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3 The predictions

We computed eclipses of J5 Amalthea by the Galileans moons from November 2002 to June 2003, since these events could give access to the best signal/noise ratio that geometric circumstances would allow, for an apparent distance of the eclipsing satellite which was large enough to measure photometric variation of Amalthea alone. The signal to detect during occultations, when both satellites are measured, is too faint. We iteratively calculated the first and last contacts of the eclipsed satellite with the umbra cone (when an eclipse is detected) and its minimum distance to the axis of this cone. The relative positions of the cone and the satellites are calculated by taking into account the aberration effects and the date of prediction includes the light-time delay.

   
Table 1: Mutual events between Amalthea and Io during the 2002-2003 period.

Julian Day
Date Greg. $\Delta X~$a $\Delta Y~$b $\Delta_{\rm Io}$    $\Delta_{\rm J}$    $\rho$     ${\rm d}t$     ${\rm d}m$    ${\rm d}p$   
UT UT arcsec arcsec arcsec arcsec arcsec second arcsec arcsec

2452595.672984954
2002/11/17 04:09:05.89 -18.494 6.756 19.68 48.94 18.99 0. 0.76 0.57
2452627.498471065 2002/12/18 23:57:47.90 -10.767 3.678 11.37 36.45 20.85 1450. 0.40 0.55
2452630.844881944 2002/12/22 08:16:37.79 -10.952 3.914 11.63 46.93 21.03 487. 0.54 0.55
2452631.060819444 2002/12/22 13:27:34.79 -16.678 6.130 17.76 54.20 21.04 0. 0.81 0.58
2452646.991589121 2003/01/07 11:47:53.30 -10.754 4.110 11.51 56.41 21.77 0. 0.80 0.57
2452655.634476852 2003/01/16 03:13:38.79 -10.602 3.870 11.28 35.09 22.05 0. 0.81 0.60
2452687.507636574 2003/02/17 00:10:59.80 8.383 -2.678 8.80 32.50 22.09 113. 0.19 0.61
2452691.019006944 2003/02/20 12:27:22.19 9.608 -3.100 10.09 45.17 21.99 136. 0.07 0.60
2452694.535236111 2003/02/24 00:50:44.39 10.044 -3.195 10.54 54.47 21.88 181. 0.02 0.58
2452698.070984954 2003/02/27 13:42:13.09 9.063 -2.700 9.45 53.46 21.76 465. 0.10 0.56
2452698.314288194 2003/02/27 19:32:34.49 10.902 -2.873 11.27 54.63 21.75 152. 0.40 0.57
2452701.834429398 2003/03/03 08:01:34.70 14.239 -4.023 14.79 43.92 21.60 134. 0.25 0.59
2452706.955986111 2003/03/08 10:56:37.19 17.460 -5.213 18.22 42.34 21.37 131. 0.01 0.60
2452710.470355324 2003/03/11 23:17:18.69 16.782 -4.880 17.47 51.50 21.20 163. 0.03 0.59
2452713.995875000 2003/03/15 11:54:03.60 14.672 -4.056 15.22 54.03 21.02 272. 0.15 0.57
2452714.245583334 2003/03/15 17:53:38.40 14.709 -4.107 15.27 54.10 21.01 272. 0.10 0.57
2452717.770649306 2003/03/19 06:29:44.09 18.841 -5.448 19.61 44.39 20.81 161. 0.06 0.59
2452722.893640046 2003/03/24 09:26:50.50 23.133 -6.541 24.04 38.82 20.53 126. 0.01 0.60
2452726.406620370 2003/03/27 21:45:31.99 21.646 -5.966 22.45 47.86 20.32 149. 0.08 0.59
2452729.927077546 2003/03/31 10:14:59.49 18.836 -5.015 19.49 52.08 20.11 208. 0.19 0.57
2452730.171966435 2003/03/31 16:07:37.90 15.725 -4.523 16.36 52.15 20.10 419. 0.14 0.56
2452737.222520833 2003/04/07 17:20:25.80 24.083 -6.968 25.07 32.45 19.68 116. 0.31 0.60
2452738.831780093 2003/04/09 07:57:45.80 26.264 -7.211 27.23 34.83 19.58 122. 0.01 0.61
2452742.343684028 2003/04/12 20:14:54.30 24.301 -6.563 25.17 43.84 19.37 139. 0.09 0.59
2452745.860995370 2003/04/16 08:39:50.00 21.179 -5.635 21.91 49.17 19.16 182. 0.15 0.58
2452749.406243056 2003/04/19 21:44:59.40 15.543 -4.125 16.08 40.68 18.95 841. 0.12 0.55
2452749.641084491 2003/04/20 03:23:09.70 20.300 -5.963 21.15 45.08 18.93 149. 0.38 0.58
2452753.159864584 2003/04/23 15:50:12.30 23.741 -6.859 24.71 33.83 18.73 117. 0.34 0.59
2452754.770166667 2003/04/25 06:29:02.40 27.027 -7.419 28.02 30.57 18.63 118. 0.00 0.61
2452758.281230324 2003/04/28 18:44:58.29 24.877 -6.813 25.79 39.62 18.43 134. 0.02 0.60
2452761.796299769 2003/05/02 07:06:40.30 21.722 -5.980 22.53 45.80 18.24 169. 0.02 0.58
2452765.324815972 2003/05/05 19:47:44.10 17.157 -4.839 17.82 45.21 18.05 323. 0.08 0.56
2452765.574181713 2003/05/06 01:46:49.30 18.321 -5.445 19.11 45.16 18.03 180. 0.38 0.57
2452769.096738426 2003/05/09 14:19:18.20 21.723 -6.323 22.62 35.37 17.85 133. 0.29 0.59
2452774.219069445 2003/05/14 17:15:27.60 23.718 -6.807 24.67 35.32 17.58 122. 0.17 0.60
2452777.732592592 2003/05/18 05:34:55.99 20.792 -6.106 21.67 42.21 17.41 138. 0.25 0.59
2452781.254724537 2003/05/21 18:06:48.19 16.874 -5.155 17.64 44.70 17.24 176. 0.38 0.57
2452781.503969907 2003/05/22 00:05:42.99 15.302 -4.628 15.98 44.58 17.23 276. 0.31 0.56
2452785.033035879 2003/05/25 12:47:34.29 18.682 -5.549 19.48 36.93 17.07 153. 0.25 0.58
2452790.157081019 2003/05/30 15:46:11.80 21.271 -6.580 22.26 30.99 16.85 72. 0.48 0.60
2452793.669351852 2003/06/03 04:03:52.00 18.646 -5.974 19.57 38.47 16.70 0. 0.60 0.59
2452797.187765046 2003/06/06 16:30:22.90 15.360 -5.149 16.20 42.83 16.56 0. 0.70 0.57
2452797.385594907 2003/06/06 21:15:15.39 9.919 -3.204 10.42 31.37 16.56 836. 0.33 0.54
2452800.968388889 2003/06/10 11:14:28.80 15.077 -4.654 15.77 38.40 16.42 170. 0.25 0.58
2452804.485777778 2003/06/13 23:39:31.19 16.651 -5.267 17.46 29.05 16.30 106. 0.38 0.59
a
$\Delta X = \Delta \alpha \cos(\delta)$ is Differential coordinate of Amalthea relative to Io.
b
$\Delta Y = \Delta \delta$ is Differential coordinate of Amalthea relative to Io.

A large set of predictions has been obtained and will be made available on the web server that we have set up, dedicated to the international campaign PHEMU03 for the observation of the Galilean satellites' mutual events (http://www.bdl.fr/Phemu03/phemu03_eng.html).

In this paper we only give a selection of the most interesting phenomena, i.e. only the eclipses of J5 Amalthea by J1 Io, when elongation to Jupiter is large enough.

This is why these predictions are given from November 17, 2002 to June 13, 2003, when the elongation of Jupiter to the Sun is greater than 50 degrees. During this period, all events are observable all around the world depending on the date of the event and the local circumstances of elevation above the horizon.

We give in Table 1:

According to the accuracy of our model and considering a mean radius of J5 Amalthea (120 km) instead of a triaxial model (125 km, 73 km, 64 km) (Thomas 1998), we include in this table only the phenomena or the grazing phenomena with ${\rm d}m-{\rm d}p$ smaller than 0.23 arcsec.


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