Äîęóěĺíň âç˙ň čç ęýřŕ ďîčńęîâîé ěŕřčíű. Ŕäđĺń îđčăčíŕëüíîăî äîęóěĺíňŕ : http://www.ipa.nw.ru/PAGE/EDITION/ENG/AE/e20020526lua.txt Äŕňŕ čçěĺíĺíč˙: Wed Mar 2 14:51:02 2016 Äŕňŕ číäĺęńčđîâŕíč˙: Sun Apr 10 02:06:25 2016 Ęîäčđîâęŕ: Ďîčńęîâűĺ ńëîâŕ: ď ď ď ď ď ď ď ď ď ď ď ď ď

Penumbral Lunar Eclipse of 2002 May 26


The beginning of the eclipse visible in North America except the north-
east, the western coast of South America, Antarctica, Australia, New Zealand,
New Guinea, the Pacific Ocean.
The end of the eclipse visible in south-eastern Asia, Antarctica, Austra-
lia, New Zealand, the Pacific Ocean except the extreme eastern part, the eas-
tern Indian Ocean.


Universal time of geocentric opposition
h m s
in right ascension 2002, May 26, 11 27 35.1

Sun Moon
h m s h m s
Right ascension . . . . . . . . . . . . . 4 12 25.005 16 12 25.005
s s
Hourly motion . . . . . . . . . . . . . +10.123 +146.085
˙š ' " ˙š ' "
Declination . . . . . . . . . . . . . . . +21 08 21.87 -19 55 56.68
" "
Hourly motion . . . . . . . . . . . . . +25.90 -571.22
" ' "
Equatorial horizontal parallax . . . . . . 8.68 59 15.32
' " ' "
Apparent semidiameter . . . . . . . . . . 15 47.30 16 08.81



Circumstances of the Eclipse
Position Angles
of the Moon's axis
h m ˙š
Moon enters penumbra . . . . . . . . May 26, 10 12.9 9.16
Greatest eclipse . . . . . . . . . 12 03.2 8.75
Moon leaves penumbra . . . . . . . . 13 53.9 8.33

ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”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”ď”ď”
˙– ˙š ' ˙– ˙š ' ˙– ˙š '
First ˙– 154 49.2 ˙– -19 51.3 ˙– 154 40.7 W
Last ˙– 236 38.9 ˙– -20 26.3 ˙– 152 08.7 E


Magnitude of the eclipse 0.712
"
Angular radius of the penumbra 4600.34
"
Angular radius of the umbra 2668.24


ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď˘ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”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 ˙–
10 10˙– 5627˙– 2.107˙– 154.1˙– ď” ˙”12 10˙– 4185˙– 1.569˙– 198.8˙– 0.709
20˙– 5410˙– 2.026˙– 156.7˙– 0.079 ˙” 20˙– 4216˙– 1.580˙– 203.2˙– 0.694
30˙– 5205˙– 1.949˙– 159.5˙– 0.185 ˙” 30˙– 4272˙– 1.602˙– 207.6˙– 0.665
40˙– 5014˙– 1.878˙– 162.5˙– 0.283 ˙” 40˙– 4353˙– 1.632˙– 211.9˙– 0.623
50˙– 4838˙– 1.812˙– 165.8˙– 0.373 ˙” 50˙– 4458˙– 1.671˙– 215.9˙– 0.570
˙– ˙– ˙– ˙– ˙” ˙– ˙– ˙– ˙–
11 00˙– 4679˙– 1.753˙– 169.2˙– 0.455 ˙”13 00˙– 4584˙– 1.719˙– 219.8˙– 0.505
10˙– 4540˙– 1.701˙– 173.0˙– 0.527 ˙” 10˙– 4730˙– 1.774˙– 223.4˙– 0.430
20˙– 4421˙– 1.656˙– 176.9˙– 0.588 ˙” 20˙– 4894˙– 1.835˙– 226.8˙– 0.345
30˙– 4324˙– 1.620˙– 181.0˙– 0.638 ˙” 30˙– 5074˙– 1.903˙– 230.0˙– 0.252
40˙– 4251˙– 1.593˙– 185.3˙– 0.675 ˙” 40˙– 5270˙– 1.977˙– 232.9˙– 0.151
50˙– 4203˙– 1.575˙– 189.7˙– 0.700 ˙” 50˙– 5478˙– 2.055˙– 235.6˙– 0.044
˙– ˙– ˙– ˙– ˙” ˙– ˙– ˙– ˙–
12 00˙– 4181˙– 1.567˙– 194.2˙– 0.711 ˙”14 00˙– 5698˙– 2.138˙– 238.2˙– ď”

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.