II. Penumbral lunar eclipse of 2024, March 25 The beginning of the eclipse is visible from western Europe, western Afri- ca, the Americas, Greenland, 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 Americas, Australia, New Zealand, the Far East, the Pacific coast of Antarctica, and the Pacific Ocean. Universal time of geocentric opposition h m s in right ascension 2024, March 25, 6 02 49.3 Sun Moon h m s h m s Right ascension . . . . . . . . . . . . . 0 18 39.311 12 18 39.311 s s Hourly motion . . . . . . . . . . . . . +9.098 +104.500 o ' " o ' " Declination. . . . . . . . . . . . . . . . +2 01 07.89 -0 55 30.52 " " Hourly motion . . . . . . . . . . . . . +58.89 -852.58 " ' " Equatorial horizontal parallax . . . . . . 8.82 54 05.00 ' " ' " Apparent semidiameter . . . . . . . . . . 16 02.24 14 44.25 Circumstances of the Eclipse Position Angles of the Moon's axis h m o Moon enters penumbra . . . . . . . March 25, 4 51.2 21.85 Greatest eclipse . . . . . . . . . 7 12.9 21.81 Moon leaves penumbra . . . . . . . 9 35.0 21.76 ----------------------------------------------- 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 | 160 44.5 │ - 0 38.8 │ 71 48.1 W Last | 257 22.6 │ - 1 46.5 │ 140 52.7 W Magnitude of the eclipse 0.980 " Angular radius of the penumbra 4300.57 " Angular radius of the umbra 2337.88 ------------------------------------------------------------------------------ T | s | d | P |Magnitudes ofI T | s | d | P |Magnitudes of | | | | penumbral I | | | | penumbral -----|-----|------|------|-------------I-----|-----|------|------|------------ h m│ "│ │ o │ I h m│ "│ │ o │ 4 50│ 5198│ 2.224│ 160.5│ ─ I 7 20│ 3449│ 1.475│ 212.3│ 0.977 │ │ │ │ I 30│ 3475│ 1.486│ 216.8│ 0.963 5 00│ 4997│ 2.138│ 162.6│ 0.100 I 40│ 3522│ 1.506│ 221.2│ 0.937 10│ 4804│ 2.055│ 164.8│ 0.209 I 50│ 3589│ 1.535│ 225.4│ 0.899 20│ 4618│ 1.976│ 167.2│ 0.315 I │ │ │ │ 30│ 4441│ 1.900│ 169.9│ 0.415 I 8 00│ 3676│ 1.572│ 229.5│ 0.851 40│ 4274│ 1.828│ 172.7│ 0.509 I 10│ 3780│ 1.617│ 233.4│ 0.792 50│ 4118│ 1.762│ 175.8│ 0.597 I 20│ 3900│ 1.668│ 237.0│ 0.725 │ │ │ │ I 30│ 4036│ 1.726│ 240.4│ 0.648 6 00│ 3975│ 1.701│ 179.0│ 0.678 I 40│ 4185│ 1.789│ 243.6│ 0.565 10│ 3846│ 1.645│ 182.6│ 0.751 I 50│ 4346│ 1.858│ 246.6│ 0.474 20│ 3732│ 1.597│ 186.3│ 0.815 I │ │ │ │ 30│ 3636│ 1.555│ 190.3│ 0.870 I 9 00│ 4517│ 1.932│ 249.3│ 0.377 40│ 3558│ 1.522│ 194.4│ 0.914 I 10│ 4798│ 2.009│ 251.9│ 0.275 50│ 3499│ 1.497│ 198.8│ 0.948 I 20│ 4888│ 2.090│ 254.2│ 0.168 │ │ │ │ I 30│ 5086│ 2.174│ 256.4│ 0.057 7 00│ 3461│ 1.480│ 203.2│ 0.970 I 40│ 5290│ 2.262│ 258.4│ ─ 10│ 3444│ 1.473│ 207.7│ 0.979 I │ │ │ │ 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.