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Ďîčńęîâűĺ ńëîâŕ: íëó

Penumbral Lunar Eclipse of 2002 November 20


The beginning of the eclipse visible in Europe, Asia except the eastern
part, Africa, Madagaskar, South America except the extreme south, Central Ame-
rica, North America except the western coast, Greenland, the western Indian
Ocean, the Arctic Ocean, and the Atlantic Ocean.
The end of the eclipse visible in Europe, Africa except the south-eastern
part, South and North America, Greenland, the Arctic Ocean, the Atlantic Oce-
an, and the eastern Pacific Ocean.


Universal time of geocentric opposition
h m s
in right ascension 2002, á­áŽďżďŽď°ďź 20, 1 02 08.3

Sun Moon
h m s h m s
Right ascension . . . . . . . . . . . . . 15 41 00.052 3 41 00.052
s s
Hourly motion . . . . . . . . . . . . . +10.431 +121.750
˙š ' " ˙š ' "
Declination . . . . . . . . . . . . . . . -19 36 27.94 +18 32 13.04
" "
Hourly motion . . . . . . . . . . . . . -34.30 +571.99
" ' "
Equatorial horizontal parallax . . . . . . 8.90 54 40.29
' " ' "
Apparent semidiameter . . . . . . . . . . 16 11.16 14 53.87



Circumstances of the Eclipse
Position Angles
of the Moon's axis
h m ˙š
Moon enters penumbra . . . . . . . . November 19, 23 32.2 348.15
Greatest eclipse . . . . . . . . . November 20, 1 46.6 348.54
Moon leaves penumbra . . . . . . . . 4 01.3 348.94

ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”
Contacts ˙– Position ˙–The Moon being in the Zenith in
of Penumbra˙– Angles ď“ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”
with Limb ˙– from the ˙– ˙–
of Moon ˙– North Point ˙– Latitude ˙– Longitude
ď”ď”ď”ď”ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”
˙– ˙š ' ˙– ˙š ' ˙– ˙š '
First ˙– 26 44.7 ˙– +18 24.7 ˙– 2 37.5 E
Last ˙– 295 53.5 ˙– +19 07.5 ˙– 62 33.7 W


Magnitude of the eclipse 0.884
"
Angular radius of the penumbra 4345.94
"
Angular radius of the umbra 2365.04

ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď˘ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”
˙– ˙– ˙– ˙– Magnitudes ˙” ˙– ˙– ˙– ˙– Magnitudes
T ˙– s ˙– d ˙– P ˙–of penumbral ˙” T ˙– s ˙– d ˙– P ˙–of penumbral
˙– ˙– ˙– ˙– eclipse ˙” ˙– ˙– ˙– ˙– eclipse
ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď§ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď”ď•ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”
h m˙– "˙– ˙– ˙š ˙– ˙” h m˙– "˙– ˙– ˙š ˙–
23 30˙– 5274˙– 2.231˙– 27.2˙– ď” ˙” 2 00˙– 3670˙– 1.551˙– 335.5˙– 0.874
40˙– 5076˙– 2.148˙– 25.0˙– 0.086 ˙” 10˙– 3708˙– 1.568˙– 331.3˙– 0.852
50˙– 4887˙– 2.068˙– 22.7˙– 0.192 ˙” 20˙– 3768˙– 1.593˙– 327.1˙– 0.820
˙– ˙– ˙– ˙– ˙” 30˙– 3846˙– 1.626˙– 323.1˙– 0.776
0 00˙– 4706˙– 1.991˙– 20.2˙– 0.293 ˙” 40˙– 3943˙– 1.667˙– 319.3˙– 0.723
10˙– 4535˙– 1.919˙– 17.5˙– 0.388 ˙” 50˙– 4057˙– 1.715˙– 315.7˙– 0.659
20˙– 4376˙– 1.851˙– 14.6˙– 0.478 ˙” ˙– ˙– ˙– ˙–
30˙– 4228˙– 1.789˙– 11.5˙– 0.560 ˙” 3 00˙– 4186˙– 1.769˙– 312.3˙– 0.587
40˙– 4095˙– 1.732˙– 8.1˙– 0.635 ˙” 10˙– 4330˙– 1.830˙– 309.1˙– 0.508
50˙– 3976˙– 1.682˙– 4.6˙– 0.701 ˙” 20˙– 4486˙– 1.896˙– 306.1˙– 0.421
˙– ˙– ˙– ˙– ˙” 30˙– 4654˙– 1.966˙– 303.3˙– 0.327
1 00˙– 3874˙– 1.639˙– 0.8˙– 0.758 ˙” 40˙– 4832˙– 2.042˙– 300.8˙– 0.228
10˙– 3790˙– 1.603˙– 356.9˙– 0.805 ˙” 50˙– 5019˙– 2.121˙– 298.4˙– 0.124
20˙– 3725˙– 1.575˙– 352.8˙– 0.842 ˙” ˙– ˙– ˙– ˙–
30˙– 3679˙– 1.556˙– 348.5˙– 0.867 ˙” 4 00˙– 5215˙– 2.203˙– 296.2˙– 0.014
40˙– 3655˙– 1.545˙– 344.2˙– 0.881 ˙” 10˙– 5418˙– 2.289˙– 294.1˙– ď”
50˙– 3652˙– 1.544˙– 339.9˙– 0.884 ˙” ˙– ˙– ˙– ˙–

T - universal time ( TDT - UT1 = 66.0 s );
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.