Äîęóěĺíň âç˙ň čç ęýřŕ ďîčńęîâîé ěŕřčíű. Ŕäđĺń îđčăčíŕëüíîăî äîęóěĺíňŕ : http://www.ipa.nw.ru/PAGE/EDITION/ENG/AE/e20020624lua.txt Äŕňŕ čçěĺíĺíč˙: Wed Mar 2 14:51:02 2016 Äŕňŕ číäĺęńčđîâŕíč˙: Sun Apr 10 02:06:33 2016 Ęîäčđîâęŕ: Ďîčńęîâűĺ ńëîâŕ: ď ď ď ď ď

Penumbral Lunar Eclipse of 2002 June 24


The beginning of the eclipse visible in Europe except the northern part,
Asia except the north-eastern part, Indonesia, Australia, Antarctica, Africa,
Madagaskar, the extreme west of the Pacific Ocean, the Indian Ocean, and the
southern Atlantic Ocean.
The end of the eclipse visible in Europe except the northern part, south-
western Asia, western Australia, Antarctica, Africa, Madagaskar, South Ameri-
ca except the north-west, the Indian Ocean, and most of the Atlantic Ocean.


Universal time of geocentric opposition
h m s
in right ascension 2002, June 24, 21 38 27.5

Sun Moon
h m s h m s
Right ascension . . . . . . . . . . . . . 6 13 53.935 18 13 53.935
s s
Hourly motion . . . . . . . . . . . . . +10.387 +148.329
˙ˆ ' " ˙ˆ ' "
Declination . . . . . . . . . . . . . . . +23 24 03.13 -24 47 29.57
" "
Hourly motion . . . . . . . . . . . . . -3.46 -130.25
" ' "
Equatorial horizontal parallax . . . . . . 8.65 57 38.08
' " ' "
Apparent semidiameter . . . . . . . . . . 15 44.15 15 42.31



Circumstances of the Eclipse
Position Angles
of the Moon's axis
h m ˙ˆ
Moon enters penumbra . . . . . . . . June 24, 20 18.6 357.47
Greatest eclipse . . . . . . . . . 21 26.9 357.19
Moon leaves penumbra . . . . . . . . 22 35.2 356.92

ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”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 ˙– 27 41.7 ˙– -24 53.3 ˙– 55 11.0 E
Last ˙– 340 41.2 ˙– -24 58.3 ˙– 22 21.3 E


Magnitude of the eclipse 0.232
"
Angular radius of the penumbra 4499.01
"
Angular radius of the umbra 2573.48

ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď˘ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”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 ˙–
20 10˙– 5549˙– 2.154˙– 30.3˙– ď” ˙”21 30˙– 4995˙– 1.941˙– 3.1˙– 0.232
20˙– 5419˙– 2.104˙– 27.3˙– 0.009 ˙” 40˙– 5010˙– 1.947˙– 359.4˙– 0.224
30˙– 5305˙– 2.060˙– 24.1˙– 0.069 ˙” 50˙– 5045˙– 1.961˙– 355.8˙– 0.205
40˙– 5208˙– 2.023˙– 20.8˙– 0.120 ˙” ˙– ˙– ˙– ˙–
50˙– 5128˙– 1.992˙– 17.4˙– 0.163 ˙”22 00˙– 5099˙– 1.982˙– 352.3˙– 0.176
˙– ˙– ˙– ˙– ˙” 10˙– 5172˙– 2.011˙– 348.9˙– 0.137
21 00˙– 5066˙– 1.968˙– 13.9˙– 0.195 ˙” 20˙– 5262˙– 2.046˙– 345.5˙– 0.090
10˙– 5022˙– 1.951˙– 10.3˙– 0.218 ˙” 30˙– 5369˙– 2.088˙– 342.3˙– 0.033
20˙– 4999˙– 1.942˙– 6.7˙– 0.230 ˙” 40˙– 5492˙– 2.136˙– 339.2˙– 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.