Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 1425
| Start | March 14, 1960 at 01:45 AM UTC |
|---|---|
| End | April 10, 1960 at 08:49 AM UTC |
| Length (days) | 27.29 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 1420 | October 29, 1959 at 10:33 AM UTC | November 25, 1959 at 05:54 PM UTC | 27.31 |
| 1421 | November 25, 1959 at 05:54 PM UTC | December 23, 1959 at 01:38 AM UTC | 27.32 |
| 1422 | December 23, 1959 at 01:38 AM UTC | January 19, 1960 at 09:42 AM UTC | 27.34 |
| 1423 | January 19, 1960 at 09:42 AM UTC | February 15, 1960 at 05:53 PM UTC | 27.34 |
| 1424 | February 15, 1960 at 05:53 PM UTC | March 14, 1960 at 01:45 AM UTC | 27.33 |
| 1425 | March 14, 1960 at 01:45 AM UTC | April 10, 1960 at 08:49 AM UTC | 27.29 |
| 1426 | April 10, 1960 at 08:49 AM UTC | May 7, 1960 at 02:49 PM UTC | 27.25 |
| 1427 | May 7, 1960 at 02:49 PM UTC | June 3, 1960 at 07:55 PM UTC | 27.21 |
| 1428 | June 3, 1960 at 07:55 PM UTC | July 1, 1960 at 12:39 AM UTC | 27.20 |
| 1429 | July 1, 1960 at 12:39 AM UTC | July 28, 1960 at 05:36 AM UTC | 27.21 |
| 1430 | July 28, 1960 at 05:36 AM UTC | August 24, 1960 at 11:09 AM UTC | 27.23 |
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.