558 ADDITIONS. 



the Planets from the Sun ; nor does any theory yet devised give such 

 reason. But an empirical formula proposed by the Astronomer Bode 

 of Berlin, gives a law of these distances (Socle's Laiv), which, to make 

 it coherent, requires a planet between Mars and Jupiter. With such 

 an addition, the distance of Mercury, Venus, Earth, Mars, the Missing 

 Planet, Jupiter, Saturn, and Uranus, are nearly as the numbers 



4, 7, 10, 16, 28, 52, 100, 196, 



in which the excesses of each number above the preceding are the 

 series 



3, 3, 6, 12, 24, 48, 96. 



On the strength of this law the Germans wrote on the long -expected 

 Planet, and formed themselves into associations for the discovery of it. 



Not only did this law stimulate the inquiries for the Missing Planet, 

 and thus lead to the discovery of the Minor Planets, but it had also a 

 share in the discovery of Neptune. According to the law, a planet 

 beyond Uranus may be expected to be at the distance represented by 

 388. Mr. Adams and M. Le Yerrier both of them began by assuming 

 a distance of nearly this magnitude for the Planet which they sought ; 

 that is, a distance more than 38 times the earth's distance. It was 

 found afterwards that the distance of Neptune is only 30 time* that oi 

 the earth; yet the assumption was of essential use in obtaining the 

 result : and Mr. Airy remarks that the history of the discovery shows 

 the importance of using any received theory as far as it will go, even 

 if the theory can claim no higher merit than that of being plausible. 4 



The discovery of Minor Planets in a certain region of the interval 

 between Mars and Jupiter has gone on to such an extent, that their 

 number makes them assume in a peculiar manner the character of 

 representatives of a Missing Planet. At first, as I have said in the 

 text, it was supposed that all these portions must pass through or near 

 a common node ; this opinion being founded on the very bold doctrine, 

 that the portions must at one time have been united in one Planet, and 

 must then have separated. At this node, as I have stated, Olbers lay 

 in wait for them, as for a hostile army at a defile. Ceres, Pallas, and 

 Juno had been discovered in this way in the period from 1801 to 

 1804 ; and Vesta was caught in 1807. For a time the chase for new 

 planets in this region seemed to have exhausted the stock. But after 

 thirty-eight years, to the astonishment of astronomers, they began to 

 be again detected in extraordinary numbers. In 1845, M. Hencke of 



Account of the Di?co"ery cf Neptune, &c., Mem. Ast. Soc., vol. xvi. p. 4H. 



