Penumbral lunar eclipse of 2023, May 5 The beginning of the eclipse is visible from Asia, Australia, New Zealand, Madagascar, the western half of the Pacific and the Indian Oceans. The end of the eclipse is visible from southern Asia, Australia, Europe, Africa, the Indian and eastern Atlantic oceans. Universal time of geocentric opposition h m s in right ascension 2023, May 5, 18 10 27.6 Sun Moon h m s h m s Right ascension . . . . . . . . . . . . . 2 50 07.313 14 50 07.313 s s Hourly motion . . . . . . . . . . . . . + 9.650 +131.182 ° ' " ° ' " Declination. . . . . . . . . . . . . . . . +16 20 01.61 -17 24 40.66 " " Hourly motion . . . . . . . . . . . . . +42.58 -766.60 " ' " Equatorial horizontal parallax . . . . . . 8.72 57 41.30 ' " ' " Apparent semidiameter . . . . . . . . . . 15 51.55 15 43.19 Circumstances of the Eclipse Position Angles of the Moon's axis h m o Moon enters penumbra . . . . . . . May 5, 15 11.9 15.97 Greatest eclipse . . . . . . . . . 17 23.0 15.65 Moon leaves penumbra . . . . . . . 19 33.6 15.32 ----------------------------------------------- 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 | 71 58.8 │ -16 52.7 │ 129 42.4 E Last | 333 29.1 │ -17 49.0 │ 66 28.5 E Magnitude of the eclipse 0.991 " Angular radius of the penumbra 4508.55 " Angular radius of the umbra 2567.94 ------------------------------------------------------------------------------ T | s | d | P |Magnitudes ofI T | s | d | P |Magnitudes of | | | | penumbral I | | | | penumbral -----|-----|------|------|-------------I-----|-----|------|------|------------ h m│ "│ │ o │ I h m│ "│ │ o │ 15 10| 5520| 2.152| 72.3| - I17 30| 3586| 1.396| 19.7| 0.989 20| 5285| 2.060| 70.1| 0.086 I 40| 3616| 1.408| 14.8| 0.974 30| 5060| 1.972| 67.7| 0.206 I 50| 3672| 1.430| 9.9| 0.944 40| 4843| 1.888| 65.1| 0.321 I | | | | 50| 4638| 1.808| 62.2| 0.430 I18 00| 3754| 1.461| 5.2| 0.900 | | | | I 10| 3860| 1.502| 0.8| 0.844 16 00| 4446| 1.733| 59.1| 0.532 I 20| 3988| 1.552| 356.6| 0.777 10| 4268| 1.663| 55.7| 0.627 I 30| 4136| 1.609| 352.7| 0.699 20| 4106| 1.600| 52.0| 0.713 I 40| 4301| 1.674| 349.1| 0.611 30| 3962| 1.544| 48.1| 0.789 I 50| 4483| 1.744| 345.7| 0.515 40| 3838| 1.495| 43.8| 0.855 I | | | | 50| 3737| 1.456| 39.3| 0.909 I19 00| 4679| 1.820| 342.6| 0.411 | | | | I 10| 4887| 1.901| 339.8| 0.301 17 00| 3659| 1.425| 34.6| 0.950 I 20| 5106| 1.986| 337.2| 0.185 10| 3608| 1.405| 29.7| 0.977 I 30| 5334| 2.074| 334.8| 0.065 20| 3583| 1.395| 24.8| 0.991 I 40| 5571| 2.166| 332.7| - T - universal time ( TDT - UT1 = 70.0s); 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.