New Ulm review. (New Ulm, Brown County, Minn.) 1892-1961, 1893-05-17
THE ECLIPSED sun.
OBSERVATIONS GATHERED FROM
.@z ECLIPSES OF THE SUN.

=
ture of his mysterious appendages to be
photographed and analysed spectroscop.
ically. Never in the whole history of
astronomy has finer opportunity fol
such work been afforded and SO skill
fully and completely improved by as
tronomers as that of the recent eclipse.
The full harvest of their observations
seems to promise some startling revela-
tons. 49,
M. Flammarion, the French astrono-
mer, after reading the Gillian cable dis
patches announcing Professor Picker
ing's recent eclipse observations, is re-
ported to have said: ''They confirm the
theory that the sun, is surrounded by q
luminous atmosphere to distance equal
to one-eighth of the suns diameter
Scarcely quarter of a century ago many
astronomers questioned whether the So
lar atmosphere. had any marked extern
sion, and even doubted whether the CO.
roma was solar appendage at all. But
in the light of the late eclipse it is not
astonishing that an astronomer expresses
the opinion that the suns atmosphere
extends outward more than 1OO, 1000 miles.
The eruptive forces of the sun must be
enormous indeed to eject the matter
composing the flaming prominences not
infrequently observed 40 900 miles broad,
with an uprush of 225 miles second and
attaining occasionally an elevation of
100000 miles. All prominences, Zollner
and Respighi have shown, are originally
phenomena Of eruption, preceded by rec
tilinear jets, either vertical or oblique,
ascending to great heights and then seen
falling back again toward the sun like
the jets of our fountains. The eruptive
prominences are, as Professor Young
says, generally associated with active
sun spots. Since during the late eclipse
these prominences were conspicuous in
connection with an unusually brilliant
and extended corona and great spotted
ness, the before seemingly established
law that the coronas size and luminosi-
ty are in direct proportion to the suns
spot producing activity is strikingly cor
roborated.
Professor Schaeberle cabled from Chill
that his eclipse observations confirm his
mechanical theory of the corona, which
regards this vast appendage as composed
OF streams Of matter elected with initial
velocities of $50 miles a second from the
sun by forces which are most active near
the sun spot zones. Indications of such
eruptive action have been often observed
IN the higher regions Of the prominences
A further confirmation Of this theory is
that the corona in outline resembled that
which Professor Schaeberle predicted
some months ago AS far back as the
eclipse Of 1870 Mr.. Brothers noted that
''prominence5 were most numerous on
the side of the sun where the corona was
brightest, an evidence that the coronal
matter is not less than that of the promi
nences elected from the sun.
Mr.. Proctor, discussing the observa~
lions of that eclipse, concluded: Il con-
celve we have now clear evidence Of a
form of action-but whether eruptive,
electrical or repulsive is not yet obvious
-exerted outward to enormous distances
by the sun and with maximum emery
over the spot zones, but local, variable
and probably intermittent"
It will be seen, then, that Professor
Schaeberle's theory, though by no means
Established, accords with old observa-
lions. No other explanation of the corona
has been offered save that which attrib-
utes 1t to reflection from myriads of in
candescent meteors or cosmical dust cir
culating around the SUM- But this hy-
pothesis has never been supported. If
the corona were chiefly due to meteoric
dust revolving around the sun, we should
certainly expect to see it regular, and
not as it generally appears, capped, quad
rllateral Or four rayed, with immense
wings CT extensions. There seems, there
fore. to be no other inference possible
but that which telescope scrutiny has
long suggested the corona is orig
mated and maintained by countless eiec-
lions issuing from beneath and flung
through the photosphere by the suns
vertical Or volcanic forces
If the final study Of the coronal photo
graphs obtained sustain this view, sci
ence will have at least a working hy-
pothesis for the determination of the
cyclical variations of solar heat and the
corresponding effects upon terrestrial
temperatures and climates. The theory
in question obviously opens up new
and fascinating inquiry into the ano1na-
lies OF the earth's seasons which are due
to variations of solar activity. We seem
to be thus happily led to the very TIRES
hold of one of the grandest discoveries of
modern science, which promises when
developed to yield a rich harvest of prac-
teal results ..&... .
Now that most numerous and perfect
photographs of all the principal append
ages Of the sun have been secured in
Chill and Africa, astronomers should
give their best energies to the study of
the data. No problem they can now at
tack can be of greater interest or inn
portance to science and the world. New
York Herald. ...s
An Early Astronomical Teacher.
Thales, born $40 years B. c.. was the
first to note the four distinct divisions
due to the positions Of the s11n-yiz the