Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 596
| Start | April 16, 1898 at 10:08 PM UTC |
|---|---|
| End | May 14, 1898 at 03:51 AM UTC |
| Length (days) | 27.24 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 591 | December 1, 1897 at 07:34 AM UTC | December 28, 1897 at 03:24 PM UTC | 27.33 |
| 592 | December 28, 1897 at 03:24 PM UTC | January 24, 1898 at 11:32 PM UTC | 27.34 |
| 593 | January 24, 1898 at 11:32 PM UTC | February 21, 1898 at 07:41 AM UTC | 27.34 |
| 594 | February 21, 1898 at 07:41 AM UTC | March 20, 1898 at 03:22 PM UTC | 27.32 |
| 595 | March 20, 1898 at 03:22 PM UTC | April 16, 1898 at 10:08 PM UTC | 27.28 |
| 596 | April 16, 1898 at 10:08 PM UTC | May 14, 1898 at 03:51 AM UTC | 27.24 |
| 597 | May 14, 1898 at 03:51 AM UTC | June 10, 1898 at 08:47 AM UTC | 27.21 |
| 598 | June 10, 1898 at 08:47 AM UTC | July 7, 1898 at 01:32 PM UTC | 27.20 |
| 599 | July 7, 1898 at 01:32 PM UTC | August 3, 1898 at 06:37 PM UTC | 27.21 |
| 600 | August 3, 1898 at 06:37 PM UTC | August 31, 1898 at 12:23 AM UTC | 27.24 |
| 601 | August 31, 1898 at 12:23 AM UTC | September 27, 1898 at 06:48 AM UTC | 27.27 |
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.