Beer and Maedler also measured the heights of one thousand and ninety-five lunar mountains and crater-summits: the resulting measures are given in a table contained in the comprehensive text-book which accompanies their map. These heights are found by one of two methods, either by measuring the length of the shadow which the object casts under a known elevation of the sun above its horizon, or by measuring the distance between the illuminated point of the mountain and the “terminator” in the following manner. In the annexed figure ([Fig. 15]) let the circle represent the moon and M a mountain upon it: let S A be the line of direction of the sun’s rays, passing the normal surface of the moon at A and just tipping the mountain top. A will be the terminator, and there will be darkness between it and the star-like mountain summit M. The distance between A and M is measured: the distance A B is known, for it is the moon’s radius. And since the line S M is a tangent to the circle the angle B A M is a right angle. We know the length of its two sides AB, AM, and we can therefore by the known properties of the right-angled triangle find the length of the hypothenuse BM: and since BM is made up of the radius BA plus the mountain height, we have only to subtract the moon’s radius from the ascertained whole length of the hypothenuse and we have the height of the mountain. MM. Beer and Maedler exhibited their measures in French toises: in the heights we shall have occasion to quote, these have been turned into English feet, upon the assumption that the toise is equal to 6·39 English feet. The nomenclature of lunar features adopted by Beer and Maedler is that introduced by Riccioli: mountains and features hitherto undistinguished were named by them after ancient and modern philosophers, in continuance of Riccioli’s system, and occasionally after terrestrial features. Some minute objects in the neighbourhood of large and named ones were included under the name of the large one and distinguished by Greek or Roman letters.

Fig. 15.

PLATE IV.
PICTURE MAP OF THE MOON.

PLATE V.
Skeleton Map of Moon
To Accompany Picture Map, [Chap. VII]

The excellent map resulting from the arduous labours of these astronomers is simply a map: it does not pretend to be a picture. The asperities and depressions are symbolized by a conventional system of shading and no attempt is made to exhibit objects as they actually appear in the telescope. A casual observer comparing details on the map with the same details on the moon itself would fail to identify or recognize them except where the features are very conspicuous. Such an observer would be struck by the shadows by which the lunar objects reveal themselves: he would get to know them mostly by their shadows, since it is mainly by those that their forms are revealed to a terrestrial observer. But such a map as that under notice indicates no shadows, and objects have to be identified upon it rather by their positions with regard to one another or to the borders of the moon than by any notable features they actually present to view. This inconvenience occurred to us in our early use of Beer and Maedler’s chart, and we were induced to prepare for ourselves a map in which every object is shown somewhat, if imperfectly, as it actually appears at some period of a lunation. This was done by copying Beer and Maedler’s outlines and filling them up by appropriate shading. To do justice to our task we enlarged our map to a diameter of six feet. Upon a circle of this diameter the positions and dimensions of all objects were laid down from the German original. Then from our own observations we depicted the general aspect of each object: and we so adjusted the shading that all objects should be shown under about the same angle of illumination—a condition which is never fulfilled upon the moon itself, but which we consider ourselves justified in exhibiting for the purpose of conveying a fair impression of how the various lunar objects actually appear at some one or other part of a lunation.

The picture-map thus produced has been photographed to the size convenient for this work: and in order to make it available for the identification of such objects as we may have occasion to refer to, we have placed around it a co-ordinate scale of arbitrary divisions by which any object can be found as by the latitude and longitude divisions upon a common geographical map. We have also prepared a skeleton map which includes the more conspicuous objects, and which faces the picture map (Plates [IV.] and [V.]) The numbers on the skeleton map are those given in the second column of the accompanying table. The table also gives the co-ordinate positions of the various craters, the names of which are, for convenience of reference, printed in alphabetical order.

Name. Number. Map Ordinates.
Abulfeda 107 30·0 120·7
Agrippa 151 31·2 110·0
Airy 93 34·7 123·0
Albategnius 109 35·5 119·7
Aliacensis 61 35·8 131·0
Almanon 94 29·0 122·3
Alpetragius 92 40·8 122·4
Alphonsus 110 39·6 120·9
Apianus 62 33·6 129·3
Apollonius 154 6·5 109·5
Arago 152 24·7 108·7
Archimedes 191 40·3 95·8
Aristarchus 176 62·3 99·2
Aristillus 190 37·0 93·3
Aristotle 209 30·0 84·6
Arzachael 84 39·5 124·0
Atlas 228 20·7 86·6
Autolycus 189 36·8 95·5
Azophi 76 30·7 126·8
Bacon 17 32·5 142·0
Baily 207 26·0 85·4
Barocius 34 31·8 138·5
Bessel 179 27·4 100·1
Bettinus 11 48·8 144·9
Bianchini 215 51·6 86·3
Billy 121 64·3 121·4
Blancanus 12 43·7 144·8
Bonpland 110 48·5 117·6
Borda 56 15·2 131·0
Boscovich 160 31·1 106·8
Bouvard 40 66·6 134·3
Briggs 196 68·0 97·2
Bullialdus 86 50·1 125·5
Burg 206 25·5 87·5
Calippus 199 32·4 90·3
Campanus 71 52·3 129·0
Capella 104 17·8 118·0
Capuanus 43 50·5 132·8
Casatus 7 43·7 147·0
Cassini 200 35·5 89·7
Catherina 95 24·7 124·0
Cavalerius 144 71·2 109·5
Cavendish 88 63·5 127·4
Cichus 44 47·3 132·8
Clavius 13 41·8 143·5
Cleomides 183 10·7 97·0
Colombo 98 12·8 122·7
Condamine 214 48·7 84·2
Condorcet 164 4·5 104·7
Copernicus 147 49·8 107·0
Cyrillus 96 23·5 121·3
Damoiseau 124 69·2 117·2
Davy 113 43·2 119·8
Deambrel 129 26·8 113·5
Delisle 195 55·7 95·2
Descartes 106 28·5 119·3
Diophantus 194 55·5 96·3
Doppelmayer 70 58·6 129·6
Encke 140 59·7 110·6
Endymion 227 20·6 83·8
Epigenes 223 39·0 79·5
Erastothenes 168 44·6 104·0
Eudoxus 208 29·7 88·0
Fabricius 35 20·0 136·8
Fernelius 37 35·1 134·8
Firmicus 156 5·8 107·7
Flamsteed 126 62·8 114·5
Fontana 122 65·9 123·0
Fontenelle 221 43·0 81·3
Fourier 67 62·5 130·7
Fracastorius 78 20·5 127·0
Furnerius 52 11·7 133·0
Gambart 138 47·2 112·2
Gartner 224 26·5 82·3
Gassendi 90 59·7 123·3
Gauricus 46 43·5 132·5
Gauss 201 10·3 90·3
Gay Lussac 169 50·1 103·8
Geber 83 29·6 124·8
Geminus 187 13·0 93·0
Gérard 218 63·7 88·8
Goclenius 101 11·8 118·5
Godin 135 31·3 111·7
Grimaldi 125 70·8 116·3
Gruemberger 6 41·4 145·8
Gueriké 114 46·5 119·6
Guttemberg 102 13·9 118·3
Hainzel 39 52·3 136·7
Hansteen 123 65·5 119·9
Hase 54 9·8 129·5
Heinsius 88 45·5 136·0
Helicon 212 48·0 89·6
Hell 47 41·7 131·6
Hercules 229 22·3 86·7
Herodotus 175 63·2 99·6
Herschel 112 39·3 116·2
Hesiodus 64 45·8 130·0
Hevelius 141 71·5 111·3
Hippalus 87 54·0 127·0
Hommel 20 26·8 140·0
Hyginus 158 33·6 108·0
Inghirami 27 61·3 138·9
Isidorus 103 16·7 118·0
Kant 105 25·8 118·5
Kepler 146 60·0 108·0
Kies 72 49·7 128·8
Kircher 10 47·5 145·8
Klaproth 8 43·5 146·7
La Caille 74 37·5 126·8
Lagrange 68 67·0 131·3
La Hire 177 54·3 99·3
Lalande 117 43·4 115·3
Lambert 193 49·6 97·8
Landsberg 127 54·0 113·0
Langreen 100 6·3 117·7
Letronne 120 62·0 119·0
Licetus 21 34·1 139·6
Lichtenberg 197 66·5 94·9
Linnæus 188 31·7 95·7
Littrow 185 20·5 99·4
Lohrman 143 71·3 112·8
Longomontanus 23 45·7 140·6
Lubiniezky 91 51·3 123·5
Macrobius 182 13·7 100·2
Maginus 22 40·0 140·4
Mairan 217 56·7 89·5
Manilius 167 32·2 103·9
Manzinus 4 31·3 146·0
Maraldi 181 18·6 100·8
Marius 171 65·0 105·5
Maskelyne 132 19·5 111·0
Mason 204 23·7 88·8
Maupertius 213 48·7 85·8
Maurolycus 33 31·8 137·0
Menelaus 165 28·3 103·0
Mercator 65 51·4 130·2
Mersenius 89 61·7 125·7
Messala 202 14·0 90·5
Messier 131 10·8 114·0
Metius 36 18·8 105·9
Moretus 5 39·5 146·5
Moesting 128 41·6 113·2
Neander 57 18·7 131·0
Nearchus 18 26·8 142·0
Newton 1 41·0 147·7
Nonius 49 36·5 133·2
Olbers 172 73·0 107·7
Pallas 149 38·6 109·5
Parrot 108 35·8 121·6
Petavius 80 9·5 127·5
Phocylides 25 55·5 141·6
Piazzi 41 65·0 133·5
Picard 163 8·3 104·7
Piccolomini 58 21·7 131·0
Pico 211 41·9 87·3
Pitatus 63 44·1 130·2
Plana 205 24·8 88·8
Plato 210 41·8 84·8
Playfair 75 33·5 127·5
Pliny 165 24·2 103·4
Poisson 60 32·8 131·0
Polybius 82 24·5 125·6
Pontanus 59 29·0 130·2
Posidonius 186 22·2 94·3
Proclus 162 11·4 104·5
Ptolemy 111 39·5 118·2
Purbach 73 38·7 128·4
Pythagoras 220 53·0 81·2
Pytheas 178 49·7 100·4
Ramsden 42 52·9 132·5
Reamur 118 37·3 114·6
Reiner 145 67·3 108·5
Reinhold 139 51·5 111·2
Repsold 219 60·2 85·7
Rheita 51 16·1 134·2
Riccioli 142 72·7 113·8
Riccius 50 23·7 133·5
Ritter 134 26·0 111·6
Roemer 184 18·3 97·6
Ross 161 25·0 105·3
Sabine 133 25·0 112·0
Sacrobosco 77 27·5 127·7
Santbech 79 15·7 126·8
Saussure 31 39·6 137·7
Scheiner 14 45·5 143·5
Schickard 28 59·0 137·5
Schiller 24 51·3 141·0
Schroeter 137 42·3 110·7
Schubert 155 2·3 110·8
Segner 16 51·3 143·5
Seleucus 174 69·0 99·8
Sharp 216 54·2 87·7
Short 2 39·7 147·4
Silberschlag 157 32·0 108·1
Simpelius 3 35·8 147·7
Snell 55 11·3 129·6
Soemmering 136 42·8 112·2
Stadius 148 45·6 107·0
Stevinus 53 11·9 130·7
Stoefler 32 35·6 136·8
Strabo 226 23·2 81·6
Struve 203 18·3 88·7
Taruntius 153 11·7 109·0
Taylor 130 27·6 116·2
Thales 225 24·3 81·8
Thebit 85 40·8 126·8
Theophilus 97 22·3 120·0
Timæus 222 38·3 80·8
Timocharis 192 45·1 97·0
Tobias Mayer 170 54·5 103·0
Triesnecker 150 35·5 109·8
Tycho 30 43·0 142·3
Ukert 159 37·1 107·5
Vasco de Gama 173 72·8 104·9
Vendelinus 99 6·8 121·6
Vieta 69 64·3 129·7
Vitello 66 55·8 130·7
Vitruvius 180 20·1 102·0
Vlacq 19 25·0 140·1
Walter 48 37·8 131·9
Wargentin 26 57·5 140·2
Werner 62 36·4 129·3
Wilhelm Humboldt 81 5·7 127·8
Wilhelm I. 29 45·9 138·6
Wilson 9 45·7 146·4
Wurzelbauer 45 45·0 132·6
Zuchius 15 50·7 144·2