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V. Partial lunar eclipse of 2012 November 28


The beginning of the eclipse is visible from Asia (except for south-western
part), Northern America, Greenland, Australia, New Zealand, Arctic and Pacific
oceans, eastern Indian ocean.
The end of the eclipse is visible from Eurasia, Alaska, Greenland, Austra-
lia, north-eastern part of Africa, Madagascar, Arctic and Indian oceans, west-
ern Pacific ocean.


Universal time of geocentric opposition
h m s
in right ascension 2012, November 28, 14 23 52.5


Sun Moon
h m s h m s
Right ascension . . . . . . . . . . . . . 16 19 41.886 4 19 41.894
s s
Hourly motion . . . . . . . . . . . . . +10.721 +126.017
˙ˆ ' " ˙ˆ ' "
Declination. . . . . . . . . . . . . . . . -21 26 11.20 +20 27 23.58
" "
Hourly motion . . . . . . . . . . . . . -25.60 +139.53
" ' "
Equatorial horizontal parallax . . . . . . 8.92 53 57.73
' " ' "
Apparent semidiameter . . . . . . . . . . 16 12.84 14 42.27



Circumstances of the Eclipse
Position Angles
of the Moon's axis
h m ˙ˆ
Moon enters penumbra . . . . . . . November 28, 12 12.6 348.34
Greatest eclipse . . . . . . . . . 14 33.0 348.80
Moon leaves penumbra . . . . . . . 16 53.5 349.25

--------------------------------------------
Contacts| Position |The Moon being in the Zenith in
of penumbra| Angles |----------------------
with Limb| from the | |
of Moon |North Point| Latitude | Longitude
---------|-----------|----------|-----------
| o ' | o ' | o '
First | 42 47.9 ˙– +20 29.6 ˙– 172 49.4 E
Last | 309 12.5 ˙– +20 40.5 ˙– 104 52.7 E

Magnitude of the eclipse 0.943
"
Angular radius of the penumbra 4303.63
"
Angular radius of the umbra 2319.53

--------------------------------------------------------------------------------
˙– ˙– ˙– ˙–Magnitudes of˙–˙– ˙– ˙– ˙– |Magnitudes of
T ˙– s ˙– d ˙– P ˙– penumbral ˙–˙– T ˙– s ˙– d ˙– P ˙– penumbral
˙– ˙– ˙– ˙– eclipse ˙–˙– ˙– ˙– ˙– ˙– eclipse
-----+-----+------+------+-------------++-----+-----+------+------+-------------
h m˙– "˙– ˙– ˙ˆ ˙– ˙–˙– h m˙– "˙– ˙– ˙ˆ ˙–
12 10˙– 5234˙– 2.256˙– 55.0˙– - ˙–˙–14 50˙– 3549˙– 1.530˙– 359.8˙– 0.928
20˙– 5037˙– 2.171˙– 52.9˙– 0.085 ˙–˙– ˙– ˙– ˙– ˙–
30˙– 4847˙– 2.089˙– 50.7˙– 0.193 ˙–˙–15 00˙– 3594˙– 1.549˙– 355.5˙– 0.902
40˙– 4664˙– 2.011˙– 48.2˙– 0.296 ˙–˙– 10˙– 3659˙– 1.577˙– 351.3˙– 0.865
50˙– 4491˙– 1.936˙– 45.6˙– 0.394 ˙–˙– 20˙– 3742˙– 1.613˙– 347.3˙– 0.818
˙– ˙– ˙– ˙– ˙–˙– 30˙– 3843˙– 1.657˙– 343.5˙– 0.761
13 00˙– 4328˙– 1.866˙– 42.8˙– 0.486 ˙–˙– 40˙– 3959˙– 1.707˙– 339.9˙– 0.695
10˙– 4176˙– 1.800˙– 39.8˙– 0.572 ˙–˙– 50˙– 4090˙– 1.763˙– 336.6˙– 0.621
20˙– 4037˙– 1.740˙– 36.6˙– 0.651 ˙–˙– ˙– ˙– ˙– ˙–
30˙– 3911˙– 1.686˙– 33.1˙– 0.722 ˙–˙–16 00˙– 4235˙– 1.826˙– 333.4˙– 0.539
40˙– 3801˙– 1.639˙– 29.4˙– 0.785 ˙–˙– 10˙– 4391˙– 1.893˙– 330.5˙– 0.450
50˙– 3707˙– 1.598˙– 25.5˙– 0.838 ˙–˙– 20˙– 4558˙– 1.965˙– 327.7˙– 0.356
˙– ˙– ˙– ˙– ˙–˙– 30˙– 4735˙– 2.041˙– 325.2˙– 0.256
14 00˙– 3631˙– 1.565˙– 21.5˙– 0.881 ˙–˙– 40˙– 4921˙– 2.121˙– 322.9˙– 0.151
10˙– 3574˙– 1.541˙– 17.3˙– 0.914 ˙–˙– 50˙– 5114˙– 2.204˙– 320.7˙– 0.041
20˙– 3537˙– 1.525˙– 12.9˙– 0.935 ˙–˙– ˙– ˙– ˙– ˙–
30˙– 3520˙– 1.518˙– 8.5˙– 0.944 ˙–˙–17 00˙– 5313˙– 2.290˙– 318.7˙– -
40˙– 3524˙– 1.519˙– 4.1˙– 0.942 ˙–˙– ˙– ˙– ˙– ˙–

T - universal time (TDT-UT1= 67.0s);
s - the angular distance between the centers of the Moon and the shadow;
d - the linear distance between the Moon's center and that of the shadow
in terms of the shadow's radius;
P - the position angle of the Moon's disk semi-diameter directed towards
the shadow's center.