Penumbral lunar eclipse of 2017, February 11 The beginning of the eclipse is visible from Eurasia (except the extreme east), Africa, Madagascar, east of Northern and South America, Greenland, In- dian, Atlantic, and Arctic oceans. The end of the eclipse is visible from Europe, Africa, America, Greenland, east of Pacific, and Atlantic oceans. Universal time of geocentric opposition h m s in right ascension 2017, February 11, 1 10 40.2 Sun Moon h m s h m s Right ascension . . . . . . . . . . . . . 21 39 23.609 9 39 23.609 s s Hourly motion . . . . . . . . . . . . . +9.856 +136.616 o ' " o ' " Declination. . . . . . . . . . . . . . . . -14 00 45.77 +12 59 31.78 " " Hourly motion . . . . . . . . . . . . . +49.33 -490.22 " ' " Equatorial horizontal parallax . . . . . . 8.91 58 04.96 ' " ' " Apparent semidiameter . . . . . . . . . . 16 12.32 15 49.64 Circumstances of the Eclipse Position Angles of the Moon's axis h m o Moon enters penumbra . . . . . . . February 10, 22 32.1 20.11 Greatest eclipse . . . . . . . . . 11, 0 43.8 20.43 Moon leaves penumbra . . . . . . . 2 55.4 20.73 ----------------------------------------------- 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 | 62 34.6 | +13 26.1 | 24 08.0 E Last | 324 11.1 | +12 50.2 | 39 22.8 W Magnitude of the eclipse 1.011 " Angular radius of the penumbra 4555.95 " Angular radius of the umbra 2572.68 ------------------------------------------------------------------------------- T | s | d | P |Magnitudes of! T | s | d | P |Magnitudes of | | | | penumbral ! | | | | penumbral -----|-----|------|------|-------------!-----|-----|------|------|------------- h m| "| | o | ! h m| "| | o | 22 30| 5558| 2.157| 63.0| - ! 0 50| 3580| 1.391| 10.2| 1.008 40| 5318| 2.065| 60.8| 0.100 ! | | | | 50| 5087| 1.975| 58.4| 0.221 ! 1 00| 3611| 1.404| 5.2| 0.992 | | | | ! 10| 3669| 1.427| 0.3| 0.961 23 00| 4866| 1.889| 55.8| 0.337 ! 20| 3754| 1.460| 355.6| 0.916 10| 4656| 1.808| 53.0| 0.447 ! 30| 3863| 1.502| 351.1| 0.859 20| 4459| 1.732| 49.9| 0.550 ! 40| 3994| 1.553| 346.9| 0.790 30| 4276| 1.661| 46.5| 0.645 ! 50| 4145| 1.612| 343.0| 0.710 40| 4110| 1.597| 42.8| 0.732 ! | | | | 50| 3963| 1.540| 38.8| 0.809 ! 2 00| 4315| 1.678| 339.4| 0.621 | | | | ! 10| 4500| 1.751| 336.1| 0.524 0 00| 3836| 1.491| 34.5| 0.875 ! 20| 4699| 1.828| 333.0| 0.419 10| 3733| 1.450| 30.0| 0.929 ! 30| 4911| 1.911| 330.3| 0.307 20| 3654| 1.420| 25.2| 0.970 ! 40| 5134| 1.998| 327.7| 0.190 30| 3601| 1.400| 20.3| 0.998 ! 50| 5366| 2.088| 325.4| 0.068 40| 3576| 1.390| 15.3| 1.010 ! | | | | | | | | ! 3 00| 5606| 2.182| 323.2| - 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.