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Total lunar eclipse of 2007 March 3-4

The beginning of the eclipse visible in Europe, in Asia except the eastern
part, east of Greenland, Africa, Madagascar, western half of Australia, the
coast of Antarctica (on the part of Indian Ocean), the western Arctic Ocean,
the Indian and Atlantic Oceans.
The end of the eclipse visible in Europe, western Asia, Africa, Madagascar,
South America, the eastern part of Northern America, Greenland, Antarctica
(on the part of Atlantic Ocean), the western Indian and Atlantic Oceans, in
extreme south-east of Pacific Ocean.

Universal time of geocentric opposition
h m s
in right ascension 2007, March 3, 23 00 43.9

Sun Moon
h m s h m s
Right ascension . . . . . . . . . . . . . 22 57 16.046 10 57 16.046
s s
Hourly motion . . . . . . . . . . . . . +9.322 +107.747
я€ ' " я€ ' "
Declination. . . . . . . . . . . . . . . . -6 41 05.66 +7 00 44.81
" "
Hourly motion . . . . . . . . . . . . . +57.57 -845.84
" ' "
Equatorial horizontal parallax . . . . . . 8.87 54 31.30
' " ' "
Apparent semidiameter . . . . . . . . . . 16 07.97 14 51.42


Circumstances of the Eclipse
Position Angles
of the Moon's axis
h m я€
Moon enters penumbra . . . . . . . March 3, 20 16.4 20.82
Moon enters umbra . . . . . . . . 21 30.0 20.89
Moon enters totality . . . . . . . 22 44.0 20.95
Greatest eclipse . . . . . . . . . 23 20.9 20.98
Moon leaves totality . . . . . . . 23 58.2 21.01
Moon leaves umbra . . . . . . . . March 4, 1 11.9 21.07
Moon leaves penumbra . . . . . . . 2 25.5 21.13

--------------------------------------------
Contacts| Position |The Moon being in the Zenith in
of Umbra| Angles |-------------------------------
with Limb| from the | |
of Moon |North Point| Latitude | Longitude
---------|-----------|--------------|----------------
| я€ ' | я€ ' | я€ '
First | 136 51.3 | + 7 25.0 | 39 51.3 E
Last | 279 44.8 | + 6 32.5 | 14 06.6 W

Magnitude of the eclipse 1.235
"
Angular radius of the penumbra 4332.76
"
Angular radius of the umbra 2358.11

-------------------------------------------------------------------------------
| | | |Magnitudes of! | | | |Magnitudes of
T | s | d | P |-------------! T | s | d | P |-------------
| | | |umbral| penum. | | | |umbral| penum.
| | | eclipse|eclipse | | | eclipse|eclipse
-----|-----|------|------|------|------!-----|-----|------|------|------|------
h m| "| | я€ | | ! h m| "| | я€ | |
20 10| 5396| 2.286| 129.2| п” | п” !23 30| 1069| 0.453| 222.0| 1.220| 2.327
20| 5124| 2.171| 129.8| п” | 0.055! 40| 1166| 0.495| 235.4| 1.166| 2.274
30| 4853| 2.056| 130.5| п” | 0.207! 50| 1316| 0.558| 246.2| 1.084| 2.191
40| 4582| 1.941| 131.2| п” | 0.359! | | | | |
50| 4312| 1.827| 132.1| п” | 0.510! 0 00| 1502| 0.637| 254.6| 0.980| 2.087
| | | | | ! 10| 1713| 0.727| 261.0| 0.861| 1.969
21 00| 4043| 1.713| 133.0| п” | 0.661! 20| 1941| 0.823| 266.0| 0.734| 1.842
10| 3775| 1.600| 134.1| п” | 0.810! 30| 2180| 0.925| 269.9| 0.600| 1.707
20| 3509| 1.487| 135.4| п” | 0.959! 40| 2427| 1.030| 273.0| 0.461| 1.569
30| 3245| 1.375| 136.9| 0.000| 1.107! 50| 2680| 1.137| 275.6| 0.319| 1.427
40| 2984| 1.265| 138.6| 0.146| 1.254! | | | | |
50| 2725| 1.155| 140.6| 0.291| 1.398! 1 00| 2938| 1.246| 277.7| 0.174| 1.282
| | | | | ! 10| 3198| 1.357| 279.4| 0.028| 1.136
22 00| 2471| 1.047| 143.1| 0.433| 1.540! 20| 3461| 1.469| 280.9| п” | 0.988
10| 2222| 0.942| 146.1| 0.572| 1.680! 30| 3727| 1.581| 282.2| п” | 0.839
20| 1981| 0.840| 149.8| 0.707| 1.814! 40| 3993| 1.694| 283.3| п” | 0.689
30| 1751| 0.742| 154.6| 0.836| 1.943! 50| 4261| 1.808| 284.3| п” | 0.539
40| 1537| 0.652| 160.8| 0.955| 2.063! | | | | |
50| 1345| 0.570| 168.8| 1.062| 2.170! 2 00| 4530| 1.923| 285.2| п” | 0.388
| | | | | ! 10| 4800| 2.037| 285.9| п” | 0.236
23 00| 1189| 0.504| 179.2| 1.150| 2.257! 20| 5071| 2.152| 286.6| п” | 0.084
10| 1081| 0.458| 192.1| 1.210| 2.318! 30| 5342| 2.267| 287.2| п” | п”
20| 1039| 0.440| 207.0| 1.235| 2.343! | | | | |
s
T - universal time ( TT - UT1 = 66.0 );
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.