OCCULTATION OF IRIS 26 NOVEMBER 2010
Conditions of visibility and various information, data elaborated with WinOccult (C)
Moon: % illumination 70-, solar elongation 114°
Disappearance
U.T. Sun Moon CA PA WA a b
Location h m s Alt Alt Az o o o m/o m/o
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Reappearance
U.T. Sun Moon CA PA WA a b
Location h m s Alt Alt Az o o o m/o m/o
AF Herat 17 56 8 27 159 36S 130 127 +1.9 -0.7
AF Jalalabad 18 13 40 30 172 39S 127 124 +2.4 -0.9
AF Kabul 18 10 27 29 170 39S 127 124 +2.3 -0.8
AF Kandahar 18 6 2 31 165 31S 136 133 +2.2 -1.3
AF Kunduz 18 8 27 27 169 44S 123 119 +2.2 -0.6
AF Maimama 18 0 7 26 163 41S 125 122 +2.0 -0.5
AF Mazar-I-Sharif 18 4 47 26 166 44S 123 119 +2.1 -0.5
AF Sheberghan 18 2 6 26 165 43S 123 120 +2.0 -0.4
AF Shindand 17 56 42 28 159 34S 132 129 +1.9 -0.8
AF Taluqan 18 9 39 27 170 44S 122 119 +2.2 -0.6
CN Hotan 18 34 21 27 187 42S 125 121 +2.6 -1.2
CN Kashi 18 22 48 25 180 49S 118 114 +2.3 -0.6
IN Amritsar 18 28 18 33 180 31S 136 133 +2.8 -1.8
IN Jammu 18 26 43 32 180 34S 133 130 +2.7 -1.6
IN Kulu 18 34 47 32 184 30S 137 133 +3.0 -2.1
IN Leh 18 31 49 30 184 37S 130 127 +2.7 -1.5
IN Pathankot 18 29 39 32 181 32S 135 131 +2.8 -1.8
IN Srinagar 18 24 43 30 179 37S 129 126 +2.6 -1.3
IR Bojnord 17 46 23 22 153 40S 126 123 +1.5 -0.2
IR Sarakhs 17 52 54 24 158 41S 126 123 +1.8 -0.3
KZ Alma-Ata 18 23 1 21 181 54S 112 109 +2.1 -0.4
PK Bannu 18 15 13 31 172 35S 131 128 +2.5 -1.2
PK Chitral 18 15 31 28 174 42S 124 121 +2.4 -0.8
PK Dera Ismail Khan 18 17 29 32 173 32S 134 131 +2.5 -1.5
PK Faisalabad 18 23 56 33 177 30S 136 133 +2.7 -1.8
PK Gilgit 18 21 36 28 178 42S 124 121 +2.5 -0.9
PK Islamabad 18 20 55 31 176 37S 130 126 +2.6 -1.2
PK Lahore 18 27 32 33 179 30S 136 133 +2.8 -1.9
PK Lahore 18 27 26 33 179 30S 136 133 +2.8 -1.9
PK Mangla 18 22 59 31 177 35S 131 128 +2.6 -1.4
PK Mianwali 18 18 19 32 174 34S 132 129 +2.5 -1.3
PK Miranshah 18 14 2 31 171 36S 131 128 +2.4 -1.2
PK Muzaffarabad 18 21 5 30 177 38S 128 125 +2.5 -1.1
PK Parachinar 18 13 2 30 171 38S 129 125 +2.4 -1.0
PK Peshawar 18 16 31 30 174 38S 129 125 +2.4 -1.1
PK Qasim 18 20 49 31 176 37S 130 127 +2.6 -1.2
PK Rawala Kot 18 22 22 30 177 37S 129 126 +2.6 -1.2
PK Risalpur 18 17 33 30 174 38S 128 125 +2.5 -1.1
PK Sahiwal 18 21 10 32 176 32S 134 131 +2.6 -1.6
PK Saidu Sharif 18 17 43 29 175 40S 127 123 +2.4 -1.0
PK Sargodha 18 21 51 32 176 33S 134 131 +2.6 -1.5
PK Skardu 18 25 4 29 180 40S 126 123 +2.5 -1.1
PK Terbela 18 19 15 30 175 38S 129 125 +2.5 -1.1
PK Wana 18 13 35 31 171 34S 133 129 +2.4 -1.3
PK Zhob 18 14 36 32 171 31S 135 132 +2.5 -1.5
RU Ashkhabad 17 48 6 22 154 42S 124 121 +1.6 -0.1
RU Bishkek 18 17 51 21 177 54S 112 108 +2.0 -0.3
RU Bukhara 17 58 37 23 163 48S 118 114 +1.9 -0.1
RU Chardzhou 17 57 5 23 161 47S 119 116 +1.9 -0.1
RU Chimkent 18 8 0 21 170 54S 112 109 +2.0 -0.1
RU Dushanbe 18 7 29 25 169 47S 119 116 +2.1 -0.4
RU Osh 18 15 11 24 175 51S 115 112 +2.1 -0.4
RU Samarkand 18 3 24 23 166 49S 117 114 +2.0 -0.2
RU Termez 18 4 47 26 167 45S 122 118 +2.1 -0.4
UZ Tashkent 18 7 46 22 170 52S 114 111 +2.0 -0.2
Times in U.T.
Sun Alt the altitude of the sun. The field is blank if the sun is lower than -12 deg. (Nautical twilight)
Moon Alt the altitude of the moon
Moon Az the azimuth of the moon
CA Cusp Angle - the angle of the event around the limb of the moon, measured from the nearest cusp. -'ve values indicate a bright limb event. The cusps are usually N (north) or S (south), but near full moon can be E (East) or W (west).
If a lunar eclipse is in progress, CA gives is the % distance from the centre of the umbra, and is followed by a 'U'. Values up to 103% are possible. Where an event occurs more than 103% of the umbral radius, the usual Cusp Angle value is displayed.
PA Position Angle - the angle of the event around the limb of the moon, measured from true north
VA Vertex Angle - the angle of the event around the limb of the moon measured anticlockwise from the vertex of the lunar limb - i.e. the point on the limb highest from the horizon
A coefficient for correcting the prediction for changes in site location. The units are minutes of time per degree (or seconds of time per minute of arc). The correction to the prediction for a change in site, in seconds of time, is found by multiplying A by the change in site longitude (+'ve for changes towards the East) from the prediction site.
B same as for A, but for changes in latitude (+'ve to the north).
Data generated with software WinOccult (C)
