Carrington rotations
Convert a date to its Carrington rotation number and back, and browse rotation start and end times.
CR 7180
| Start | December 18, 2389 at 07:57 PM UTC |
|---|---|
| End | January 15, 2390 at 03:53 AM UTC |
| Length (days) | 27.33 |
Neighbouring rotations
| CR | Start | End | Length (days) |
|---|---|---|---|
| 7175 | August 4, 2389 at 10:32 AM UTC | August 31, 2389 at 04:06 PM UTC | 27.23 |
| 7176 | August 31, 2389 at 04:06 PM UTC | September 27, 2389 at 10:21 PM UTC | 27.26 |
| 7177 | September 27, 2389 at 10:21 PM UTC | October 25, 2389 at 05:09 AM UTC | 27.28 |
| 7178 | October 25, 2389 at 05:09 AM UTC | November 21, 2389 at 12:22 PM UTC | 27.30 |
| 7179 | November 21, 2389 at 12:22 PM UTC | December 18, 2389 at 07:57 PM UTC | 27.32 |
| 7180 | December 18, 2389 at 07:57 PM UTC | January 15, 2390 at 03:53 AM UTC | 27.33 |
| 7181 | January 15, 2390 at 03:53 AM UTC | February 11, 2390 at 12:04 PM UTC | 27.34 |
| 7182 | February 11, 2390 at 12:04 PM UTC | March 10, 2390 at 08:08 PM UTC | 27.34 |
| 7183 | March 10, 2390 at 08:08 PM UTC | April 7, 2390 at 03:33 AM UTC | 27.31 |
| 7184 | April 7, 2390 at 03:33 AM UTC | May 4, 2390 at 09:59 AM UTC | 27.27 |
| 7185 | May 4, 2390 at 09:59 AM UTC | May 31, 2390 at 03:24 PM UTC | 27.23 |
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.