Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 5951
| Start | March 9, 2298 at 06:07 PM UTC |
|---|---|
| End | April 6, 2298 at 01:31 AM UTC |
| Length (days) | 27.31 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 5946 | October 24, 2297 at 03:07 AM UTC | November 20, 2297 at 10:21 AM UTC | 27.30 |
| 5947 | November 20, 2297 at 10:21 AM UTC | December 17, 2297 at 05:56 PM UTC | 27.32 |
| 5948 | December 17, 2297 at 05:56 PM UTC | January 14, 2298 at 01:53 AM UTC | 27.33 |
| 5949 | January 14, 2298 at 01:53 AM UTC | February 10, 2298 at 10:04 AM UTC | 27.34 |
| 5950 | February 10, 2298 at 10:04 AM UTC | March 9, 2298 at 06:07 PM UTC | 27.34 |
| 5951 | March 9, 2298 at 06:07 PM UTC | April 6, 2298 at 01:31 AM UTC | 27.31 |
| 5952 | April 6, 2298 at 01:31 AM UTC | May 3, 2298 at 07:55 AM UTC | 27.27 |
| 5953 | May 3, 2298 at 07:55 AM UTC | May 30, 2298 at 01:18 PM UTC | 27.22 |
| 5954 | May 30, 2298 at 01:18 PM UTC | June 26, 2298 at 06:06 PM UTC | 27.20 |
| 5955 | June 26, 2298 at 06:06 PM UTC | July 23, 2298 at 10:54 PM UTC | 27.20 |
| 5956 | July 23, 2298 at 10:54 PM UTC | August 20, 2298 at 04:13 AM UTC | 27.22 |
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.