Penumbral lunar eclipse of 2020, June 5 The beginning of the eclipse is visible from the south of Eurasia, east of Africa, Madagascar, Australia, New Zealand, Antarctica at coast of Indian oce- an, west of Pacific, and Indian oceans. The end of the eclipse is visible from a southwest part of Eurasia, Africa, Madagascar, Australia, east of the South America, African coast of Antarctica, south of Atlantic, and Indian oceans. Universal time of geocentric opposition h m s in right ascension 2020, June 5, 18 57 47.9 Sun Moon h m s h m s Right ascension . . . . . . . . . . . . . 4 57 16.927 16 57 16.926 s s Hourly motion . . . . . . . . . . . . . +10.307 +150.963 o ' " o ' " Declination. . . . . . . . . . . . . . . . +22 39 14.31 -21 23 58.43 " " Hourly motion . . . . . . . . . . . . . +15.42 -420.72 " ' " Equatorial horizontal parallax . . . . . . 8.67 59 25.73 ' " ' " Apparent semidiameter . . . . . . . . . . 15 45.70 16 11.64 Circumstances of the Eclipse Position Angles of the Moon's axis h m o Moon enters penumbra . . . . . . . June 5, 17 43.6 4.99 Greatest eclipse . . . . . . . . . 19 25.0 4.58 Moon leaves penumbra . . . . . . . 21 06.6 4.16 ----------------------------------------------- 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 | 154 25.3 ¦ -21 23.0 ¦ 93 02.5 E Last | 228 38.5 ¦ -21 46.6 ¦ 44 16.6 E Magnitude of the eclipse 0.591 " Angular radius of the penumbra 4609.52 " Angular radius of the umbra 2680.71 ------------------------------------------------------------------------------ T | s | d | P |Magnitudes ofI T | s | d | P |Magnitudes of | | | | penumbral I | | | | penumbral -----|-----|------|------|-------------I-----|-----|------|------|------------ h m¦ "¦ ¦ o ¦ I h m¦ "¦ ¦ o ¦ 17 40¦ 5649¦ 2.105¦ 153.5¦ Д I19 30¦ 4426¦ 1.651¦ 193.7¦ 0.590 50¦ 5447¦ 2.030¦ 156.2¦ 0.066 I 40¦ 4451¦ 1.661¦ 197.9¦ 0.577 ¦ ¦ ¦ ¦ I 50¦ 4501¦ 1.679¦ 202.1¦ 0.551 18 00¦ 5259¦ 1.960¦ 159.1¦ 0.162 I ¦ ¦ ¦ ¦ 10¦ 5086¦ 1.896¦ 162.3¦ 0.251 I20 00¦ 4575¦ 1.707¦ 206.2¦ 0.513 20¦ 4929¦ 1.838¦ 165.6¦ 0.332 I 10¦ 4671¦ 1.743¦ 210.1¦ 0.464 30¦ 4791¦ 1.786¦ 169.2¦ 0.402 I 20¦ 4789¦ 1.787¦ 213.9¦ 0.403 40¦ 4672¦ 1.742¦ 172.9¦ 0.463 I 30¦ 4927¦ 1.839¦ 217.4¦ 0.333 50¦ 4576¦ 1.706¦ 176.8¦ 0.513 I 40¦ 5083¦ 1.897¦ 220.8¦ 0.253 ¦ ¦ ¦ ¦ I 50¦ 5255¦ 1.962¦ 223.9¦ 0.164 19 00¦ 4501¦ 1.679¦ 180.9¦ 0.551 I ¦ ¦ ¦ ¦ 10¦ 4451¦ 1.660¦ 185.1¦ 0.576 I21 00¦ 5443¦ 2.032¦ 226.8¦ 0.067 20¦ 4426¦ 1.651¦ 189.4¦ 0.589 I 10¦ 5644¦ 2.107¦ 229.5¦ Д 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.