Omaha Daily Bee Newspaper, November 30, 1916, Page 9

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. | SR ———— Thanksgiving still 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 games. There you will find half of maha's elite tomorrow. Some will . see big eastern games, others will motor to Lincoln to see the Nebraska- 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 evening! when the Fontenelle, 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- cts have been 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- noon. The program consisted of two 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, 5 Mr. and Mrs. W. O. Gilbert will have with them at dinner this evenipg at the Omaha club: Messrs. and Mesdames— R. L. Huntley, E. T. Swobe, i3, 8. Westbrook, Dwight Swobe Louls Nash, Mrs, Eva Wallace Mr. Stockton Heth 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 Mesdames— B/ M. Fairtleld, Arthur Gulou. Frank Judson, Mrs. E. H, Sprague. Miss Daisy Doane. Captain Chandler. Captain White, Mr. Earl Gannelt Mr. and Mrs. G. A, Meyer will have with them this evening: Messrs. and Mesdames— T. L. Davis, Louls Meyer, Glenn Wharton, Migs Louise Dinning. Mensrs.— Ben Warren, Messrs.— 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 guests were included in the party. No Notre Dame Dinner. " Notre Dame's foot ball team will not 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 1. 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- ren Howard and Mr. Clyde Barton plan to motor to Lincoln with a party of yom{f 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 Pritchett and 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 Décember 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 g b Original Cooking club this week on account of the Thanksgiving holiday, but Mrs. Moshier Colpetzer will be hostess at a meeting Thursday of next week. The members of Vesta chapter No. G, 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. Al;out 500 articles will be placed on sale, Personal Mention. Miss Elizabeth Wright of Fair- mount, Neb., is the guest of her aunt, | Mrs. J. H. Rushton, for a few days. Miss Wright is state treasurer of the Daughters of the American Revolu- tion, Monday afternoon Mrs. How- ard Rushton entertained at a small Orpheum matinee party in her honor. Mr. and Mrs: T. F. Stroud have gone to Pontiac, Ill, to spend the Thanksgiving. Mrs. Leonora Nelson has gone to Culver, Ind.,, to spend Thanksgiving with her twq sons who 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 of this city over Thanksgiving. Mr. and Mrs. Edward B. iefierts left Tuesday evening for a short trip to New York. ‘TURKS START DOWN FROM HIGH PERGH People of East Refuse to Pay Fancy Prices for Thanksgiv- ing Birds and Drop Comes. EGG BOYCOTT IS AT WORK Pittsburgh, Pa., Nov. 29.—With the public refusing to buy the turkeys at high prices, the Inarket 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 expectin;, 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 Go 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 ey,gs stored in another warehouse. Chatrles 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, ~ More Gold from Canada. New York, Nov. 20.—~An additional con- slgnment of gold from Canada, valued at $8.000,000, ws deposted at the assay office here today by J. P. Morgan & Co. 'This malkes a total of $24,000,000 recelved in this city and Philadelphia thus far this woek and brings the year's lotal Imports to date from all sources up to about $510,- 000,900 By WILLIAM F. RIGGE. This month brings with it a most exceptional eclipse, nothing less than an eclipse of the Christmas midnight sun. Although nothing whatever of it will be visible to us in Omaha, the occurrence itself is so interesting that it may well find a place here. This eclipse, which is in a certain way the most remarkable that can possibly occur, will come when we are busily preparing for Christmas, that is, ‘when our clocks show 8 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 seas the sun will be shining undimmed in its full splendor, as far as the weather and the season permit. But far away in the Antarctic ocean, about half | way between the Cape of Good Hope and the South Pole, r a limited tract of unfrequented waters, the sun will be eclipsed to such a tiny extent, a trifle 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 see 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 hemisphere, as it will appear to the sun at 2:40 p. m., central time. The sun will then be overhead in the cen- ter of the figure, in latitude 23 degrees, 25 minutes south, and in longitude 130 degrees 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 that 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 as the date is but a few days after the wi ter solstice, the sun's rays shine degrees and 25 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, 35 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 66 de- grees 35 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, 35 minutes south, beyond which it lengthens rapldly until it becomes six months long at the pole. As soon as we drrive 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 further mo- tion must take us away from it, that is, carry us north. Hence, as soon ag 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 come to 66 degrees, 356 minutes, south latitude, the lower- most point on our diagram, when it will sink below the south horizon. All the way between this latitude and the pole, we can'see the sun at midnight. As we leave this limit, that is, pro- ceed on our northward journmey 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 degrees, 356 minutes, north latitude, across the sunlight hemisphere towards 66 degrees, 35 minutes, south latitude, beyond the south pole, will be repeated in the same order If we exchange night and day, and north and south, 1 must call attention to another fact, that is, a8 soon as we passed the south pole, our meridian changed 180 degrees, from being 130 degrees west, it becomes b0 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 avold confusion, since all the meridians meet at the poles. Th 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 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 N8, to 3 o'clock, on the last mark to the right. | The larger circle is the moon's penumbra, which is of great impor-| To under- | Ask for and Get 9 ‘ SKINNERS THE HIGHEST QUALITY MACARONI 36 ge Aecipe Book Free SKIENZR MFG.CO., OMAHA, U.SA LARGEST MACARON! FACTORY IN AMERICA ° THE BEE: OMAHA, THURSDAY, Heavens in December of One of the Unusual Marvels of Terrestrial Geography and Siderial Astronomy NOVEMBER 30, 1916. FIGURE 1—SOLAR ECLIPSE OF DECEMBER 24-25, 1910 FIGURE 2—-MAP OF THE SOLAR ECLIPSE, stand its nature and its action, I must and we have an annular ask the reader to try with me a very| eclipse. instructive experiment. Let us place a pilece of white paper in direct sun- light and hold a small ball to the paper. We notice that the shadow is black and sharp and as large as the ball. As 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 as 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. 1In 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|even a magnifying glass woul ring of light about the black moon, | show the differenc Thanksgwmg Hotel Fontenelle Special Dinner de Luxe in Main Restaurant From Six to Nine at Two Dollars the Plate or which amounts to the same thin sary, of the present eclipse, In an nary solar eclipse the path ol moon, AB on figure 1, lies across part of the earth, so that the pla golar eclipse. penumbra sees the its center. contact at the same moment, contact. ' In some .eclipses the central moon's path AB is so far off the that the pel tran graze the earth, covering that s, This is the 'first most excep- pres- pened years dius, miles. tional fact connected with the ent eclipse, and has never hap before during the thirty-three bral circle cverlaps the ecarth is 2:46 p. m. central time. gram figure 1 in this position. As this is six utes later than the time for the earth has turned one ana degrees more, so that the Jongit the central meridian at this ti 131 difference is hardly noticeable, time 2:40 instead of 2:46 it 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. ““Built for You to Enjoy”’ HOTEL FONTENELLE Management—John F. Letton. Wonders of an Eclipse of the Midnight Sun Described by Father Rigge, Who Tells mbra does little " ring In the second case the apex of the shadow would penetrate the earth if the latter were transparent, or g, the | moon's shadow on the earth is of gome size, and everyone that chances to be in it sees the sun totally eclipsed. After this probably long, but neces- preamble we are prepared to understand the exceptional conditions ordi- f the some ces 80 |' situated may see a total or an annular Every place inside the sun partially eclipsed, the magnitude Increasing al- most in a direct ratio to nearness to Every place on the for- ward edge of the penumbra has first every place on its retreating side has last 1 line |§ does not fall on the earth at all, so that the eclipse is only a partial one everywhere. In the present eclipse the earth more “it to the extent of only 0.008 of its ra- only about thirty-two that the writer has studied eclipses. The moment at which the penum- most The dla- shows the penumbra min- which the terrestrial meridians were drawn, vt ide of me s 1-2 instead of 130 degrees. The If the penumbra had been /drawn for the would overlap the earth so little less that ¢ not | DRI T R H | €D, which is parallel to AB ani tan-|the right of this region the eclipse gent to the penumbra and earth, are all so close together that they prac- tically coincide. The second exceptional pecutiarity of the present eclipse s the fact of the | 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 is | seventeen minutes, For the whole re- | glon, or as astronomers say, for the the pounmbra’s falling south pole, where on beyond | imit of the eclipse,” enters upon the | is, in fact, an eclipse of the midnight | sun. north and south exc t and west as well. For this rea-| son the penumbra moves aganet the higher up on the diagram it would| move with the earth, as It yencrally | does, and lengthen the time of the celipee, . Thirdly, the line CD, the “northern earth at a point to the left of the 13{4.55/ | line NS, so that CD crosses NS on the 4.54) | earth’s disk. As the local time on this | part of the line NS is midnight there That the line CD does really enter the terrestrial sphere at the place mentioned, as well as all tho fother data that are necessary for the construction of the eclipse map, could never be known by even a micro- | ent “eclipse which spectalists will ap- \’llIllllllmm!!!!I!!lll!'l!I!!!!!I“l||I|lIIIIIIIIIIIIIIIIIIIIIIIIIHIIIIIIII"IIIIIIII!'!“!!!“"’ i | course had to be had to rigorous and | versed. This was done on purpose in | The broken 1Z scople examination of figure 1. Re- lengthy calculations, which alone 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 however, the graphic method falls ut terly-—another peculiarity of the pres: preciate Fourthly and lastly, perhaps most exceptional peculiarity of the present eclipse Is the fact of its oc- curring for most places within the eclipse region_on Christmas eve, for some at Christmas midnight. and for|* some others on Christmas morn. Let us now look at figure 2, the eclipse map, and see what wonderful 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 the right, in other words, that the map has been apparently re- order to facilitate comparisons of fig- ures 1 and 2. The numbers 60, 40, 30, 20, 10 below mean the degrees of east longitude, and 75, 70, 65 to the right the degrees of south latitude, arallel of latitude is the antarctic cirele. The point C Is where the line CD of figure 1 enters the earth and the point D where it leaves it. The hglf ellipse marked ‘“northern limit Jof 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 (he eclipse begin, and LC that of ‘‘last contact,” the very last to see it end, The point GE 1is the place of the ‘‘greatest Fcllpne." where 1 per cent of the sun's'diameter is covered by the moon. The dotted curves tangent to the ‘“northern limit" at the pumbers 36, 40 and so on are successiVe pro- Jections of the circular rim of the . moon's penumbra at the correspond- ing minutes after 2 p. m, central time, The last one to the right, however, is the one for 2:69. The eclipse begins at those minutes all along the western {mrtlnn 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.” The penum- bra moves westward, as was said be- fore, instead of eastward, as in all The shaded portion near the letter M shows the reglon where the Christ- mas midnight sun_will be eclipsed. To The ORIGINAL Malted Milk A Nutritious Diet for All Ages, Keep Horlick’s Always on Hand | earth Here, | 2 the | facts calculation has elicited from that | ¢ other eclipges. 1 generally, it is twenty-eight minutes, from the moment of first contact at 2:32 p. m, central time, diurnal motion of the earth anc there- ' when the eclipse begins at the point fore shortens the duration of the|FC, to 8§ p. m., the moment of last oclipse, whereas if it were placed|contact, when it ends at the point LC, | | MOON, [Rine . [South| Set. T2[4.58] 124,65/ 1454 1484 14.54( 454! Tirat quarter on the 1at, 7 Full moon on the 9th, 6:44 a. m. Last quarter on the Tth, 13:06 p. m. New moon on the 24th, 2:31 p. m. First quarter on the 31st. 7 & m, The days are shortening on!i four= teen minutes during the first half of the month and scarcely change at all during the second half. On the 21st at 10 p. m. the sun enters Capricorn and s then at the winter solstice. This is the shortest day of the year, nine hours ten minutes, although all the days from the 16th to the end of the month do ndt differ more than a min« ute from it in length, Venus is morning s rising on' the 16th at 9 .a. m. piter is even- ing star &nd crosses the meridian on the 16th at 8:24 p. m. Saturn, still technically a morning star, rises onm that day at 7:37 ? m, The moon i8 in- conjunction with Jupiter on the 6th, with Saturn om the 12th and with Venus on the 22d. S " At the first sign of skin trouble Resinol ‘That patch of eruption is not meces- sartly a serious matter] Eveninsevere, well-established cases of eczema, ring- worm or similar affections,’ Resinol Ointment and Resinol Soap usually re- lieve the itching at once and quickly overcome the trouble comrlmly. How much more, then, can this simple, in- expensive treatment be relied on to dis-( pel skin troubles in their earlier stages. 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