Äîęóěĺíň âç˙ň čç ęýřŕ ďîčńęîâîé ěŕřčíű. Ŕäđĺń îđčăčíŕëüíîăî äîęóěĺíňŕ : http://www.ipa.nw.ru/PAGE/EDITION/ENG/AE/e20000121lua.txt Äŕňŕ čçěĺíĺíč˙: Wed Mar 2 14:51:01 2016 Äŕňŕ číäĺęńčđîâŕíč˙: Sun Apr 10 02:06:05 2016 Ęîäčđîâęŕ: Ďîčńęîâűĺ ńëîâŕ: ď ď ď ď ď ď ď ď ď ď

Total Lunar Eclipse of 2000 January 21

The beginning of the eclipse visible in Europe, western and south-western
Asia, Africa, North America, South America, Greenland,the Antarctic peninsula,
the Arctic Ocean, the Atlantic Ocean, and the eastern Pacific Ocean.
The end of the eclipse visible in Europe ( except for the south-east ),
extreme northern and north-eastern Asia, north-western Africa, North America,
South America, Greenland, Antarctic peninsula, the Arctic Ocean, the Atlantic
Ocean, and most of the Pacific Ocean.


Universal time of geocentric opposition
h m s
in right ascension 2000, January 21, 4 47 08.7

Sun Moon
h m s h m s
Right ascension . . . . . . . 20 10 33.530 8 10 33.530
s s
Hourly motion . . . . . . . +10.577 +157.962
o , ,, o , ,,
Declination . . . . . . . . . -20 03 18.19 +19 45 12.44
,, ,,
Hourly motion . . . . . . . +32.75 -277.77
,, , ,,
Equatorial horizontal parallax 8.94 60 46.78
, ,, , ,,
Apparent semidiameter . . . . 16 15.22 16 33.73



Circumstances of the Eclipse
Position Angles
of the Moon's axis
h m o
Moon enters penumbra January 21, 2 02.8 13.28
Moon enters umbra 3 01.3 13.50
Moon enters totality 4 04.5 13.75
Greatest eclipse 4 43.5 13.89
Moon leaves totality 5 22.4 14.04
Moon leaves umbra 6 25.6 14.28
Moon leaves penumbra 7 24.3 14.49

ď”ď”ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”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 Umbra˙– 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”
˙– o , ˙– o , ˙– o ,
First ˙– 79 31.0 ˙– +20 00.6 ˙– 43 39.2 W
Last ˙– 293 54.6 ˙– +19 44.7 ˙– 92 37.8 W

Magnitude of the eclipse 1.328
,,
Angular radius of the penumbra 4723.48
,,
Angular radius of the umbra 2734.03

ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď”ď˘ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď’ď”ď”ď”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 of ˙” ˙– ˙– ˙– ˙– Magnitudes of
T ˙– s ˙– d ˙– P ď“ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”áś T ˙– s ˙– d ˙– P ď“ď”ď”ď”ď”ď”ď”ď”ď’ď”ď”ď”ď”ď”ď”ď”
˙– ˙– ˙– ˙– umbral˙– penum.˙” ˙– ˙– ˙– ˙– umbral˙– penum.
˙– ˙– ˙– ˙–eclipse˙–eclipse˙” ˙– ˙– ˙– ˙–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˙– ,,˙– ˙– o ˙– ˙– ˙” h m˙– ,,˙– ˙– o ˙– ˙–
2 00˙– 5814˙–2.124˙– 85.4˙– ď” ˙– ď” ˙” 4 50˙– 1102˙–0.403˙–354.8˙– 1.316 ˙– 2.316
10˙– 5471˙–1.999˙– 84.8˙– ď” ˙– 0.125 ˙” ˙– ˙– ˙– ˙– ˙–
20˙– 5129˙–1.874˙– 84.0˙– ď” ˙– 0.297 ˙” 5 00˙– 1223˙–0.447˙–338.6˙– 1.255 ˙– 2.256
30˙– 4788˙–1.750˙– 83.2˙– ď” ˙– 0.469 ˙” 10˙– 1421˙–0.520˙–326.2˙– 1.157 ˙– 2.158
40˙– 4448˙–1.625˙– 82.2˙– ď” ˙– 0.640 ˙” 20˙– 1670˙–0.611˙–317.1˙– 1.032 ˙– 2.033
50˙– 4109˙–1.502˙– 81.1˙– ď” ˙– 0.810 ˙” 30˙– 1949˙–0.713˙–310.5˙– 0.892 ˙– 1.893
˙– ˙– ˙– ˙– ˙– ˙” 40˙– 2249˙–0.823˙–305.6˙– 0.742 ˙– 1.743
3 00˙– 3773˙–1.379˙– 79.7˙– ď” ˙– 0.979 ˙” 50˙– 2560˙–0.937˙–301.9˙– 0.585 ˙– 1.587
10˙– 3440˙–1.257˙– 78.1˙– 0.146 ˙– 1.146 ˙” ˙– ˙– ˙– ˙– ˙–
20˙– 3110˙–1.137˙– 76.1˙– 0.312 ˙– 1.312 ˙” 6 00˙– 2881˙–1.054˙–299.0˙– 0.424 ˙– 1.426
30˙– 2784˙–1.018˙– 73.6˙– 0.475 ˙– 1.475 ˙” 10˙– 3207˙–1.174˙–296.7˙– 0.260 ˙– 1.262
40˙– 2466˙–0.902˙– 70.5˙– 0.635 ˙– 1.635 ˙” 20˙– 3537˙–1.295˙–294.8˙– 0.094 ˙– 1.095
50˙– 2157˙–0.789˙– 66.5˙– 0.790 ˙– 1.790 ˙” 30˙– 3871˙–1.417˙–293.3˙– ď” ˙– 0.927
˙– ˙– ˙– ˙– ˙– ˙” 40˙– 4207˙–1.540˙–292.0˙– ď” ˙– 0.758
4 00˙– 1863˙–0.681˙– 61.2˙– 0.937 ˙– 1.938 ˙” 50˙– 4545˙–1.664˙–290.9˙– ď” ˙– 0.588
10˙– 1591˙–0.582˙– 53.9˙– 1.073 ˙– 2.074 ˙” ˙– ˙– ˙– ˙– ˙–
20˙– 1355˙–0.495˙– 43.9˙– 1.191 ˙– 2.192 ˙” 7 00˙– 4885˙–1.788˙–290.0˙– ď” ˙– 0.417
30˙– 1177˙–0.430˙– 30.2˙– 1.279 ˙– 2.280 ˙” 10˙– 5226˙–1.913˙–289.2˙– ď” ˙– 0.245
40˙– 1085˙–0.397˙– 13.1˙– 1.324 ˙– 2.325 ˙” 20˙– 5567˙–2.038˙–288.4˙– ď” ˙– 0.073
˙– ˙– ˙– ˙– ˙– ˙” 30˙– 5910˙–2.163˙–287.8˙– ď” ˙– ď”

T - universal time (TDT-UT1= 63.9s);
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.