September 1913 lunar eclipse

A total lunar eclipse took place on September 15, 1913. The moon passed through the center of the Earth's shadow.[1]

The moon passed through the center of the Earth's shadow

Visibility

Inex series

The inex series repeats eclipses 20 days short of 29 years, repeating on average every 10571.95 days. This period is equal to 358 lunations (synodic months) and 388.5 draconic months. Saros series increment by one on successive Inex events and repeat at alternate ascending and descending lunar nodes.

This period is 383.6734 anomalistic months (the period of the Moon's elliptical orbital precession). Despite the average 0.05 time-of-day shift between subsequent events, the variation of the Moon in its elliptical orbit at each event causes the actual eclipse time to vary significantly. It is a part of Lunar Inex series 40.

All events in this series shown (from 1000 to 2500 and beyond) are central total lunar eclipses.

Inex series from 1000–2500 AD
Descending node Ascending node Descending node Ascending node
Saros Date Saros Date Saros Date Saros Date
95 1016 May 24 96 1045 May 3 97 1074 Apr 14 98 1103 Mar 25
99 1132 Mar 3 100 1161 Feb 12 101 1190 Jan 23 102 1219 Jan 2
103 1247 Dec 13 104 1276 Nov 23 105 1305 Nov 2 106 1334 Oct 13
107 1363 Sep 23 108 1392 Sep 2 109 1421 Aug 13 110 1450 Jul 24
111 1479 Jul 4 112 1508 Jun 13
 113 1537 May 24 114 1566 May 4
115 1595 Apr 24 116 1624 Apr 3 117 1653 Mar 14 118 1682 Feb 21
119 1711 Feb 3 120 1740 Jan 13 121 1768 Dec 23 122 1797 Dec 4
123 1826 Nov 14 124 1855 Oct 25 125 1884 Oct 4 126 1913 Sep 15
127 1942 Aug 26
 128 1971 Aug 6
 129 2000 Jul 16
 130 2029 Jun 26
131 2058 Jun 6
 132 2087 May 17
 133 2116 Apr 27 134 2145 Apr 7
135 2174 Mar 18 136 2203 Feb 26 137 2232 Feb 7 138 2261 Jan 17
139 2289 Dec 27 140 2318 Dec 9 141 2347 Nov 19 142 2376 Oct 28
143 2405 Oct 8 144 2434 Sep 18 145 2463 Aug 29 146 2492 Aug 8

Saros series

Lunar Saros series 126, repeating every 18 years and 11 days, has a total of 70 lunar eclipse events including 14 total lunar eclipses. Solar Saros 133 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

First Penumbral Lunar Eclipse: 1228 Jul 18

First Partial Lunar Eclipse: 1625 Mar 24

First Total Lunar Eclipse: 1769 Jun 19

First Central Lunar Eclipse: 1805 Jul 11

Greatest Eclipse of the Lunar Saros 126: 1859 Aug 13, lasting 106 minutes.

Last Central Lunar Eclipse: 1931 Sep 26

Last Total Lunar Eclipse: 2003 Nov 09

Last Partial Lunar Eclipse: 2346 Jun 05

Last Penumbral Lunar Eclipse: 2472 Aug 19

1901-2100

1913 Sep 15

1931 Sep 26

1949 Oct 07

1967 Oct 18

1985 Oct 28

2003 Nov 09

2021 Nov 19

2039 Nov 30

2057 Dec 11

2075 Dec 22

2094 Jan 01

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[2] This lunar eclipse is related to two total solar eclipses of Solar Saros 133.

September 9, 1904 September 21, 1922
gollark: > If you make the temperature higher, then the frequency increases. No, you keep ignoring me on this.> Thus meaning the amount of photons emited is related/proportional to the temperature increasing.Also no, the amount is a different thing.
gollark: Also wrong, objects emit multiple frequencies at once and the relationship is more complex than that.
gollark: The energy is a property of the photon similarly to frequency and stuff, the energy doesn't have frequency either, but can I just say that trying to brute-force your way to coherent-sounding wording is not a path to great understanding.
gollark: Why does the energy have a wavelength now?
gollark: It isn't a wording problem.

See also

Notes
  1. Saros series 126
  2. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros


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