E c l i p s e s 2011 161 ------------------------------------------------------------------------------- V. Partial solar eclipse of 2011 November 25 The eclipse is visible from New Zealand, Antarctica, southern Atlantic and southern Indian oceans. Universal time of geocentric conjunction h m s in right ascension 2011, November 25, 6 31 21.3 Geocentric coordinates of the Sun h m s s h Right ascension . . . . . . . 16 02 20.74+10.606( T- 7 ) ° ' " " h Declination . . . . . . . . . -20 41 15.9 -29.64 ( T- 7 ) " Equatorial horizontal parallax 8.91 ' " Apparent semidiameter . . . . 16 12.06 Geocentric coordinates of the Moon h m s s h s h 2 Right ascension . . . . . . . 16 03 32.08+160.045(T- 7 )+0.029(T- 7 ) ° ' " " h " h 2 Declination . . . . . . . . . -21 47 02.0 -233.45 (T- 7 )+4.88 (T- 7 ) ° ' " " h " h 2 Equatorial horizontal parallax 1 00 42.07- 0.981(T- 7 )-0.015(T- 7 ) ' " " h " h 2 Apparent semidiameter . . . . 16 32.44- 0.268(T- 7 )-0.004(T- 7 ) T - universal time in hours (TDT-UT1= 67.0s) General Circumstances of the Eclipse ------------------------------------------------------------------------------ Phenomena ¦ Universal ¦ Latitude ¦ Longitude ¦ Time ¦ ¦ ------------------------------+----------------+------------+----------------- ¦ h m ¦ ° ' ¦ ° ' Eclipse begins . . . . . . . ¦ 4 23.2 ¦ -34 35.8 ¦ 5 27.0 E Greatest eclipse . . . 0.906¦ 6 20.3 ¦ -68 18.8 ¦ 82 43.0 W Eclipse ends . . . . . . . . ¦ 8 17.3 ¦ -44 47.1 ¦ 164 50.2 E Besselian Elements ------------------------------------------------------------------------------ Universal¦ x ¦ y ¦ sin d ¦ cos d ¦ u ¦ u ¦ m Time ¦ ¦ ¦ ¦ ¦ e ¦ i ¦ --------+---------+---------+---------+---------+---------+---------+--------- h m ¦ ¦ ¦ ¦ ¦ ¦ ¦ ° ' 4 20 ¦-1.25416 ¦-0.93170 ¦-0.35288 ¦+0.93567 ¦+0.54045 ¦-0.00590 ¦ 248 18.1 30 ¦-1.15870 ¦-0.94145 ¦-0.35290 ¦+0.93566 ¦+0.54047 ¦-0.00588 ¦ 250 48.1 40 ¦-1.06323 ¦-0.95120 ¦-0.35292 ¦+0.93565 ¦+0.54049 ¦-0.00586 ¦ 253 18.0 50 ¦-0.96776 ¦-0.96093 ¦-0.35294 ¦+0.93564 ¦+0.54051 ¦-0.00584 ¦ 255 48.0 ¦ ¦ ¦ ¦ ¦ ¦ ¦ 5 00 ¦-0.87229 ¦-0.97065 ¦-0.35297 ¦+0.93564 ¦+0.54053 ¦-0.00583 ¦ 258 18.0 10 ¦-0.77682 ¦-0.98036 ¦-0.35299 ¦+0.93563 ¦+0.54055 ¦-0.00581 ¦ 260 48.0 20 ¦-0.68134 ¦-0.99006 ¦-0.35301 ¦+0.93562 ¦+0.54056 ¦-0.00579 ¦ 263 18.0 30 ¦-0.58586 ¦-0.99974 ¦-0.35303 ¦+0.93561 ¦+0.54058 ¦-0.00578 ¦ 265 48.0 40 ¦-0.49038 ¦-1.00942 ¦-0.35305 ¦+0.93560 ¦+0.54060 ¦-0.00576 ¦ 268 17.9 50 ¦-0.39490 ¦-1.01908 ¦-0.35308 ¦+0.93559 ¦+0.54061 ¦-0.00575 ¦ 270 47.9 ¦ ¦ ¦ ¦ ¦ ¦ ¦ 6 00 ¦-0.29941 ¦-1.02873 ¦-0.35310 ¦+0.93559 ¦+0.54063 ¦-0.00573 ¦ 273 17.9 10 ¦-0.20393 ¦-1.03837 ¦-0.35312 ¦+0.93558 ¦+0.54064 ¦-0.00572 ¦ 275 47.9 20 ¦-0.10844 ¦-1.04800 ¦-0.35314 ¦+0.93557 ¦+0.54065 ¦-0.00571 ¦ 278 17.9 30 ¦-0.01296 ¦-1.05762 ¦-0.35316 ¦+0.93556 ¦+0.54066 ¦-0.00569 ¦ 280 47.9 40 ¦+0.08253 ¦-1.06722 ¦-0.35319 ¦+0.93555 ¦+0.54067 ¦-0.00568 ¦ 283 17.8 50 ¦+0.17802 ¦-1.07681 ¦-0.35321 ¦+0.93554 ¦+0.54068 ¦-0.00567 ¦ 285 47.8 ¦ ¦ ¦ ¦ ¦ ¦ ¦ 7 00 ¦+0.27350 ¦-1.08639 ¦-0.35323 ¦+0.93554 ¦+0.54069 ¦-0.00566 ¦ 288 17.8 10 ¦+0.36899 ¦-1.09596 ¦-0.35325 ¦+0.93553 ¦+0.54070 ¦-0.00565 ¦ 290 47.8 20 ¦+0.46448 ¦-1.10552 ¦-0.35327 ¦+0.93552 ¦+0.54071 ¦-0.00565 ¦ 293 17.8 30 ¦+0.55996 ¦-1.11507 ¦-0.35330 ¦+0.93551 ¦+0.54072 ¦-0.00564 ¦ 295 47.8 40 ¦+0.65544 ¦-1.12460 ¦-0.35332 ¦+0.93550 ¦+0.54073 ¦-0.00563 ¦ 298 17.8 50 ¦+0.75093 ¦-1.13412 ¦-0.35334 ¦+0.93549 ¦+0.54073 ¦-0.00563 ¦ 300 47.7 ¦ ¦ ¦ ¦ ¦ ¦ ¦ 8 00 ¦+0.84641 ¦-1.14363 ¦-0.35336 ¦+0.93549 ¦+0.54074 ¦-0.00562 ¦ 303 17.7 10 ¦+0.94188 ¦-1.15313 ¦-0.35338 ¦+0.93548 ¦+0.54074 ¦-0.00562 ¦ 305 47.7 20 ¦+1.03736 ¦-1.16261 ¦-0.35341 ¦+0.93547 ¦+0.54075 ¦-0.00561 ¦ 308 17.7 ---------------------------------------------------------------- Univers.¦ x' ¦ y' ¦Univers.¦ x' ¦ y' tgf =0.0047361 Time ¦ ¦ ¦ Time ¦ ¦ e --------+-----------+-----------+--------+-----------+----------tgf =0.0047125 h ¦ ¦ ¦ h ¦ ¦ i 4 ¦ +0.009545 ¦ -0.000978 ¦ 7 ¦ +0.009549 ¦ -0.000957 m'=0.0043629 5 ¦ +0.009547 ¦ -0.000972 ¦ 8 ¦ +0.009548 ¦ -0.000950 6 ¦ +0.009548 ¦ -0.000965 ¦ 9 ¦ +0.009546 ¦ -0.000943