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Besselian elements

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17: 99:. This is the geocentric, normal plane of the shadow axis. In other words, it is the plane through the Earth's center that is perpendicular to the line through the centers of the occulting and the occulted bodies. One advantage, among others, of choosing this plane is that the outline of the shadow on it is always a circle, and there is no 94:
The basic concept is that Besselian elements describe the movement of the shadow cast by the occulting body – for solar eclipses this is the shadow of the Moon – on a specifically chosen plane, called the
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on the Earth's surface, and hence the circumstances of the eclipse at a specific location. This method was developed in the 1820s by the German mathematician and astronomer,
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Comparatively few values are needed to accurately describe the movement of the shadow on the fundamental plane. Based on this, the next step is to
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measures how much that rotation has slowed over time and must also be taken into account when predicting local eclipse circumstances.
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on the Earth's surface will experience an eclipse are determined by the Earth's rotation. A variable called
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a similar method is used, in which the shadow is cast on the Moon instead of the Earth.
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Although the Besselian elements determine the overall geometry of an eclipse, which
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For solar eclipses, the Besselian elements are used to calculate the path of the
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are a set of values used to calculate and predict the local circumstances of
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the shadow cone on to the Earth's surface, taking into account the
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for an observer on Earth. This method is particularly used for
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Seidelmann, P. Kenneth; Urban, Sean E., eds. (2013).
164:Explanatory Supplement to the Astronomical Almanac 228:A manual of spherical and practical astronomy. 8: 231:J. B. Lippincott & Co, Philadelphia 1863 215:Cambridge University Press, Cambridge 1985, 166:(3rd ed.). University Science Books. 48:, but is also applied for occultations of 196:Canon of solar eclipses: -2003 to +2526 149: 7: 14: 1: 271: 28:on Earth's surface and in 87:, and later improved by 198:. Astronomisches Büro. 101:perspective distortion 33: 118:, and the observer's 24:(green) during total 19: 213:Spherical astronomy. 255:Celestial mechanics 225:William Chauvenet: 112:figure of the Earth 72:. In addition, for 81:umbra and penumbra 38:Besselian elements 34: 22:umbra and penumbra 173:978-1-891389-85-6 97:fundamental plane 89:William Chauvenet 30:fundamental plane 262: 211:Robin M. Green: 200: 199: 184: 178: 177: 159: 85:Friedrich Bessel 270: 269: 265: 264: 263: 261: 260: 259: 235: 234: 208: 206:Further reading 203: 186: 185: 181: 174: 161: 160: 151: 147: 12: 11: 5: 268: 266: 258: 257: 252: 250:Solar eclipses 247: 237: 236: 233: 232: 223: 207: 204: 202: 201: 188:Mucke, Hermann 179: 172: 148: 146: 143: 74:lunar eclipses 46:solar eclipses 13: 10: 9: 6: 4: 3: 2: 267: 256: 253: 251: 248: 246: 243: 242: 240: 230: 229: 224: 222: 221:0-521-23988-5 218: 214: 210: 209: 205: 197: 193: 189: 183: 180: 175: 169: 165: 158: 156: 154: 150: 144: 142: 140: 136: 131: 129: 125: 121: 117: 113: 109: 104: 102: 98: 92: 90: 86: 82: 77: 75: 71: 67: 63: 59: 55: 51: 47: 43: 39: 31: 27: 26:solar eclipse 23: 18: 226: 212: 195: 182: 163: 134: 132: 105: 96: 93: 78: 42:occultations 37: 35: 192:Meeus, Jean 20:Outline of 239:Categories 145:References 135:longitudes 128:elevation 124:longitude 245:Eclipses 194:(1992). 120:latitude 116:rotation 62:transits 108:project 70:Mercury 56:by the 54:planets 219:  170:  114:, its 66:Venus 50:stars 32:(red) 217:ISBN 168:ISBN 126:and 60:and 58:Moon 36:The 68:or 64:of 52:or 241:: 190:; 152:^ 139:ΔT 130:. 122:, 103:. 91:. 176:.

Index


umbra and penumbra
solar eclipse
fundamental plane
occultations
solar eclipses
stars
planets
Moon
transits
Venus
Mercury
lunar eclipses
umbra and penumbra
Friedrich Bessel
William Chauvenet
perspective distortion
project
figure of the Earth
rotation
latitude
longitude
elevation
ΔT



ISBN
978-1-891389-85-6
Mucke, Hermann

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