Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.ipa.nw.ru/PAGE/EDITION/ENG/AE/e20131019lua.txt Äàòà èçìåíåíèÿ: Wed Mar 2 14:51:03 2016 Äàòà èíäåêñèðîâàíèÿ: Sun Apr 10 02:11:08 2016 Êîäèðîâêà:

V. Partial lunar eclipse of 2013 October 18-19


The beginning of the eclipse is visible from Eurasia (except for extreme
east), Africa and Madagascar, east of Northern and South Americas, Greenland,
Arctic, Indian and Atlantic oceans.
The end of the eclipse is visible from Europe, west of Asia, Africa and Ma-
dagascar, Northern and South Americas, Greenland, Arctic ocean, west of Indian,
Atlantic and east of Pasific oceans.



Universal time of geocentric opposition
h m s
in right ascension 2013, October 19, 0 26 43.6


Sun Moon
h m s h m s
Right ascension . . . . . . . . . . . . . 13 35 37.585 1 35 37.584
s s
Hourly motion . . . . . . . . . . . . . + 9.391 +128.499
o ' " o ' "
Declination. . . . . . . . . . . . . . . . - 9 57 47.80 +11 05 45.60
" "
Hourly motion . . . . . . . . . . . . . -54.15 +547.97
" ' "
Equatorial horizontal parallax . . . . . . 8.83 56 49.86
' " ' "
Apparent semidiameter . . . . . . . . . . 16 03.43 15 29.17



Circumstances of the Eclipse
Position Angles
of the Moon's axis
h m o
Moon enters penumbra . . . . . . . October 18, 21 48.2 336.94
Greatest eclipse . . . . . . . . . 23 50.2 337.12
Moon leaves penumbra . . . . . . . 19, 1 52.0 337.30

---------T-----------T----------------------
ContactsᦠPosition á¦The Moon being in the Zenith in
of penum.ᦠAngles +----------T-----------
with Limbᦠfrom the ᦠᦠMagnitude of the eclipse 0.788
of Moon á¦North PointᦠLatitude ᦠLongitude "
---------+-----------+----------+----------- Angular radius of the penumbra 4470.37
ᦠo ' ᦠo ' ᦠo ' "
First ᦠ120 36.6 ᦠ+10 45.6 ᦠ27 53.8 E Angular radius of the umbra 2505.31
Last ᦠ207 38.8 ᦠ+11 23.1 ᦠ31 01.8 W

-----T-----T------T------T-------------T-----T-----T------T------T-------------
ᦠᦠᦠá¦Magnitudes ofᦠᦠᦠᦠá¦Magnitudes of
T ᦠs ᦠd ᦠP ᦠpenumbral ᦠT ᦠs ᦠd ᦠP ᦠpenumbral
ᦠᦠᦠᦠeclipse ᦠᦠᦠᦠᦠeclipse
-----+-----+------+------+-------------+-----+-----+------+------+-------------
h mᦠ"ᦠᦠo ᦠᦠh mᦠ"ᦠᦠo á¦
21 40ᦠ5575ᦠ2.222ᦠ118.7ᦠ- ᦠ0 00ᦠ3936ᦠ1.571ᦠ168.5ᦠ0.782
50ᦠ5363ᦠ2.138ᦠ121.0ᦠ0.020 ᦠ10ᦠ3970ᦠ1.585ᦠ172.9ᦠ0.763
ᦠᦠᦠᦠᦠ20ᦠ4027ᦠ1.608ᦠ177.2ᦠ0.732
22 00ᦠ5161ᦠ2.058ᦠ123.5ᦠ0.129 ᦠ30ᦠ4106ᦠ1.640ᦠ181.3ᦠ0.690
10ᦠ4969ᦠ1.981ᦠ126.2ᦠ0.231 ᦠ40ᦠ4205ᦠ1.679ᦠ185.3ᦠ0.636
20ᦠ4788ᦠ1.910ᦠ129.1ᦠ0.328 ᦠ50ᦠ4323ᦠ1.727ᦠ189.1ᦠ0.573
30ᦠ4621ᦠ1.843ᦠ132.2ᦠ0.417 ᦠᦠᦠᦠá¦
40ᦠ4468ᦠ1.782ᦠ135.5ᦠ0.499 ᦠ1 00ᦠ4459ᦠ1.781ᦠ192.7ᦠ0.500
50ᦠ4331ᦠ1.728ᦠ139.1ᦠ0.572 ᦠ10ᦠ4611ᦠ1.842ᦠ196.0ᦠ0.418
ᦠᦠᦠᦠᦠ20ᦠ4777ᦠ1.908ᦠ199.1ᦠ0.329
23 00ᦠ4211ᦠ1.680ᦠ142.9ᦠ0.636 ᦠ30ᦠ4956ᦠ1.980ᦠ202.0ᦠ0.232
10ᦠ4111ᦠ1.640ᦠ146.8ᦠ0.690 ᦠ40ᦠ5147ᦠ2.056ᦠ204.7ᦠ0.130
20ᦠ4031ᦠ1.609ᦠ151.0ᦠ0.732 ᦠ50ᦠ5348ᦠ2.137ᦠ207.2ᦠ0.021
30ᦠ3973ᦠ1.585ᦠ155.3ᦠ0.763 ᦠᦠᦠᦠá¦
40ᦠ3937ᦠ1.571ᦠ159.6ᦠ0.782 ᦠ2 00ᦠ5558ᦠ2.221ᦠ209.5ᦠ-
50ᦠ3925ᦠ1.567ᦠ164.1ᦠ0.788 ᦠᦠᦠᦠá¦

T - universal time (TDT-UT1= 67.0s);
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.