Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 8010
| Start | December 12, 2451 at 06:15 AM UTC |
|---|---|
| End | January 8, 2452 at 02:06 PM UTC |
| Length (days) | 27.33 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 8005 | July 28, 2451 at 09:34 PM UTC | August 25, 2451 at 02:56 AM UTC | 27.22 |
| 8006 | August 25, 2451 at 02:56 AM UTC | September 21, 2451 at 09:00 AM UTC | 27.25 |
| 8007 | September 21, 2451 at 09:00 AM UTC | October 18, 2451 at 03:40 PM UTC | 27.28 |
| 8008 | October 18, 2451 at 03:40 PM UTC | November 14, 2451 at 10:46 PM UTC | 27.30 |
| 8009 | November 14, 2451 at 10:46 PM UTC | December 12, 2451 at 06:15 AM UTC | 27.31 |
| 8010 | December 12, 2451 at 06:15 AM UTC | January 8, 2452 at 02:06 PM UTC | 27.33 |
| 8011 | January 8, 2452 at 02:06 PM UTC | February 4, 2452 at 10:14 PM UTC | 27.34 |
| 8012 | February 4, 2452 at 10:14 PM UTC | March 3, 2452 at 06:22 AM UTC | 27.34 |
| 8013 | March 3, 2452 at 06:22 AM UTC | March 30, 2452 at 02:02 PM UTC | 27.32 |
| 8014 | March 30, 2452 at 02:02 PM UTC | April 26, 2452 at 08:45 PM UTC | 27.28 |
| 8015 | April 26, 2452 at 08:45 PM UTC | May 24, 2452 at 02:26 AM UTC | 27.24 |
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.