THE BEE: OMAHA, THURSDAY, NOVEMBER 30, 1916.
Personal Gossip : Society Notes : Woman s Work : Household Topics
I
i
November 29, 1916.
Time' was and I feel that I should
finish the quotation by saying, "When
the little toy dog was new and the
soldier was passing fair," but this is
no time for sorrow and I had intended
to talk about Thanksgiving. To re
sume the thread of thought, then,
time was when Thanksgiving stood
for snow and sleigh rides to the old
country place, where all the cousins
and uncles and aunts, big and little,
gathered after service at the little
country church to give thanks with
grandfather and grandmother over a
bountiful turkey dinner.
Thanksgiving stilt remains the day
of homecomings and plentiful repasts,
but snow and sleigh-bells have gone
out of fashion. Now we frown if dark
clouds threaten a downfall of flakes,
for our plans necessitate clear weather
our plans, you understand, to at
tend one of the numerous foot ball
ti : i t j i i r r
games. ncrc vuu win iiiiu nu ui
maha's elite tomorrow. Some will
see diet eastern trames. otners will
mnrnr in i.inrnln m see th Nehraslfa-
Notre Dame fray and yet others will
attend the High school-St. Joseph
game or the Creighton game here.
Some visitors are coming to make the
day festive and despite all our troubles
and the high cost of living Omaha
will lift a radiant face tomorrow morn
to give thanks for its many blessings.
Many celebrations will begin this
eveningf when the FonteneTle, the
Blackstone and the Omaha club will
be the scene of a large number of big
Thanksgiving dinner parties.
Franco-Belgian Card Party.
No tickets for the benefit card
party given by the Franco-Belgian
Relief society at the Blackstone will
be sold at the door Saturday after
noon. Four hundred and fifty tick
ets haveeen sold to Omaha women
and requests have come from inter
ested friends in Plattsmouth, Council
Bluffs and Fremont. A few tickets
still remain, which may be had by
applying to Mrs. O. C. Redick before
Friday noon.
Studio Program.
Alice Virginia Davis and Cecil W.
Berryman gave forth two piano pro
grams at the studio Saturday after-
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waltzes by Chabrier, the Saint-Saens
variations on a Beethoven minuet and
a concerto played by Miss Davis. The
studio was filled with an enthusiastic
audience.
Dinners at the Omaha Club.
Mr. and Mrs. W. O. Gilbert will
have with them at dinner this evening
at the Omaha club:
Messrs. and Mesdamsa
R. I.. Huntley, Bj. T. Swob.
E. S. Westbroolt, Dwhrht Swobs. .
Louis Nash,
Mrs. Kva Wallace.
Mr. Stockton Hoth.
A Dutch treat party will be given
at the Thanksgiving eve dinner-dance
at the Omaha club, which will in
clude: Dr. and Mrs. C. A. Hull.
Messrs. and Mesdamee-
E. M. Fairfield. Arthur Oulou.
Frank Judson.
Mrs. E. H. Spraffue.
. Miss Daisy Doane.
Captain Chandler. ..
Captain White.
Mr. Earl Oannetl.
Mr. and Mrs. G. A. Meyer will have
with them this evening: .
Messrs. and Mesdantes
T. b. Davis, Louis Meyer,
tllenn Wharton.
Miss Louise Dtnntns.
Mwsra Messrs
Ben Warren, Gerald Wharton.
Luncheon and Matinee Party.
Complimentary to Mrs. Julius
Schonberger of Portland, Ore., Mrs.
Louis Sommer and Mrs. Samuel Som
mer entertained at luncheon at the
Hotel Fontenelle today, followed by
a matinee party at the Orpheum. Nine
guesti were included in the party.
No Notre Dame Dinner.
jNOtre uame s ioot. Dan team win
ndt stop in Omaha for dinner and
dance after Thanksgiving, is the ul
timatum of the president of the
school. Consequently Mr. Harold
McConnell and his committee are re
funding to Notre Dame alumni the
$725 which they subscribed for the
dinner which was to have been given
at the Blackstone.
Thanksgiving Day Gossip.
Mrs. A. V. Kinsler, who has just re
turned from New York, and Mr. Kins
ler expect to celebrate Thanksgiving
day by attending the foot ball game.
Mr. and Mrs. James I. Woodard will
have a quiet family dinner tomorrow.
. Mr. and Mrs. John A. McShane will
have with them for Thanksgiving din
ner Mr. and Mrs. Willard D. Hosford.
Mr. Clyde Barton of Pawnee City,
a law fraternity brother of Mr. War
ren Howard, will come up today for
an Orpheum party this evening. To
morrow Miss Loa Howard, Mr. War
reu Howard and Mr. Clyde Barton
plan to motor to Lincoln with a party
of young people to attend the Ne-braska-Notre
Dame game.
Mr. and Mrs. S. S. Carlisle will
have as their dinner guests tomorrow
Mr. and Mrs. R. L. Huntley.
Mr. Sam Carlisle and Miss Virginia
go this evening to Chicago to spend
Thanksgiving and remain until Mon
day with Mr. Winston Cowgill.
Mr. and Mrs. G. A. Meyer will have
at a family Thanksgiving dinner to
morrow Mrs. Henry Meyer and Miss
Marguerite Meyer,
Mr. and Mrs. John L. Kennedy,
will have with them for Thanksgiving
dinner Miss Mary France and Miss
Virginia Hanscom of New York and
Mr. and Mrs. Harold Pritchettand
Miss Hilda Hammer.
On the Calendar. .
Mrs. A. V. Kinsler will be one of
the hostesses to entertain for members
of the younger set during the Christ
mas holidays. On Friday evening,
December 29, she will give a large
dancing party at the Fontenelle.
The White Shrine Whist club will
give a luncheon and card party at
the Blackstone December 7.
The Woman's club of the Railway
Mail Service will give a kensington at
the home of Mrs. R. L. Frantz, 2916
Poppleton avenue, Wednesday after
noon, December 6. at 2:30 o'clock.
The affair is for all members and ex
members of the club.
There will be no meeting of the
Original Cooking club this week on
acconnt of the Thanksgiving holiday,
but Mrs. Moshier Colpetier will be
hostess at a meeting Thursday of next
week.
The members of Vesta chapter No.
6, Order of Eastern Star, will give
a card party Wednesday evening at
the Masonic temple. Prizes will be
given for both games, whist and high
five.
Mrs. Arthur Remington will enter
tain the members of the Original
Monday Bridge club on Monday of
next week. '
The Christmas bazar of the Ladies'
auxiliary of the Omaha Letter Car
riers, will be held on December 15 and
16 in the lobby of the Bee building.
About 500 articles will be placed on
sale.
Personal Mention.
Miss Elizabeth Wright of Fair-
mount, iseb., is the guest ot her aunt,
Mrs. I H. Rushton, for a few days.
Miss Wright is state-treasurer of the
Daughters of the American Revolu
tion. Monday afternoon Mrs. How
ard Kushton entertained at a small
Orpheum matinee party in her honor.
Mr. and Mrs. T. F. Stroud have
gone to Pontiac, 111., to spend the
inanKsgiving.
Mrs. Leonora Nelson has srone to
Culver, Ind., to spend Thanksgiving
witn ner twq sons wno are in the
military school.
Mrs. Tom Murray of St. Paul.
Minn., and Miss Anna Krenz of Dun
lap, la., are visiting Mrs. Anna Royer
ot tms city over .thanksgiving.
Mr. and Mrs. Edward B. Lefferts
left Tuesday evening for a short trip
to New York.
TURKS START DOWN
FROMJGH PERCH
People of East Refuse to Fay
Fancy Prices for Thanksgiv
ing Birds and Drop Comes.
00 BOYCOTT IS AT WORK
Pittsburgh, Pa., Nov. 29. With the
public refusing to buy the turkeys at
high prices, the market here has sus
tained another sharp slump and
prices today were as low as 18 cents
a pound for the live fowls and a large
supply on hand.
Shippers who had sent many car
loads and boat loads here expecting
to sell their fowls for 35 cents a
pound live weight, found few buyers
and they had to slash their quotations
or find no takers.
Retail dealers are still holding out
for 35 cents a pound dressed weight,
but some were forced to sell as low as
22 cents a pound yesterday.
Shippers had been expecting to get
35 cents a pound live weight. Some
shippers, rather than accept the low
prices, sent loads of turkeys back to
Ohio and West Virginia. Others sold
for what they could get. Further
price reductions are expected.
Egg Prices Co Down.
New York,Nov. 29. The price of
cold storage eggs at wholesale was
1 to 2 cents lower today than yester
day morning when the egg boycott
began.
Eggs sold at 34 to 38 cents a dozen,
according to grade. The average price
for fresh eggs was 63 cents, as com
pared with 55 cents at this time a
year ago. The price of fresh eggs
showed no change from yesterday.
Some wholesale dealers asserted
that the boycott would play into the
hands of -foreign buyers. They said
that, men who want eggs for export
are waiting for a price reduction. The
Housewives' league today continued
active missionary work to discourage
the use of eggs. '
Chicago, Nov. 29. City," state and
federal officials together with civic,
women's and other organizations
were working today in an attempt to
solve the high cost of foodstuffs
problem.
It was announced that municipal in
spectors had discovered in storage
about 800,000 eggs of questionable
quality, while more than 2,000,000
eggs were found in cold storage
houses awaiting price increases. In
addition government inspectors found
36,000,000 et,gs stored in another
warehouse.
Charles F. Clyne, United States dis
trict attorney, began an inquiry into
charges that James E. Wetz is the
holder of 72,000,000 eggs in Chicago
and to learn if Wetz is not the actual
owner who is backing the alleged at
tempted corner.
"Lincoln Seated" is
To Remain in Omaha
"Seated Lincoln," the magnificent
bronze statue by Solon Borglum
which was on exhibition at the Fine
Arts exhibit at the Fontenelle, has
been purchased by C. N. Dietz. The
original of this expressive statue is
now in Newark, N. J. "Blizzard," a
small bronze, has become the posses
sion of Mrs. Moshier Colpetzer and
the painting by Paul Dougherty enti
tled "Midsummer" was . bought by
Charles T. Kountze.
After the Palimpsest club dinner
Tuesday evening the Fine Arts soci
ety closed its successful exhibit. The
collection was first opened a week ago
last Saturday to the Fine Arts society
for a private view and has since been
open to the public. Mrs. Ward Bur
gess, chairman of the exhibition com
mittee, delayed the closing until the
last possible moment in order to give
everyone an opportunity to enjoy the
works of art. '
Mora Gold frol
Now Tork, Nov. II, An additional con
signment of fold from Canada, valued at
18.000,000, we deposted at the aaaay olTlce
here today by J. P. Morgan A Co. This
makes a total of $24,000,000 received in
this city and Philadelphia thus far this
woek and brlns the year's total Imports
to date from all sources up to about $510,.
OOO.OOO.
Heavens in December Sun Described by Father Rigge, Who Tells
of One of the Unusual Marvels of Terrestrial Geography and Sidmal Astronomy
By WILLIAM F. RIGGE.
This month brings with it a most
exceptional eclipse, nothing leas than
an eclipse of the Christmas midnight
sun. Although nothing whatever ot
It will be visible to us In Omaha, the
occurrence Itself I so Interesting that
It may well find a place here. This
eclipse, which la In a certain way the
most remarkable that can possibly
occur, will come when we are busily
preparing for Christmas, that la, when
our clocks show t p. m. central time
on Christmas eve. We In the United
States will not even get a glimpse of
it nor will any one in the whole of
North and South America, nor In the
wide extent of the Pacific ocean. For
us and for all these lands and seaa the
sun will be shining undimmed In Its
full splendor, as far aa the weather
and the season permit. But far away
In the Antarctic ocean, about half
way between the Cape of Ciood Hope
and the South Pole, over a limited
tract of unfrequented waters, the sun
will be eclipsed to such a tiny extent,
a trine over 1 per cent, that it seems
to be a downright waste of time, If
not absolute folly, to mention It at
all. But for the ships that may be
there to nee it, the eclipse will occur
when some of them have midnight,
Christmas midnight, while others have
any hour or minute on Christmas eve
from 9:41 p. m. to midnight and few
have already for a few minutes after
midnight begun Christmas day.
Look at figure 2 for explanation.
Here we have the earth, the sunlit
hemlaphere, aa It will appear to the
sun at 3:40 p. m., central time. The
sun will then be overhead in the cen
ter of the figure, in latitude 23 degrees,
26 minutes south, and In longitude 130
degreea west. The greater part of
North America, and all except the ex
treme eastern part of South America,
the whole Pacific ocean and a part of
Australia will then have day. As the
earth Is turning eastward on its axis,
that is, towards the right in the dia
gram, the sun will be setting all along
the entire right half of the circle thai
is seen to bound the terrestrial globe
in figure 2, and rising all along Its
left half. The north pole is not visi
ble, it Is In the middle of Its six
months' darkness. The south pole,
however, Is in full view, and aa the
date is but a few days after the win
ter solstice, the sun's rays shine 28
degrees and 26 minutes beyond the
South Pole, so that If the earth did
not move In an orbit around the sun,
but only turned on Its axis, all the
sunlit region about the South Pole
would have perpetual day.
The line N 8 crossing the earth is
the central meridian, the only one of
all the meridians on the earth to be
projected Into a straight line at the
time mentioned, when our clocks show
2:40 p. m., central time, on Christmas
eve. Its longitude, as said before, is
130 degrees west. All along that line
It is noon. if we were to start at the
very top of the figure near the letter
N in latitude 66 degrees, 36 minutes
north, the sun would be seen to just
rise above the southern , horizon at
midday. For every degree of latitude
that we go south on this central merid
ian, the sun Is one degree higher at
noon, and the day is getting longer.
From a few minutes in latitude 06 de
grees 36 minutes north, it lengthens
to twelve hours at the equator, where
its length never changes all the year
round. When we come to latitude
23 degrees, 26 minutes south, to the
place In the exact center of the dia
gram, the sun Is directly overhead.
As we proceed southward, the sun be
gins to sink towards the north. The
day is all the time lengthening and
becomes equal to twenty-four hours
as we reach latitude 66 degrees, 36
minutes south, beyond which It
lengthens rapidly until it becomes six
months long at the pole.
As soon as we arrive at the south
pole, there is no direction but north,
since we eannot possibly go farther
south than the south pole, and when
we have reached It, any rurtner mo
tion must take us away from it, that
is, carry us north. Hence, aa soon as
we have passed the South Pole, while
we continue on our straight line or on
our great circle, we are going north,
the sun is now south of us, instead
of north, as it was before, and noon
has changed to midnight. The sun
Is visible until we oome to 66 degrees,
36 minutes, south latitude, the lower
most point on our diagram, when it
will sink below the south horlson. All
the way between this latitude and the
pole, we can1 see the sun at midnight.
As we leave this limit, that is, pro
ceed on our northward journey past
the lowermost point on the diagram
and enter the dark hemisphere, the
sun begins to dip more and more be
low the south horizon at midnight.
And all that has been said about our
Journey from 66 degreea, 36 minutes,
north latitude, across the sunlight
hemisphere towards 66 degrees, 36
minutes, south latitude, beyond the
south pole, will be repeated in the
same order If we exchange night and
day, and north and south.
I must call attention to another
fact, that is, as soon as we passed the
south pole, our meridian changed 180
degrees, from being 180 degrees west.
It becomes 60 degrees east. We will
need all these facts to understand the
exceptional circumstances of the pres
ent eclipse.
The reader will also notice that
only two meridians have been drawn
across the south pole for the region
within ten degrees of It. This was
done to avoid confusion, slnoe all the
meridians meet at the poles. The
two, or we may say, the four that
are drawn, are first, the meridian of
Greenwich, which is the one to the
right and below, and quickly enters
the dark hemisphere. The second
one, the upper one to the right, is
the ninetieth meridian, which we may
trace through the middle of the Gulf
of Mexico and the United States, and
which is our own standard meridian
and gives us central time, this being
six hours slow of Greenwich. The
next one on the diagram is the 180th
meridian, on which all mariners
change their date, dropping a day
when going west and repeating it when
going east The last meridian drawn
across the south pole, the lower one
to the left, Is the ninetieth east of
Greenwich.
We may now turn our attention to
the two circles below the terrestrial
sphere on figure 1. The smaller one
is the moon. Its center moves along
the line AB, where its position is
given for every ten minutes during the
eclipse time, from 2:30 p. m, central
time, on the first mark to the left,
near the line NS, to 8 o'clock, on the
last mark to the right.
The larger circle Is the moon's
penumbra, which is of great impor
tance in every solar eclipse. To under-
Skinner5
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FIGURE 1 SOLAR ECLIPSE OF
FIGURE 2-MAP OF
stand Its nature and its action, 1 must
ask the reader to try with me a very
instructive experiment. Let us place a
piece of white paper In direct sun
light and hold a small hall to the
paper. We notice that the shadow Is
black and sharp and as large as the
ball. Aa we separate the ball and
paper, the shadow becomes more and
more Indistinct at the edge. The true,
shadow we call the umbra, and the In
distinct part the penumbra. When we
have separated our ball and paper so
far that their distance apart is 114
times the size of the ball, the umbra
has diminished to a point and the
penumbra has grown to have a diam
eter twice as large, as the ball. If our
ball is as large as the moon on figure
1, and Is held at a distance of 114
times Its diameter from the figure, Its
shadow or umbra will be the point on
the line AB which Is at the time 2:46,
while the penumbra will be the outer
and larger circle. We will not be able
to see the umbra and penumbra on
our paper, because the first Is a point
and the second is too faint, but they
are really there, notwithstanding. We
can actually see them or their effects
very accurately If we put our eye In
the place of the paper and look at the
ball, taking the precaution to use a
smoked glass. When our eye Is. ex
actly on the circumference or edge of
the penumbra, we will see our ball
apparently touching the sun. This
astronomers call contact, first con
tact when the eclipse begins, last con
tact when it ends. As we move our
eye along, or better, as our moon, the
ball, moves across the sun, we will
see the sun obscured more and more,
until It is completely covered and we
have a total eclipse.
Now aa the moon's distance from
the earth may vary about 16 per cent,
the moon when far away appears
smaller than usual and cannot cover
the whole sun, whereas when near It
appears larger and can more than
cover the whole sun. In the first case,
the point of the moon's shadow, the
apex of the shadow cone, does not
reach the earth; the sun appears as a
ring of light about the black moon,
(
Illlllllllllllllllllllllllllllllllllllllllllllllllllllllllllilllllllllllllllllllllllllllllllllllll8
I Thanksgiving
I Hotel Fontenelle
Special Dinner de Luxe
1 in Main Restaurant .
I From Six to Nine at Two Dollars the Plate I
Commencing at Ten P. M.
A Supper Dance
In Main Restaurant and Palm Room
Service a La Carte
Table Reservations may be made by Phone
Douglas 3207.
I "Built for You to Enjoy" I
1 HOTEL FONTENELLE
Management John F. Letton. . ?
VlllUMIIMllUH!!!!!MI!!!!n!!!lllilllllMIIIIIIIIIIIIIMIIIIIIIIIIIlilllUlllllllltlMIM!l!i'
DECEMBER 24-25, 19K..
THE SOLAR ECLIPSE.
and we have an annular or ring
eclipse. In the second case the apex
or the snaaow wotim penetrate tne
earth If the latter were transparent, or
which amounts to the same thing, the
moon's shadow on the earth la of sme
size, and everyone that chances to be
in It sees the sun totally eclipsed.
After this probably long, but neces
sary, preamble we are prepared to
understand the exceptional conditions
of the present eellpsej in' an ordi
nary solar eclipse the path ot the
moon, AB oh figure 1, lies across some
part of the earth, so that the places so
situated may see a total or an annular
Solar eclipse. Every place Inside the
penumbra sees the sun partially
eclipsed, the magnitude Increasing al
most in a direct ratio to nearness to
Its center. Every place on the for
ward edge of the penumbra has first
contact at the same moment, every
place on Its retreating side has last
contact ( ,
In some .eclipses the central line
does not fall on the earth at all, so
that the eclipse is only a partial one
everywhere. In the present eclipse the
moon's path AB Is so far off the earth
that the pesyimbra does llttla ' more
tun graze the earth, coverlng'Mt to
the extent of only 0.008 of Its ra
dius, that Is, only about thirty-two
miles. This is the 'first most excep
tional fact connected with the pres
ent eclipse, and has never happened
hanrn rinptna th thtriv.lhree VAHrs
that the writer has studied eclipses. J
The moment at wnicn tne penum
bral circle overlaps the earth nuwt
is 2:46 p. m. central time. The illa
gram figure 1 shows the penumbra
In this position. As this Is six min
utes later than the time for which
the terrestrial meridians were drawn,
tin, earth has turned one an.l t liuif
dtp;reea more, so that thu longitude of
the central meridian at this time in
131 1-2 Instead of 130 degrees. The
difference is hardly noticeable, if the
penumbra had been Alrawn for the
time 2:40 Instead of 2:46 it would
overlap the earth so little less I hat
even a magnifying glass wotiltj not
show the difference. In fact, the line
CD, which is parallel to AM an.'! tun:
gent to the penumhru and earth, ure
all so close together that they prac
tically toineiUe.
The second exceptional peculiarity
of the present eclipse is the fact of
the i-otinmbra's falling beyond the
south pole, where on the tllar:im
north and south exchange na-ne, and
e;ist and west as well, Kor this rea
son Ihe penumltra moves "att.m't the
ititirnal motion of the earth unc there
fore shortens the duration of the
eclipse, whereaa if it were placed
higher up on the diaKram it would
move with the earlh. as It generally
does, and lengthen the time of the
jell:fre.
Thirdly, the line CD. the "northern
limit of the eclipse," enters upon the
earth at a point to the left of the
line NS, so that CD crosses NS on the
earth's disk. As the local time on Hiis
part of the line NS la midnight, there
is. In fact, an eclipse of the midnight
sun. That the line CD does really
enter the terrestrial sphero at the
place mentioned, as well aa all th?
other data that are necessary for the
construction or the eclipse map, could
ne;er be known by even a micro
scopic examination of figure 1. Re
course had to he had to rltrorous and
lengthy calculations, which nlone
could ferret out the desired knowl
edge. Deriving the necessary data
from a diagram like figure 1 Is "al
ways a very easy and expeditious
method, when the penumbra crosses
the earth somewhat centrally. Hero,
however, the graphic method falls ut
terly another peculiarity of the prea
ent eclipse which specialists will ap
preciate. fourthly and lastly, perhaps the
moat exceptional peculiarity of the
preaent eclipse in the fact of Its oc
curring for most places within the
eclipse reglon,.on Christmas eve, for
snino at Christmas 'midnight, and for
some others on Christmas morn.
Let us now look at figure 2, the
eclipse map, and see what wunderful
farts calculation has elicited from that
minute portion of figure 1, where the
moon's penumbra passes across the
earth's disk.
The first thing we notice on the
map, figure 2, Is that south Is on top
and west to tne right In other words,
that the map has been apparently re
versed. This was done on purpose in
order to facilitate comparisons of fig
ures 1 and 8. The numbers 60, 40,
30, 20, 10 below mean the degreea of
east longitude, and 76, 70, 66 to the
right the degrees of south latitude.
The brokan parallel of latitude Is the
antarctic circle. .
The point C Is where the line CD
of figure 1 enters the earth and the
point D where it leaves It The half
ellipse marked "northern limit fof
eclipse" Is the projection of ' the
straight line CD of figure 1 on the
spherical earth, distorted partly by Its
rotation. The point FC on figure 2
Is the place of "first contact." the
very first place on earth to see Ihe
eclipse begin, and LC that of "last
contact" the very last to see It end.
The point OK Is the place of the
"greatest eclipse," where 1 per cent of
the sun's 'diameter Is covered by the
moon. The dotted curves tangent to
the "northern limit" at the numbers
35, 40 and so on are successive pro
jections of the circular rim ot the
moon's penumbra at the correspond
ing minutes after 2 p. m. central time.
The last one to the right however, 1b
the one for atts. The ecllpss begins
at those minutes all along the western
portion of the curve from the num
ber on the "northern limit" line to
the curve "eclipse begins at sunset"
and ends along the eastern portion
from this same number to the curve
"eclipse ends at sunset," Ths penum
bra moves westward, as- was sold be
fore, instead ot eastward, as in all
other eclipses, .
Ths shaded portion near the! letter
M shows the region where the Christ-
mas midnight sun will beeellpserjTi
Safe
Milk
orlntaitt
ft Invalid
SubttiratM
Cost YOU
aasaerriM
A Nutritious Diet for Alt Age.
Keep HorUclc's Always on Hand
Quick Lunch , Homa or Office.
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lli'iQpT.Mi'Hlfi I
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WOMEN! I INVITE YOU TO CALL
And know of the help for diseases and disorders of your sex. Many
hundreds have been to me and are pleased. I have saved many from
an operation. SPECIAL and PRIVATE diseases treated strictly
confidential. Cash fees, but small. Medicine free.
DR. J. C. WOODWARD, 301 Rose Bldf., T.I. Tyler 2SO, OMAHA.
the right of this region the ecllpss
occurs between 9:41 p. m. and mid
night, local time, on Christmas eve;
to the left of It after midnight on
Christmas morn. The longest dura
tion of the eclipse at any one place la
seventeen minutes. For the whole re
gion, or as astronomers say, for the
earth generally, It la twenty-eight
minutes, from the moment of first
contact at 2:32 p. m., central time,
when the eclipse begins at ths point
FC, to 3 p. m., the moment of last
contact, when It ends at the point
l.c.
MOON.
nil.
RIfNoonHt. flBC Rise. South get.
i;t itiii.iM.sst wud. ii : t.asl i 7:
10 7 30 tt.ii4.it Thu. li.si l.iiit.mas
t7 SI II. 1J I.St FN. 11. ! l.lTMIdnt
l7 31 11.13 4.14 Hat. 11. S4 7.04 13 15 2
317 33 13.14 4.14 Sun. 1.33 7 .11 114 1
417 34lt.l4 4.34 Mon. 1.43 1.17 1314
lit 33 13.14 4.34 Tue. 1.11 1.11 lilt
'7 3 IS.lt 4.34 Wad. 1.47 IS. II 4 41 C
7 7 87 11.13 I SI Thu. 1.17 11.01 134 7
3 7 II 13.11 4. S3 FH. 3.03 Mldn IBS
I 7 33 12.lt 1.13 Sat. 4.38 13 31 T 31 1
10 7 40 11.13 4.88 Sun. t. 34 11 33 8 48 IS
1 1 7 41 13.17 1.83 Hon. I.tt 1 44 ( 38 11
117 4113.17 1.13 Tun. 7.87 1 13 It 04 II
13 7 43 13.18 4.84 Wed. 8.37 1 It 10 83 tl
14 7 43 13.18 4.84 Thu. I ll 4 03 10 38 14
18 7 44 13.114.14 Prl. 10.68 4 48 11 33 13
If 7 41 11.11 4.14 Hat. 11.18 I 18 11 43 IS
17 7 41 11.10 1.84 Sun. Hldn ) 08 11.08 IT
18 7 41 II. SO 4.88 Mon. It tt I 47 tl. 17 11
11 7 47 11.31 I.tt Tus. 103 T 33 11.83 It
30 7 47 11. 81 4.88 Wsd. 110 8 10 1.13 St
3I7 48 18 .83 4.81 Thu. 4 13 t IS 1.88 31
S3 7 48 1 3 . S3 4.88 Prl. 8 33 11 11 1.41 31
ii 7 43 18. S3 4.87 Bat. I 43 11 11 1. 4131
14 7 41 13.13 4.87 Sun. T4I1I.1I 4.BS34
38 7 80 11.84 4. 88 Mon. 140 1.S3 I.08 3S
30 7 80 11.31 4.88 Tus. lit 1.33 7.31 20
S77 81 IS.St I II Wsd. 10 00 I. II 1.47 IT
387 81 13.38 4.18 Thu. 10 31 4.11 10.03 31
31 7 83 IS. 3111.00 Prl. 10 II I.tt 11.14 SI
3017 83 13.30ll.0t Sal. 1114 i.41 Mldn 3
HIT S3 11.17 Lit Sun. lilt 8.81 II 31 It
117 83 18.37 8.03 Mon. 11.17 T.14 11)1
3 7 83 18.18 8.01 Tus. 11.48 I. II 1411
1 7 84 11.18 8.04 Wsd. 1.34 1 04 1 41 1
MOON'S PHASES.
Plrst quartar on ths 1st, 7:18 p. la.
Pull moon on ths Ith, 1:44 a. m.
Last quartar en tho Tth. 11:M s. m.
Nsw moon on ths 14th, 3:11 p. m.
Plrst quartar an ths 31st 1:07 a. m.
The days are shortening only four
teen minutes during the first half ot
the month and scarcely change at all
during the second half. On the 21st
at 10 p. m. the sun enters Capricorn
and Is then at the winter solstice. This
Is the shortest day ot the year, nine
hours ten minutes, although all the
days from the 15th to the end of the
month do ndt differ more than a min
ute from It in length.
Venus Is morning star, rising or the
16th at 6:09 a. m. Jupiter is even
ing star and crosses the meridian on
the 16th at 1:24 p. m. Saturn, still
technically a morning star, rises on
that day at 7:17 P. m. '
The moon Is In- conjunction with
Jupiter on the 6th, with Saturn on
the 12th and with Venus on the 2d.
'At the first sign of
skin trouble apply
That patch of eruption It not ntcu
sarily a serious matter) Even In severe,
well-established easel of ecienu, ring
worm, or similar affections,' Reiinol
Ointment and Reiinol Soap usually re
lieve the itching at once and qtuckly
overcome the trouble completely. How
much more, then, can thit simple, hv
expensive treatment be relied on to db-i
pel skin troubles In their. earlier stages.
Reslnol Soap sad Rafinol Obtaamt an said br
all drurrisu. For samplss of ssch, fraa, writ la
Papt 1-R, Rssiaol, fialuners, Me.
