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IV. Penumbral lunar eclipse of 2016, March 23


The beginning of the eclipse is visible from extreme east of Asia, Austra-
lia, New Zealand, Northern and west of South America, Pacific coast of Antarc-
tica, Pacific ocean.
The end of the eclipse is visible from Asia, Australia, New Zealand, west
of Northern America, Pacific coast of Antarctica, east of Indian, and Pacific
oceans.


Universal time of geocentric opposition
h m s
in right ascension 2016, March 23, 11 03 11.1

Sun Moon
h m s h m s
Right ascension . . . . . . . . . . . . . 0 11 55.280 12 11 55.278
s s
Hourly motion . . . . . . . . . . . . . + 9.100 +113.473
я€ ' " я€ ' "
Declination. . . . . . . . . . . . . . . . + 1 17 27.59 - 0 11 30.22
" "
Hourly motion . . . . . . . . . . . . . +59.06 -560.16
" ' "
Equatorial horizontal parallax . . . . . . 8.82 54 11.95
' " ' "
Apparent semidiameter . . . . . . . . . . 16 02.69 14 46.15



Circumstances of the Eclipse
Position Angles
of the Moon's axis
h m o
Moon enters penumbra . . . . . . . March 23, 9 37.2 24.95
Greatest eclipse . . . . . . . . . 11 47.2 24.92
Moon leaves penumbra . . . . . . . 13 57.5 24.88

-----------------------------------------------
Contacts | Position |The Moon being in the Zenith in
of penumbra| Angles |------------------------
with Limb | from the | |
of Moon |North Point| Latitude | Longitude
----------|-----------|----------|-------------
| o ' | o ' | o '
First | 154 22.1 | + 0 01.9 | 143 18.5 W
Last | 241 10.1 | - 0 38.9 | 153 28.9 E

Magnitude of the eclipse 0.798
"
Angular radius of the penumbra 4307.34
"
Angular radius of the umbra 2343.77


-------------------------------------------------------------------------------
T | s | d | P |Magnitudes of! T | s | d | P |Magnitudes of
| | | | penumbral ! | | | | penumbral
-----|-----|------|------|-------------!-----|-----|------|------|-------------
h m| "| | o | ! h m| "| | o |
9 30| 5323| 2.270| 152.8| - !11 50| 3770| 1.608| 198.9| 0.798
40| 5133| 2.189| 155.0| 0.030 ! | | | |
50| 4951| 2.112| 157.3| 0.132 !12 00| 3785| 1.615| 203.1| 0.789
| | | | ! 10| 3820| 1.630| 207.2| 0.770
10 00| 4778| 2.038| 159.8| 0.229 ! 20| 3874| 1.653| 211.1| 0.740
10| 4615| 1.968| 162.5| 0.321 ! 30| 3947| 1.684| 215.0| 0.699
20| 4462| 1.903| 165.4| 0.407 ! 40| 4037| 1.723| 218.7| 0.649
30| 4322| 1.843| 168.5| 0.486 ! 50| 4143| 1.768| 222.3| 0.589
40| 4195| 1.789| 171.7| 0.558 ! | | | |
50| 4082| 1.741| 175.2| 0.621 !13 00| 4264| 1.820| 225.6| 0.521
| | | | ! 10| 4398| 1.877| 228.8| 0.446
11 00| 3985| 1.700| 178.8| 0.676 ! 20| 4545| 1.940| 231.7| 0.363
10| 3904| 1.666| 182.6| 0.721 ! 30| 4704| 2.008| 234.5| 0.274
20| 3842| 1.639| 186.6| 0.757 ! 40| 4873| 2.080| 237.1| 0.179
30| 3798| 1.621| 190.6| 0.781 ! 50| 5051| 2.156| 239.5| 0.078
40| 3774| 1.610| 194.8| 0.795 ! | | | |
| | | | !14 00| 5237| 2.235| 241.7| -

T - universal time;
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.