REPORT OF TEE CEIEF ASTRONOMER 159 



SESSIONAL PAPER No. 25a 



The Lone Star schists were traversed during bad weather at the close of 

 the season of 1902, when, as yet, the existence of the Summit series monocline 

 just described was unsuspected. No later opportunity was afforded for revisit- 

 ing 1 the few sections in which the schists are exposed in the belt. For these 

 reasons the collection of specimens and of field data is especially meagre for 

 the formation. The foregoing brief and very general account is all that is 

 warranted from the writer's limited knowledge of these rocks. 



