Penumbral Lunar Eclipse of 2002 November 20 The beginning of the eclipse visible in Europe, Asia except the eastern part, Africa, Madagaskar, South America except the extreme south, Central Ame- rica, North America except the western coast, Greenland, the western Indian Ocean, the Arctic Ocean, and the Atlantic Ocean. The end of the eclipse visible in Europe, Africa except the south-eastern part, South and North America, Greenland, the Arctic Ocean, the Atlantic Oce- an, and the eastern Pacific Ocean. Universal time of geocentric opposition h m s in right ascension 2002, ­®пЎам 20, 1 02 08.3 Sun Moon h m s h m s Right ascension . . . . . . . . . . . . . 15 41 00.052 3 41 00.052 s s Hourly motion . . . . . . . . . . . . . +10.431 +121.750 o ' " o ' " Declination . . . . . . . . . . . . . . . -19 36 27.94 +18 32 13.04 " " Hourly motion . . . . . . . . . . . . . -34.30 +571.99 " ' " Equatorial horizontal parallax . . . . . . 8.90 54 40.29 ' " ' " Apparent semidiameter . . . . . . . . . . 16 11.16 14 53.87 Circumstances of the Eclipse Position Angles of the Moon's axis h m o Moon enters penumbra . . . . . . . . November 19, 23 32.2 348.15 Greatest eclipse . . . . . . . . . November 20, 1 46.6 348.54 Moon leaves penumbra . . . . . . . . 4 01.3 348.94 --------------------------------------------------------- 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 | 26 44.7 | +18 24.7 | 2 37.5 E Last | 295 53.5 | +19 07.5 | 62 33.7 W Magnitude of the eclipse 0.884 " Angular radius of the penumbra 4345.94 " Angular radius of the umbra 2365.04 ------------------------------------------------------------------------------- | | | | Magnitudes ║ | | | | Magnitudes T | s | d | P |of penumbral ║ T | s | d | P |of penumbral | | | | eclipse ║ | | | | eclipse -----|-----|------|------|-------------║-----|-----|------|------|------------- h m| "| | o | ║ h m| "| | o | 23 30| 5274| 2.231| 27.2| - ║ 2 00| 3670| 1.551| 335.5| 0.874 40| 5076| 2.148| 25.0| 0.086 ║ 10| 3708| 1.568| 331.3| 0.852 50| 4887| 2.068| 22.7| 0.192 ║ 20| 3768| 1.593| 327.1| 0.820 | | | | ║ 30| 3846| 1.626| 323.1| 0.776 0 00| 4706| 1.991| 20.2| 0.293 ║ 40| 3943| 1.667| 319.3| 0.723 10| 4535| 1.919| 17.5| 0.388 ║ 50| 4057| 1.715| 315.7| 0.659 20| 4376| 1.851| 14.6| 0.478 ║ | | | | 30| 4228| 1.789| 11.5| 0.560 ║ 3 00| 4186| 1.769| 312.3| 0.587 40| 4095| 1.732| 8.1| 0.635 ║ 10| 4330| 1.830| 309.1| 0.508 50| 3976| 1.682| 4.6| 0.701 ║ 20| 4486| 1.896| 306.1| 0.421 | | | | ║ 30| 4654| 1.966| 303.3| 0.327 1 00| 3874| 1.639| 0.8| 0.758 ║ 40| 4832| 2.042| 300.8| 0.228 10| 3790| 1.603| 356.9| 0.805 ║ 50| 5019| 2.121| 298.4| 0.124 20| 3725| 1.575| 352.8| 0.842 ║ | | | | 30| 3679| 1.556| 348.5| 0.867 ║ 4 00| 5215| 2.203| 296.2| 0.014 40| 3655| 1.545| 344.2| 0.881 ║ 10| 5418| 2.289| 294.1| - 50| 3652| 1.544| 339.9| 0.884 ║ | | | | T - universal time ( TDT - UT1 = 66.0 s ); 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.