Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 4558
| Start | February 28, 2194 at 08:13 AM UTC |
|---|---|
| End | March 27, 2194 at 03:51 PM UTC |
| Length (days) | 27.32 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 4553 | October 14, 2193 at 05:28 PM UTC | November 11, 2193 at 12:36 AM UTC | 27.30 |
| 4554 | November 11, 2193 at 12:36 AM UTC | December 8, 2193 at 08:05 AM UTC | 27.31 |
| 4555 | December 8, 2193 at 08:05 AM UTC | January 4, 2194 at 03:57 PM UTC | 27.33 |
| 4556 | January 4, 2194 at 03:57 PM UTC | February 1, 2194 at 12:06 AM UTC | 27.34 |
| 4557 | February 1, 2194 at 12:06 AM UTC | February 28, 2194 at 08:13 AM UTC | 27.34 |
| 4558 | February 28, 2194 at 08:13 AM UTC | March 27, 2194 at 03:51 PM UTC | 27.32 |
| 4559 | March 27, 2194 at 03:51 PM UTC | April 23, 2194 at 10:32 PM UTC | 27.28 |
| 4560 | April 23, 2194 at 10:32 PM UTC | May 21, 2194 at 04:10 AM UTC | 27.23 |
| 4561 | May 21, 2194 at 04:10 AM UTC | June 17, 2194 at 09:05 AM UTC | 27.20 |
| 4562 | June 17, 2194 at 09:05 AM UTC | July 14, 2194 at 01:49 PM UTC | 27.20 |
| 4563 | July 14, 2194 at 01:49 PM UTC | August 10, 2194 at 06:58 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.