Extreme values of the equation of time through the centuries

The Equation of Time is the difference between the time determined by a sundial and the clock time. It is due to the obliquity of the Earth's axis and the unequal motion of the Earth (ellipse). The value, computed for 12:00 UT, is between -14 :20 min (near Feb 12) and +16:24 min (near Nov 4).


The length of the current solar day (i.e. the time interval between culmination of the Sun on prev. and curent day) is not exactly 24 hours; the difference is given in brackets (e.g. +18.8 s).

 

Equation of time and length of solar day:
(for 2001)

equation of time
length of solar day
Jan 1
- 03:45 min
24 h - 28.3 s
15
- 09:34 min
24 h - 21.2 s
Feb 1
- 13:38 min
24 h - 08.1 s
15
- 14:07 min
24 h + 02.8 s
Mar 1
- 12:18 min
24 h + 11.6 s
15
- 08:51 min
24 h + 16.8 s
Apr 1
- 03:48 min
24 h + 17.9 s
15
+ 00:02 min
24 h + 14.6 s
May 1
+ 02:57 min
24 h + 07.3 s
15
+ 03:40 min
24 h - 00.6 s
Jun 1
+ 02:09 min
24 h - 09.1 s
15
- 00:31 min
24 h - 12.8 s
Jul 1
- 03:53 min
24 h - 11.6 s
15
- 05:59 min
24 h - 06.2 s
Aug 1
- 06:18 min
24 h + 03.6 s
15
- 04:24 min
24 h + 11.7 s
Sep 1
+ 00:06 min
24 h + 18.9 s
15
+ 04:55 min
24 h + 21.4 s
Oct 1
+ 10:26 min
24 h + 19.4 s
15
+ 14:17 min
24 h + 13.4 s
Nov 1
+ 16:24 min
24 h + 01.7 s
15
+ 15:20 min
24 h - 10.0 s
Dec 1
+ 10:50 min
24 h - 22.3 s
15
+ 04:41 min
24 h - 28.8 s

Equation of Time

Length of Solar Day

 

Web Links

Equation of Time (Royal Greenwich Observatory Information Leaflet)

Sundials on the Internet - the Equation of Time

Equation of Time -- Problem in Astronomy (M. Müller)