39 



in the interior. The surface is now rough but appears to have 

 been originally smooth. An average specimen of the ellip- 

 soids, which is the prevailing form, measures 0,292 mm. and 

 0,247 mm. in the longer and shorter diameters respectively. 

 I have not noticed any trace of depression or hilum in any 

 of these bodies, which are abundant. 



There can scarcely be any doubt that these small ellip 

 soids belong to the dermal crust of a sponge similar to Geodia. 

 The beautiful radiate arrangement of the siliceous balls of 

 the recent sponges has however, through the alteration of 

 the silica, quite disappeared in these examples, but I have 

 had the opportunity of comparing them with similarly shaped 

 spicules from the Upper Chalk of Coesfeld in which the ra- 

 diate structure is still preserved equally as perfect as in those 

 of existing sponges. In the Coesfeld examples I have noticed 

 a small cavity in the cental portion of the spicule, into 

 which the radiate structure does not extend, and to the en- 

 largement of this originally small cavity may be attributed 

 the irregularly shaped interior hollows of the Horstead spe- 

 cimens. This is further confirmed by finding in one of the 

 Coesfeld examples, an abnormally enlarged central portion, 

 while the exterior portion of the spicule yet retains the ra- 

 diate structure. 



Excellent illustrations of the radiate structure of these 

 bodies in the existing sponge Geodia Me Andrcwii , Bower- 

 bank are given by Dr. Bowerbank (Mon. Brit. Spong. Vol. I, 

 PL XXIII, XXIV, figs. 326 335. Similar siliceous globules 

 are described by Mr. Carter from the Haldon Green Sand 

 (An. Mag. Nat. Hist. Vol. VII, PL IX, figs. 55. 56); by Prof. 

 Zittel from Coesfeld (Ueber Coelop. Taf. V, figs. 1820); 

 and also by Rutot from the Eocene Sand of Brussels (op. 

 cit. PI. Ill, figs. 36, 37). 



The second form of these siliceous bodies (fig. 26), which 

 Mr. Carter has termed globo-stellate consists of a minute 

 spherical body whose surface is thickly studded with very 



