Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 1562
| Start | June 6, 1970 at 04:55 PM UTC |
|---|---|
| End | July 3, 1970 at 09:38 PM UTC |
| Length (days) | 27.20 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 1557 | January 21, 1970 at 06:59 AM UTC | February 17, 1970 at 03:09 PM UTC | 27.34 |
| 1558 | February 17, 1970 at 03:09 PM UTC | March 16, 1970 at 10:58 PM UTC | 27.33 |
| 1559 | March 16, 1970 at 10:58 PM UTC | April 13, 1970 at 05:57 AM UTC | 27.29 |
| 1560 | April 13, 1970 at 05:57 AM UTC | May 10, 1970 at 11:52 AM UTC | 27.25 |
| 1561 | May 10, 1970 at 11:52 AM UTC | June 6, 1970 at 04:55 PM UTC | 27.21 |
| 1562 | June 6, 1970 at 04:55 PM UTC | July 3, 1970 at 09:38 PM UTC | 27.20 |
| 1563 | July 3, 1970 at 09:38 PM UTC | July 31, 1970 at 02:38 AM UTC | 27.21 |
| 1564 | July 31, 1970 at 02:38 AM UTC | August 27, 1970 at 08:15 AM UTC | 27.23 |
| 1565 | August 27, 1970 at 08:15 AM UTC | September 23, 1970 at 02:33 PM UTC | 27.26 |
| 1566 | September 23, 1970 at 02:33 PM UTC | October 20, 1970 at 09:24 PM UTC | 27.29 |
| 1567 | October 20, 1970 at 09:24 PM UTC | November 17, 1970 at 04:39 AM UTC | 27.30 |
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.