Saros Series of Solar Eclipses

Solar Eclipses in Saros Series -6

This page lists all the solar eclipses in saros series -6 which are in our database. Note that the beginning of this series is not included in our database, so the list below only covers the latter part of the series.

This series is partnered with lunar Saros series -13.

3 Aug, 1994 BC max: 08:43 UT Partial Solar Eclipse (umbral mag. 0.43; Saros -6)	A small partial eclipse barely darkened the Sun. With just 43% of the Sun covered for viewers closest to the center, this was of limited interest.
13 Aug, 1976 BC max: 16:04 UT Partial Solar Eclipse (umbral mag. 0.35; Saros -6)	A small partial eclipse barely darkened the Sun. With just 35% of the Sun covered for viewers closest to the center, this was of limited interest.
24 Aug, 1958 BC max: 23:35 UT Partial Solar Eclipse (umbral mag. 0.29; Saros -6)	A small partial eclipse barely darkened the Sun. With just 29% of the Sun covered for viewers closest to the center, this was of limited interest.
4 Sep, 1940 BC max: 07:17 UT Partial Solar Eclipse (umbral mag. 0.24; Saros -6)	A small partial eclipse barely darkened the Sun. With just 24% of the Sun covered for viewers closest to the center, this was of limited interest.
15 Sep, 1922 BC max: 15:10 UT Partial Solar Eclipse (umbral mag. 0.20; Saros -6)	A small partial eclipse barely darkened the Sun. With just 20% of the Sun covered for viewers closest to the center, this was of limited interest.
25 Sep, 1904 BC max: 23:12 UT Partial Solar Eclipse (umbral mag. 0.18; Saros -6)	With only 18% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
7 Oct, 1886 BC max: 07:22 UT Partial Solar Eclipse (umbral mag. 0.16; Saros -6)	With only 16% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
17 Oct, 1868 BC max: 15:40 UT Partial Solar Eclipse (umbral mag. 0.16; Saros -6)	With only 16% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
29 Oct, 1850 BC max: 00:04 UT Partial Solar Eclipse (umbral mag. 0.16; Saros -6)	With only 16% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
8 Nov, 1832 BC max: 08:31 UT Partial Solar Eclipse (umbral mag. 0.16; Saros -6)	With only 16% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
19 Nov, 1814 BC max: 17:01 UT Partial Solar Eclipse (umbral mag. 0.17; Saros -6)	With only 17% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
30 Nov, 1796 BC max: 01:31 UT Partial Solar Eclipse (umbral mag. 0.17; Saros -6)	With only 17% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
11 Dec, 1778 BC max: 10:00 UT Partial Solar Eclipse (umbral mag. 0.17; Saros -6)	With only 17% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
21 Dec, 1760 BC max: 18:25 UT Partial Solar Eclipse (umbral mag. 0.17; Saros -6)	With only 17% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
2 Jan, 1741 BC max: 02:46 UT Partial Solar Eclipse (umbral mag. 0.16; Saros -6)	With only 16% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
12 Jan, 1723 BC max: 11:01 UT Partial Solar Eclipse (umbral mag. 0.13; Saros -6)	With only 13% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
23 Jan, 1705 BC max: 19:10 UT Partial Solar Eclipse (umbral mag. 0.10; Saros -6)	With only 10% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.
3 Feb, 1687 BC max: 03:10 UT Partial Solar Eclipse (umbral mag. 0.05; Saros -6)	With only 5% of the Sun covered at maximum eclipse, this was a very marginal eclipse at best, and rather uninteresting.