III. Total lunar eclipse of 2025, March 14 The beginning of the eclipse is visible from western Europe, in western Africa, in the Americas, Greenland, on the Pacific coast of Antarctica, in the eastern half of the Pacific and in the Atlantic oceans. The end of the eclipse is visible from the North and western of South Ame- rica, Australia, New Zealand, eastern Asia, the Pacific coast of Antarctica, in the Pacific Ocean. Universal time of geocentric opposition h m s in right ascension 2025, March 14, 6 35 59.5 Sun Moon h m s h m s Right ascension . . . . . . . . . . . . . 23 37 42.484 11 37 42.485 s s Hourly motion . . . . . . . . . . . . . + 9.160 +106.642 o ' " o ' " Declination. . . . . . . . . . . . . . . . 2 24 39.31 + 2 46 25.60 " " Hourly motion . . . . . . . . . . . . . +59.18 -871.07 " ' " Equatorial horizontal parallax . . . . . . 8.85 54 37.05 ' " ' " Apparent semidiameter . . . . . . . . . . 16 05.24 14 52.99 Circumstances of the Eclipse Position Angles of the Moon's axis h m o Moon enters penumbra . . . . . . . March 14, 3 57.7 21.72 Moon enters umbra . . . . . . . . 5 09.4 21.74 Moon enters totality . . . . . . . 6 25.9 21.77 Greatest eclipse . . . . . . . . . 7 04.9 21.78 Moon leaves totality . . . . . . . 7 32.2 21.78 Moon leaves umbra . . . . . . . . 8 48.4 21.80 Moon leaves penumbra . . . . . . . 10 02.9 21.82 -------------------------------------------- Contacts| Position |The Moon being in the Zenith in of umbra| Angles |---------------------- with Limb| from the | | of Moon |North Point| Latitude | Longitude ---------|-----------|----------|----------- | o ' | o ' | o ' First | 139 34.4 | + 3 08.6 | 75 37.9 W Last | 278 36.0 | + 2 15.3 | 128 55.6 W Magnitude of the eclipse 1.181 " Angular radius of the penumbra 4335.12 " Angular radius of the umbra 2366.54 -------------------------------------------------------------------------------- | | | |Magnitudes of I | | | |Magnitudes of T | s | d | P |--------------I T | s | d | P |------------- | | | |umbral| penum.I | | | |umbral| penum. | | | eclipse|eclipseI | | | eclipse|eclipse -----|-----|------|------|------|-------I-----|-----|------|------|------|------ h m| "| | o | | I h m| "| | o | | 3 50│ 5414| 2.284| 131.2| - | - I 7 00│ 1142| 0.482| 209.2| 1.186| 2.288 │ | | | | I 10│ 1176| 0.497| 222.9| 1.167| 2.269 4 00│ 5142| 2.170| 131.9| - | 0.050 I 20│ 1271| 0.537| 235.1| 1.113| 2.216 10│ 4871| 2.055| 132.6| - | 0.202 I 30│ 1416| 0.598| 245.3| 1.032| 2.135 20│ 4600| 1.941| 133.4| - | 0.353 I 40│ 1596| 0.675| 253.4| 0.931| 2.034 30│ 4331| 1.828| 134.3| - | 0.504 I 50│ 1802| 0.761| 259.7| 0.816| 1.919 40│ 4062| 1.715| 135.4| - | 0.654 I │ | | | | 50│ 3796| 1.602| 136.6| - | 0.803 I 8 00│ 2025| 0.856| 264.7| 0.691| 1.794 │ | | | | I 10│ 2260| 0.955| 268.7| 0.559| 1.662 5 00│ 3531| 1.491| 137.9| - | 0.951 I 20│ 2504| 1.058| 271.9| 0.423| 1.525 10│ 3268| 1.380| 139.5| - | 1.098 I 30│ 2755| 1.164| 274.6| 0.282| 1.385 20│ 3009| 1.270| 141.4| 0.141| 1.243 I 40│ 3010| 1.272| 276.8| 0.139| 1.242 30│ 2753| 1.163| 143.6| 0.285| 1.387 I 50│ 3269| 1.382| 278.6| - | 1.097 40│ 2502| 1.057| 146.2| 0.425| 1.527 I │ | | | | 50│ 2258| 0.954| 149.4| 0.562| 1.664 I 9 00│ 3531| 1.493| 280.2| - | 0.950 │ | | | | I 10│ 3795| 1.604| 281.6| - | 0.802 6 00│ 2022| 0.854| 153.4| 0.693| 1.795 I 20│ 4061| 1.717| 282.7| - | 0.653 10│ 1799| 0.760| 158.4| 0.818| 1.920 I 30│ 4329| 1.830| 283.8| - | 0.503 20│ 1594| 0.673| 164.8| 0.933| 2.035 I 40│ 4598| 1.944| 284.7| - | 0.352 30│ 1414| 0.597| 172.9| 1.034| 2.136 I 50│ 4868| 2.058| 285.5| - | 0.201 40│ 1269| 0.536| 183.1| 1.114| 2.217 I │ | | | | 50│ 1175| 0.496| 195.4| 1.167| 2.270 I10 00│ 5138| 2.172| 286.2| - | 0.049 │ | | | | I 10│ 5410| 2.287| 286.9| - | - T - universal time ( TDT - UT1 = 69.0s); 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.