Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 158
| Start | August 1, 1865 at 03:03 AM UTC |
|---|---|
| End | August 28, 1865 at 08:46 AM UTC |
| Length (days) | 27.24 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 153 | March 17, 1865 at 11:39 PM UTC | April 14, 1865 at 06:30 AM UTC | 27.29 |
| 154 | April 14, 1865 at 06:30 AM UTC | May 11, 1865 at 12:18 PM UTC | 27.24 |
| 155 | May 11, 1865 at 12:18 PM UTC | June 7, 1865 at 05:17 PM UTC | 27.21 |
| 156 | June 7, 1865 at 05:17 PM UTC | July 4, 1865 at 10:00 PM UTC | 27.20 |
| 157 | July 4, 1865 at 10:00 PM UTC | August 1, 1865 at 03:03 AM UTC | 27.21 |
| 158 | August 1, 1865 at 03:03 AM UTC | August 28, 1865 at 08:46 AM UTC | 27.24 |
| 159 | August 28, 1865 at 08:46 AM UTC | September 24, 1865 at 03:09 PM UTC | 27.27 |
| 160 | September 24, 1865 at 03:09 PM UTC | October 21, 1865 at 10:03 PM UTC | 27.29 |
| 161 | October 21, 1865 at 10:03 PM UTC | November 18, 1865 at 05:20 AM UTC | 27.30 |
| 162 | November 18, 1865 at 05:20 AM UTC | December 15, 1865 at 01:00 PM UTC | 27.32 |
| 163 | December 15, 1865 at 01:00 PM UTC | January 11, 1866 at 09:01 PM UTC | 27.33 |
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.