LUNAR PENUMBRAL ECLIPSES NON TOTAL
Are listed all penumbral lunar eclipses non total, from the year 0 to 3000
Lunar eclipses with max magnitude
The longest total lunar eclipses
U.T.
Maximum Saros Pen. Umb. S.D. S.D.
Date Type # Gamma Mag. Mag. Par Tot
0012/05/24 02:38 P 79 -1.025 0.978 0.008 10m -
0153/04/26 00:30 P 82 1.014 0.999 0.027 18m -
0276/03/17 13:52 P 85 -1.021 0.992 0.009 10m -
0475/07/04 18:07 P 95 -1.019 0.994 0.013 13m -
0483/07/06 01:51 P 66 -1.014 0.994 0.032 20m -
0616/06/05 16:06 P 98 1.016 0.999 0.019 15m -
0624/06/06 23:49 P 69 1.028 0.966 0.006 8m -
0804/10/22 15:09 P 107 -1.023 0.989 0.002 4m -
0888/03/31 11:17 P 75 1.020 0.987 0.017 14m -
0899/08/24 17:05 P 81 1.022 0.986 0.011 11m -
0939/01/08 12:30 P 78 -1.020 0.996 0.008 10m -
1163/06/18 04:13 P 87 1.027 0.972 0.006 9m -
1427/04/11 15:32 P 93 1.015 0.998 0.023 17m -
1430/09/02 14:14 P 128 1.022 0.987 0.007 9m -
1470/01/17 09:48 P 125 -1.019 0.997 0.009 10m -
1553/07/25 03:22 P 131 -1.025 0.979 0.007 9m -
1958/05/03 12:13 P 140 1.019 0.992 0.015 13m -
2042/09/29 10:44 P 118 -1.026 0.978 0.003 6m -
2421/06/16 03:15 P 156 1.023 0.986 0.006 8m -
2429/06/17 10:53 P 127 1.019 0.985 0.023 17m -
2581/10/13 14:25 P 136 -1.025 0.982 0.002 4m -
2657/03/22 03:40 P 133 1.022 0.988 0.007 9m -
2678/08/24 12:01 P 168 1.031 0.963 0.001 3m -
2827/07/29 16:32 P 142 -1.019 0.988 0.019 15m -
Date Calendar Date (Gregorian) at instant of
Greatest Eclipse.
(Julian calendar is used before 1582 Oct 15).
Greatest Universal Time (UT) of Greatest Eclipse, which is
Eclipse defined as the instant when Moon passes closest
to the axis of Earth's shadows.
Type Type of lunar eclipse where:
N = Penumbral Eclipse.
P = Partial (Umbral) Eclipse.
T = Total (Umbral) Eclipse.
(Tc = central total eclipse)
If the Type ends with:
"m" = Middle eclipse of Saros series.
"+" = Central eclipse (Moon north of axis).
"-" = Central eclipse (Moon south of axis).
"b" = Saros series begins (first eclipse in series).
"e" = Saros series ends (last eclipse in series).
Saros Saros series of eclipse.
(Each eclipse in a Saros is separated by an interval
of 18 years 11.3 days.)
Gamma Distance of the Moon from the axis of Earth's
shadow cone (units of equatorial radii) at the
instant of greatest eclipse.
Pen. Penumbral eclipse magnitude is the fraction of
Mag. the Moon's diameter obscured by the penumbra.
Umb. Umbral eclipse magnitude is the fraction of
Mag. the Moon's diameter obscured by the umbra.
S.D. Semi-duration of partial (umbral) eclipse (minutes).
Par
S.D. Semi-duration of total (umbral) eclipse (minutes).
Tot
Dati fonte Nasa (C)