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.
Julian Day | Date Greg. | ![]() |
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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 |
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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:
Copyright ESO 2002