25, 1923 at 09:53 AM UTC | January 21, 1924 at 05:59 PM UTC | 27.34 |
| 941 | January 21, 1924 at 05:59 PM UTC | February 18, 1924 at 02:09 AM UTC | 27.34 |
| 942 | February 18, 1924 at 02:09 AM UTC | March 16, 1924 at 09:57 AM UTC | 27.33 |
| 943 | March 16, 1924 at 09:57 AM UTC | April 12, 1924 at 04:55 PM UTC | 27.29 |
| 944 | April 12, 1924 at 04:55 PM UTC | May 9, 1924 at 10:49 PM UTC | 27.25 |
| 945 | May 9, 1924 at 10:49 PM UTC | June 6, 1924 at 03:52 AM UTC | 27.21 |
| 946 | June 6, 1924 at 03:52 AM UTC | July 3, 1924 at 08:35 AM UTC | 27.20 |
| 947 | July 3, 1924 at 08:35 AM UTC | July 30, 1924 at 01:35 PM UTC | 27.21 |
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.