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VI. Penumbral lunar eclipse of 2016, September 16


The beginning of the eclipse is visible from Eurasia (except the Western
Europe), east of Africa, Madagascar, Australia, New Zealand, Antarctica at co-
ast of Indian ocean, west of Pacific, and Indian oceans.
The end of the eclipse is visible from Eurasia (except the extreme east),
Africa, west of Australia, Antarctica at coast of Indian ocean, at Indian, and
Atlantic oceans.


Universal time of geocentric opposition
h m s
in right ascension 2016, September 16, 18 18 37.8

Sun Moon
h m s h m s
Right ascension . . . . . . . . . . . . . 11 39 04.375 23 39 04.375
s s
Hourly motion . . . . . . . . . . . . . + 8.960 +139.476
я€ ' " я€ ' "
Declination. . . . . . . . . . . . . . . . + 2 15 48.62 - 3 22 24.26
" "
Hourly motion . . . . . . . . . . . . . -57.93 +684.91
" я€ ' "
Equatorial horizontal parallax . . . . . . 8.75 1 00 06.01
' " ' "
Apparent semidiameter . . . . . . . . . . 15 54.75 16 22.61



Circumstances of the Eclipse
Position Angles
of the Moon's axis
h m o
Moon enters penumbra . . . . . . . September 16, 16 52.9 335.20
Greatest eclipse . . . . . . . . . 18 54.4 335.16
Moon leaves penumbra . . . . . . . 20 56.1 335.13


-----------------------------------------------
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 | 29 45.8 | - 3 40.2 | 104 39.4 E
Last | 294 29.8 | - 2 53.5 | 46 01.7 E

Magnitude of the eclipse 0.930
"
Angular radius of the penumbra 4661.37
"
Angular radius of the umbra 2713.97


-------------------------------------------------------------------------------
T | s | d | P |Magnitudes of! T | s | d | P |Magnitudes of
| | | | penumbral ! | | | | penumbral
-----|-----|------|------|-------------!-----|-----|------|------|-------------
h m| "| | o | ! h m| "| | o |
16 50| 5704| 2.104| 30.4| - !19 00| 3810| 1.404| 339.3| 0.928
| | | | ! 10| 3842| 1.416| 334.1| 0.912
17 00| 5454| 2.011| 28.0| 0.090 ! 20| 3905| 1.439| 329.2| 0.881
10| 5215| 1.923| 25.4| 0.212 ! 30| 3996| 1.472| 324.4| 0.835
20| 4987| 1.839| 22.5| 0.328 ! 40| 4114| 1.515| 319.8| 0.776
30| 4774| 1.760| 19.4| 0.437 ! 50| 4256| 1.567| 315.5| 0.704
40| 4575| 1.687| 16.0| 0.537 ! | | | |
50| 4394| 1.620| 12.3| 0.629 !20 00| 4420| 1.628| 311.6| 0.621
| | | | ! 10| 4603| 1.695| 307.9| 0.528
18 00| 4234| 1.561| 8.2| 0.711 ! 20| 4804| 1.769| 304.5| 0.426
10| 4095| 1.509| 3.9| 0.781 ! 30| 5021| 1.849| 301.4| 0.317
20| 3981| 1.467| 359.3| 0.839 ! 40| 5251| 1.933| 298.6| 0.200
30| 3894| 1.435| 354.5| 0.884 ! 50| 5493| 2.022| 296.0| 0.078
40| 3836| 1.414| 349.5| 0.914 ! | | | |
50| 3807| 1.403| 344.4| 0.929 !21 00| 5745| 2.115| 293.6| -

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.