FREE BOOKS

Author's List




PREV.   NEXT  
|<   442   443   444   445   446   447   448   449   450   451   452   453   454   455   456   457   458   459   460   461   462   463   464   465   466  
467   468   469   470   471   472   473   474   475   476   477   478   479   480   481   482   483   484   485   486   487   488   489   490   491   >>   >|  
wards in all directions from the axis of the cone of Vesuvius, are intersected by veins or dikes of compact lava, for the most part in a vertical position. In 1828 these were seen to be about seven in number, some of them not less than four or five hundred feet in height, and thinning out before they reached the uppermost part of the cone. Being harder than the beds through which they pass, they have decomposed less rapidly, and therefore stand out in relief. When I visited Vesuvius, in November, 1828, I was prevented from descending into the crater by the constant ejections then thrown out; so that I got sight of three only of the dikes; but Signor Monticelli had previously had drawings made of the whole, which he showed me. The dikes which I saw were on that side of the cone which is encircled by Somma. The eruption before mentioned, of 1828, began in March, and in the November following the ejected matter had filled up nearly one-third of the deep abyss formed at the close of the eruption of 1822. In November I found a single black cone at the bottom of the crater continually throwing out scoriae, while on the exterior of the cone I observed the lava of 1822, which had flowed out six years before, not yet cool, and still evolving much heat and vapor from crevices. Hoffmann, in 1832, saw on the north side of Vesuvius, near the peak called Palo, a great many parallel bands of lava, some from six to eight feet thick, alternating with scoriae and conglomerate. These beds, he says, were cut through by many dikes, some of them five feet broad. They resemble those of Somma, the stone being composed of grains of leucite and augite.[528] There can be no doubt that the dikes above mentioned have been produced by the filling up of open fissures with liquid lava; but of the date of their formation we know nothing farther than that they are all subsequent to the year 79, and, relatively speaking, that they are more modern than all the lavas and scoriae which they intersect. A considerable number of the upper strata are not traversed by them. That the earthquakes, which almost invariably precede eruptions, occasion rents in the mass, is well known; and, in 1822, three months before the lava flowed out, open fissures, evolving hot vapors, were numerous. It is clear that such rents must be ejected with melted matter when the column of lava rises, so that the origin of the dikes is easily explained, as also the great solidity and
PREV.   NEXT  
|<   442   443   444   445   446   447   448   449   450   451   452   453   454   455   456   457   458   459   460   461   462   463   464   465   466  
467   468   469   470   471   472   473   474   475   476   477   478   479   480   481   482   483   484   485   486   487   488   489   490   491   >>   >|  



Top keywords:

November

 

Vesuvius

 

scoriae

 
fissures
 

flowed

 
evolving
 

matter

 
eruption
 

mentioned

 
ejected

crater

 
number
 
augite
 
filling
 

melted

 
grains
 

leucite

 

column

 

composed

 
produced

alternating

 

conglomerate

 
solidity
 

parallel

 

explained

 

resemble

 

origin

 

easily

 

intersect

 

modern


speaking

 

considerable

 

invariably

 
precede
 

eruptions

 

earthquakes

 
strata
 

traversed

 
numerous
 

vapors


liquid

 
occasion
 

formation

 
subsequent
 

months

 

farther

 
relief
 

visited

 

rapidly

 

harder