Proceedings of the California Academy of Sciences, Volume III, 1863-1867Various
Science
Proceedings of the California Academy of Sciences, Volume III, 1863-1867
Various
California Academy of Sciences -- Periodicals; Science -- Periodicals
The direction of the wave in this earthquake was north fifty
degrees west; the limited area over which it extended has not
furnished sufficient data to calculate its velocity.
This earthquake differs from all others that have occurred
in this locality in this particular: the earth continued to
vibrate with increasing and again decreasing degrees of force
for ten hours, at no time entirely ceasing during this period.
22 h. 1 m., another light shock, consisting of a single
vibration.
23 h. 50 m., another shock. After this shock the vibrations of
the earth ceased to be noticeable.
October 9th, 10 h. 34 m.—Another light shock.
11 h. 32 m., another shock. After this shock the earth
continued to vibrate at intervals till noon of the tenth.
OCTOBER 13th, 2 h. 5 m.—A smart shock at San Francisco; felt at
Oakland and Santa Clara; also at Angel Island.
OCTOBER 14th, 23 h. 45 m.—Another shock at San Francisco.
OCTOBER 15th, 3 h. 40 m.—Another shock at San Francisco.
NOVEMBER 24th, 3 h. 45 m.—A smart shock at Watsonville, Santa
Cruz Co.
DECEMBER 7th, 1 h. 15 m.—A light shock at San Francisco.
Professor Whitney presented the plate published by Mr. Haidinger, the
distinguished Chief of the Austrian Geological Survey, to exhibit the
structure of the Carleton meteoric iron. This plate, together with
an elaborate article describing the appearance and structure of this
meteorite, is published in the proceedings of the Vienna Academy of
Science, Vol. XLVIII, page 301.
Professor Whitney also made some remarks on the nature and distribution
of the meteorites which have, up to the present time, been discovered on
the Pacific Coast and in Mexico; of these remarks the following is an
abstract.
It is remarkable that no meteoric stones have ever been
discovered, either near the Pacific coast or, indeed, so far as
we know, anywhere on this side of the Rocky Mountains. Masses
of meteoric iron, on the other hand, are known to exist in
quite a number of localities, and many of these masses are of
very large size.
On page eleven, of the third volume of the Academy’s
Proceedings, I have given a list of the localities of meteoric
iron known in Arizona and Northern Mexico. This was done in
order to attract the attention of explorers and prospectors
to these remarkable masses, and in the hope of getting more
definite information in regard to some of them. Indeed, some
additional items have already been obtained in reference to the
masses there noticed.
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