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 ш ' " ш ' " Declination. . . . . . . . . . . . . . . . + 2 15 48.62 - 3 22 24.26 " " Hourly motion . . . . . . . . . . . . . -57.93 +684.91 " ш ' " 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.