Äîęóěĺíň âç˙ň čç ęýřŕ ďîčńęîâîé ěŕřčíű. Ŕäđĺń îđčăčíŕëüíîăî äîęóěĺíňŕ : http://www.ipa.nw.ru/PAGE/EDITION/ENG/AE/e20021120lua.txt Äŕňŕ čçěĺíĺíč˙: Wed Mar 2 14:51:02 2016 Äŕňŕ číäĺęńčđîâŕíč˙: Sun Apr 10 02:06:37 2016 Ęîäčđîâęŕ: Ďîčńęîâűĺ ńëîâŕ: ď ď ď ď ď ď ď ď ď ď ď ď ď ď ď ď ď ď ď

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.