AnjTjit rr, 1905.
THE OMAITA ILLUSTRATED T.EE.
Eclipse of the Sun Visible in Omaha August 30
.moot. ash mLi.rnr.!i.
riioni.a. ao roiiEfirs.
ITroc mlll ha a ti.fal .r.lnB ftf
I I Hi sun on rent Wednesday, Aa-
I nil v tt mill h vlsihln a a
total eclipse on a line beginning
Just north, but completely out
side of the state of Minnesota, and run
ning arrnns Canada and the Atlantic ocean,
over Spain, the Mediterranean and Red
Mas and terminating on t lie south roast
Cf Arabia. The greatest duration of the total
phase will be three mlnit-s and forty-five
seconds, fully twice as long as the duration
of the eclipse of May 23, 19K, In the south
ern states. The total phase will this time,
however, not occur anywhere within the
Vnlted States, so that our astronomers,
like those of most European nations, will
go to Bpaln to observe the eclipse, and not
to Canada, because In Canada the sun will
be very low in the sky, while In Spain It
will be very high and the eclipse will last
longer.
Explanation of Diagrams.
But the readers of these pages will re
main at home and will therefore be In
terested to know how the eclipse will ap
pear In the Vnlted States. Here the eclipse
will only be partial and will occur near the
time of sunrise. The accompanying map,
Fig. I, will give all the necessary Informa
tion. The first glance at It will show three
Important curves. The one to the right Is
marked "Eclipsa begins at sunrise" and
signifies that all those places through
which this line runs will see the eclipse
beginning at the moment the sun rises.
For all those places that are to the right
of this line the eclipse begins after sun
rise, and for all those to the left before
sunrise, that is, all these latter places will
not see the whole of the eclipse, but will
miss a part of It, owing to the fact that the
eclipse will have begun already before the
un rises for them, the sun therefore rising
partially eclipsed.
Along the middle line marked "Middle
of Eclipse at 8unrlse," the sun will rise
with the maximum obscuration it Is to
have for thoso places. This maximum
obscuration Is Indicated by the numbers
SUN -XklV-zZ-h-X-X U,
1 . l- LI I ',V I fV-Y , If if I
7 0 s
ECLIPSE OF THE
Aug. jo ipos
as visible In, the
UNITED STATES
rig-, x .
"Eclipse begins at Sunrise" near Cnne
Charles, at the mouth of Chesapeake bay,
shows the place of 'First Contact," that is
the nlace which Is the very first on earth
and Is expressed in tenths of the iun'1 to S(,e thlB eclpSp begin.
diameter obscured, intermediate distances
being In proportion. For example, at
Cairo, 111., the sun will rise with an ob
scuration of 0.83.
The exact appearance of the sun when
various tenths of its diameter are obscured
are represented In Fig. II. The first circle
Is the sun with the moon placed before It
In such a way as to hide 1, 2, 3, 4, 6, (, 7, 8,
( tenths of Its diameter, the separate ap
pearances of the sun thus eclipsed being
shown In the other figures.
The line to the left marked "Eclipse ends
at Sunrise," connects all those places for
which the eclipse will end at the moment
of sunrise, and which will therefore Just
miss the eclipse completely. To the left
or west of this line the eclipse will not be
visible at all.
Between the lines "Eclipse begins at Sun
rise" and "Middle of Eclipse at Sunrise,"
the sun will rise eclipsed to the extent
which may be found by reference to the
curved lines marked 0, 2, 4, 6, 8, which show
the even tenths of obscuration. The eclipse
will Increase until it reaches the magnitude
shown by the other set of lines which start
from the "Middle of the Eclipse" line, run
eastward and are marked to single tenths
of obscuration. An example will make this
Clear. At Columbus, O., the sun will rise
omewhat lens than four-tenths (0.S8)
eclipsed, and the obscuration will Increase
to nearly four-tenths (0.69), and, of course,
.Iter that diminish to nothing.
What Omaha ns Will Pee.
It Is a pity that the path of this totxl
eclipse should come so near to the Vnlted
States and not enter them at all, for a
total eclipse of the sun Is, without excep-
we see suspended In midair an enormous
black ball the moon the geometrical solid
ity of which Is most Impressive. Around
about it on all sides is that superb and
nrnirnlncent radiance called the corona,
which, like a halo of glory about the head
of a saint. Is brtWant with roseate and
scarlet light. It encircles the moon like a
close ring, Interspersed with pearly points
tlon, the most magnificent phenomenon that resembling carbuncles and gems. Beyond
It Is truly these there Issue delicate and fading fllft
a Journey monts of light, like a bursting mass of
fireworks, In the midst of which are dark
rifts and streams of light of such surpass
ing beauty that no artist's brush, no pho
tographic plate can ever portray to those
it is given to man to witness.
a sight that It is worth
around the world to see.
Eclipse a Wonderfnl lht.
While the outer positions of the solar
disk are belrg obscured by the advancing
OQQQ
rg. n.
THE BUN WITH VAHIOU8 TEN THS OF ITS DIAMETER OBSCURED.
could be known of them until Lockyer
"and Jansen In 1R68 simultaneously discov
ered a method of seeing and measuring
them apart from times of eclipse. No cor
responding method has been discovered of
photographing or seeing the corona in full
sunlight,' although many and most in
genious devices have been used to that enJ,
Hence astronomers are forced to make use
of every total eclipse to ascertain the sun's
physical condition. They wish to know
what the corona Is, what causes it, does It
change, does It change rapidly like the
prominences, Is there any causal connec
tion between the corona and the promi
nences or sun spots?
Fhntosrranhy Plays Important Role.
The most general method of observin F I
the coming total eclipse will be to photo- I
graph the corona. The "science of solar(
eclipse photography has made considerable
advances and an amateur can scarcely
do any useful work unless he makes an
especial study of the subject and profits
by the experiences of others. Successful
eclipse photographers know thoroughly how
to regulate the aperture and the focal
length cf the camera, as well as the
sensitizing and backing of the plate, the
time of exposure, the time and manner of
developing, and many other details, in or
der to bring out a desired feature of the
corona. They know that, on account of the
great Inequality In the tight, one plate
cannot reproduce the whole corona, but
may disclose Its Identity during this eclipse
In the same way that helium and other
substances have done in former eclipses.
rhotometrlc observations of the corona
and of Its varous parts will be another
task to be performed during the coming
eclipse. This Is done more accurately
by photograph? and requires a special
outfit.
The nest radiation of the eorona will
engage the attention of other astronomers
and Important Information Is expected on
this point from the present eclipse.
Work-for the Obserrers.
All scientific astronomers will hare at
least one observer In their party whose
duty It will be to note the beginning and
end of the total eclipse as well as of Its
partial phases with the utmost accuracy.
To render these observations of value
to science in giving us a tietter knowledge
of the moon's position and motion, the
latitude and longitude of the place of ob
servation must be determined by many
night's work before or after the eclipse.
There are a few astronomers who will
not observe the sun at all when It Is
totally eclipsed, but selxe the advantage
ofTered by the darkness to devote their
attention to other phenomena which can
be seen only during that time. The most
important of these Is the discovery of
planets called Intra-merucrlal, because
their orbits lie Inside the orbit of Mercury,
which are always so near the sun that
Its light prevents our seeing them at njl
times outside of a total eclipse. The ex
istence of some of these bodies Is sus
pected, and two great astronomers claim
to have seen them, but their observations
require confirmation.
From the above mentioned methods and
objects of observation it is easy to under
stand the Importance which astronomers
attach to a total eclipse of the sun and
why so much expense Is Incurred to sol-.?
these problems. I might add other points,
but these would be loo technical.
How Batto Watch It.
Figure III, as Indicated above, represents
the appearance of the eclipsed sun as It
will be visible In Omaha at the moment of
THE UNIVERSITY OF NOTRE DAIY1E
NOTRE DAME, INDIANA.
Twe bears' rise frsaa Chlcaf .
123d Session opens Tuesday, September 12, 1903.
N
7 W
S
FIO. III-THE SUN AS IT WIt,t, AP
PEAR IN OMAHA AT SUNRISE, 5:19
A. M., WEDNESDAY, AUGUST 30, 1905.
moon, and even after three-fourths or more
of the sun's light have been thus Inter-
Between the lines "Middle of Eclipse at cepted. nothing peculiar Is noticed by an
Sunrise" and "Eclipse ends at Sunrise," Inexperienced observer, because this dlmin-
the sun will rise obscured to the extent ution of light might equally well be the
Indicated by the distance of the place effect of massing clouds. When, however,
concerned from the curves which show the moon has advanced so far that only a
the even tenths of obscuration, and this thin crescent remains of the once glorious
obscuration will be on the decrease. For orb of day, the sunlight begins to appear
example, at Omaha, the sun will rise fl.Sfl of ashen color. Something unusual and un-
eoilpsed and present the appearance shown natural comes over the aspect of nature,
on figure S. Animals become puzzled, fowls retire to
The dotted lines marked V, VI. VII, at rest and all nature seems to pause In pres-
tho bottom of the map connect thoso places ence of the great portent. The sunlight
at which the sun will rise at 8, S, 7 o'clock now diminishes rapidly, something like an
central time. If eastern time Is used, one Impenetrable black cloud comes earthward
hour must be added to the time indicated over the landscape with the speed of a
and if mountain or Pacific times, one and cannonball, and an Instant later we are
two hours respectively subtracted. enveloped In darkness. The stars shine out
The mark f on the line where the and in place of the sun's waning crescent,
who have not seen It the entrancing loveli
ness of that sublime phenomenon.
Scientific t'ses of Solnr Eclipse.
The scientific uses to which a total solar
eclipse Is devoted are numerous and lm-
sunrtse, at 1:49 a. m., next Wednesday
mnfnlnCT M B TIT . " , ). n Mn.ll... I nnlnl.
they must either make many exposures of , ... , . , . ,
. . . .. . of the sun. T being the uppermost point.
Unfortunately l'or us, the maximum ob
scuration will occur for Omaha before sun
rise, so that when we do get to see the sun
the eclipse will be more than half over and
the moon will be well on its way off the
sun's face. However, as solar eclipses are
pretty rare, it will repay the reader to rise
variable durations and then construct a
composite photograph from all of these, or
else prepare their plate In sections for the
Individual parts of the corona It Is to se
cure. With Immense labor and skill most
admirable photographs of the corona have
been made In former eclipses and It Is
TKa llirh I. an Int.nl.lv hnnal Vi t thnu rt tha nra.nnl aAI In, will
r i. .. . " , v . before the sun next Wednesday and see the
brilliant that even the smallest visible por- surpass them all. . ... T 1V. ' ,.
tlon of the solar disk blinds our eyes to Its The spectroscope Is the Instrument from f " ! ri h. f, Ji v
environs. It I. only when the entire disk which the most valuable Information Is ex- . m f r hMe 0r Bmke "er
is covered by the moon that the sun's pected. It I. to determine the position 1., h?"? the ?u" maV bfed at d
v. van, Biru .Hie in iiia. ain?i:i. uiu ored
ui me; corona, wuicn up 10 me present is
the only one that has never been Identi
fied with the line of any terrestrial sub
stance. The unknown element causing this
fainter surroundings, the prominences and
the corona become visible. The promi
nences or protuberances are those brilliant
carbuncles seen close to the lunar orb.
They are eruptions, mainly of hydrogpn
gas, from the solar surface. Very little line Is provisionally called coronlum, and
Gossip ond Slories About Noted People
m
96J9Sk.
or smoked glass must be used. A tele
scope, of coflrse, will add much to the In
terest of the observation. An excellent
method of using a telescope Is to hold a
white card a short distance beyond the eye
piece and to focus the sun's Image upon
it. In this way ' many persona
may view the sun at the same time and no
dark glass need be used. In default of a
telescope the sun's Image may be projected
by means of a small hole In a card, and,
more Interestingly still, by watching the
numerous images of the eclipsed sun made
Senator Daniel's Debt to Grant, Tribune, being entitled. In that capacity,
AM going to tell you of an lncl- to the courtesy of a telegraph frank. The
dent In the life ofl Genera occasion of his wrltlns- his noem wna In
Ulysses S. Grant which has never connection with a request for renewal of by noleB or chlncks ln tn window blind.
ttDoeared in Drlnt. that I know his annual Dass that had exnired with the. Every ow,ot these holes, which ordinarily
of, but which happened to come old year. We believe this effusion has not lve8 a clrcu,ar 'mage, will then show the
Willi I n tny cognizance," said Senator Daniel
of Virginia, when In Chicago, as the guest
of the Hamilton club, to a Record-Herald
writer.
"Along In January or February, 1S6S, a
young Virginia soldier, about 17 or 18 years
before seen the light of print, and we
sun as a cresent. Even the small spaces
offer It to our readers as additional evl- or Interstices between the leaves of a tree
dence. If any were needed, of the natural through which the sunlight can find Its
humor In Mr. Hay's disposition, that had wa to the found will form these crescent
already found expression ln "Jim Bludso" lmM- So that Bucn a Iare collection of
and "Little Breeches." and that was ready crescent images or me sun wm present an
of age (and I want you to understand that at all times to find vent for tha interest aPP'""'a'";e well worth the Inconvenience
The Por fact 3 ear
I Jyy k c crowning feature of any
I function. Nothing so cood wh?n trV
weather's hot, nothing so refreshing when
you are tired, nothing gives such restful sleep.
Omaha
HUOO
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Headquarters
F . U1LZ
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Co. lilurfs Headquarter
Lee mitchell
KB Main Street, Tel. to
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Telephone Number 8, South Omaha.
GrINGul GOING-1 1 GONE ! 11
rzmiviirjin mnascwuwtn iQCunrc&uBPiass
NEWBRO'S HERPIC1DE
Til Osteal AL, rssr tl "kills Dft(l Cars.'
DtOfTT KNOW IT WAtLOADf.il
Mast youn aa4 BMW-agd saea sever
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suluroUc STowtba until the hair aas
'Ton Nature sala bar warn
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fitlanff batr, but the discovery of the
4 itrwg nns la too recent for the
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the dandruff microbe; stops falling
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reinfection. A delightful hair dress
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Save your hair white ysa hare hair t
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m m ti e. Sm4 SK. staawt. at IttnaM Ct , tost I. atuwt. Kick., tm s SMplt.
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APPLICATION'S AT f-ROUlNBNT BARUER KHOPtt. A
every boy ln Virginia from 13 to 14 years
of age upwards was carrying arms
at the time), was instructed by his com
mander, who was Colonel John S. Mosby,
to cross the Potomac to a certain postoffloe
ln Maryland and bring him the mail. lie
wanted It for the military Information be
could get out of it.
"This young man was in his full Con
federate uniform, and, with a comrade or
two, proceeded to execute the order. He
arrived at the postoffloe, and the inconven
ient postmaster showed fight. He killed
him. He got the mail and brought It and
delivered It to his commander. A short
time afterwards he was captured. He was
taken to the city of Washington. He was
court-martialed and condemned to be shot
for murder.
At that stage of the proceedings his father
and mother, whom I knew well and there
were no more respectable and reputable
people ln Virginia went to the city of
Washington and laid the 'case before the
president of the United States, Andrew
Johnson. He referred them to General
Grant.
"General Grant sent for the papers and
read them over, and wrote upon the back
of them words to this effect: 'This young
soldier, In full uniform, obeyed the orders
of his commander. If he had not done so
he ought to have been shot. As he did so
It would be murder to shoot him. He should
be li.stantly discharged.'
"And that Is one reason why I am here,
and why I am glad to pay the respect of a
soldier to the brave, true and honorable
American soldier, Ulysses S. Grant."
Noted Pablle Man.
A unique figure Is that of Goldwln Bmith
of Toronto, who was 82 years old the other
day. He has lived and done public servtre
ln the United States, Canada and England,
and enjoys a large share of esteem and
effectlon ln each coutry. Many years ago
he took front rank as a scholar and thinker.
A Toronto paper says of him: "In the
coutry In which for much more than a gen
eration Goldwln Smith has made his home
be has borne his full part ln the fray of
human affairs, sometimes on the winning,
sometimes on the losing side, exhibiting al
ways a rare degree of personal force and
courage of conviction, but never falling
also to manifest the patience, courtesy and
dignity that are alone consistent with real
eminence of Intellect and Integrity of
heart."
Jobs Hay's ! of Haasor.
Leslie's Weekly has received from a
source of undoubted authenticity a copy of
the following little rhyme by the late John
Hay, written about thirty years ago, when
he was acting as editor of the Ijw York
of early rlsin.
ng.
er c
or amusement of his friends.
I'd rather ride a balky ass,
Or lose my hook to a big black bass
Or stand a she-book-agent's sass,
C f In. .in niil,n. V. . . F 1. 1 . .
Or share King Nebuchadneizar's grass, ct"itlflo observation and note the exact
I have mentioned obtain a distinct Image
of the sun he may try his hand at a real
Than carry around a last vtur'i minx
Them's my sentiments.
THE BARD OF THE MAUMEE.
How Umant Lost f4MM)0,000.
The note of affectlun has been very no
ticeable ln the flood of obituary discourse
in the newspapers about Colonel Lamont.
Prof. H. L. Nelson, writing about him In
the Boston Herald, said that he was a good
deal more than an able man, ln that there
are very few men ln the world who were
possessed as he was of "the beautiful
genius for friendship." He was willing to
sacrifice himself, says Mr. Nelson, either
for a' cause or a friend. There are many
comments from other sources to the same
effect, says Harper's Weekly, taking note
of Colonel Lamont's liking for his fellow
creatures and of the absolute constancy of
his fidelity to those who trusted him.
One story about him that we see In print
tells how, at the Instigation of James J.
Hill and others,, and with their aid, ..La
mont bought a good deal of Northern Pa
cific stock when It was very cheap, and
how when there came along In May, 1901,
the fight between Mr. Hill and others for
the control of the road, someone from tha
group opposed to Mr. Hill came to Lamont
and offered him a bonus of 6,OOO.ouu for his
holdings, which Just then had a market
value of $1,100,000. The ownership of the
shares Lamont held would have carried the
control of the road to Mr. Hill's rivals. But
Lamont would not sell, and subsequently
turned In his tsock to the holding com
pany at a profit of less than a million.
It is noted somewhat too breathlessly
that he threw away something more than
$4,000,000. Of course he did! No man of
good, common sense, let alone sentiment,
would have sold out his friends at such a
Juncture, and It is not abnormally to La
mont's credit that he didn't. But the story,
whether true or not, la pleaaant, and the
stse of the figures help to make It Inter
esting. t Mortis end His Body Guard.
J. Plerpont Morgan Is said to be attended
everywhere he goes, except on his yacht
Cosair or on special trains, by two dis
creet detectives Mr. Morgan Is not aware
of the presence of these men and new
officers are constantly employed in order
that he may not learn their Identity. Mr.
Morgan has several large policies on his
life. In addition so many financial Inter
ests in this eountry and abroad are deeply
Interested In the distinguished banker's
health and freedom from accident that a
pool has been formed to protect hlio la
vary $osslbU way.
time of the end of the eclipse. This will
occur for the Creighton university observa
tory at 6 o'clock 26 minutes and 3S.82 sec
onds. As the big Union Pacific whistle
blows at 6 o'clock exactly and Is generally
correct to the second, the reader will have
a fine opportunity of obtaining the correc
tion to his timepiece and of thus seeing
whether the moon Is on time. The moon
will leave the sun that is, the last contact
will occur, very near the point E on Fig.
III. WILLIAM F. BIGQE,
Prof. Creighton University Observatory.
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CHICAGO MUSICAL COLLEGE
FOUNDED 1807. DR. W. ZIEGPELD, President.
College Duildlng, 202 Michigan Dout., Chicago. Ills.
Ths largest soil most complete College of Muilo and Dramatic Art In America.
Has the strongest faculty ever assembled In a school of musical learning.
BOARD OP MU5ICAL DIRECTORSi
Dr. P. Zlsgfeld Emlle Saurct Dr. Louis Fslk Hans ran Schiller
William Castle Bernhard Uetemsna Herman Deviics Fellg Borewskl
ftrthar Speedy tWaldemar Lutschg Alexander Von Flellta fltra.O. UPen
Hart Conway, Director 5cbool sf Acting
1 All Branches of
SCHOOL OF ACTING?1 P H 1 1 0 I fl SCHOOL OF OPERA,
ELOCUTION, Itl U U I U Uodirn Lntuipi.
RECENT ACQUISITIONS TO THE FACULTYl
WALDEMAR LUTSCHO. The Ores! Russian Pianist.
ALEXANDER von P1ELITZ. The Eminent Composer.
HANS 8CHROEDER, The Distinguished Baritone.
FREDERIK FREDEKIKSEN. The Scandinavian Violinist.
EMILE 5AURET, Ths world renowned rlollnlst hat been re-engaged for a term of years.
,40th 8EASON DECIN3 SEPTEMBER llth.
ILLUSTRATED CATALOG MAILID PUCK.
( NOTK-Appllcatlont for the 45 free and 130 partial Scholarships will be receive
an til September Z.
BR0WNELL HALL OMAHA
A Home Bchool for Young Women. Advanced seminary and college preparatory
courses. Certificate admits to Vatsar, Werirsley, Mount H'olyoke, Smith, the Univer
sity jf Chicago and the University of Nebraska. Exceptional advantages In musto,
art and the modern languages. Well equpped gymnasium, tennis, field hockey and
other nut-door sports. Instructors college graduates of large teaching experience
and extended advantages In European travel. Students mothered sympathetically
by experienced women who appreciate the needs of young womanhood. Send for lUue
t rated prospectus.
ST. BERCHMANS' DAY ACADEMY
FOB YOCNO LADIBS. IKDER CARE OF SISTERS Of MKRCV.
Thorough courses In Academic, Prepa ratory and Primary departments. Kinder-
farten for little ones; Seminary for small boys. Music and Art under competent
nstructors.
SCHOOL REOPENS 8EPTEMBER 6th-
17th AND ST. MARY'S AVENUI
Western Military
Academy
Upper Alton,
Illinois.
nth year. New fireproof buildings. Modsrst
equipment. Delightful location. Numbw
limited. Strong faculty. Trorough mill
tary and academlo department. Local
references.
Col. Albert sfl. Jsekssn. A.M.. President
American
Conservatory
KIMBALL MALL
l te 2iJ Wthuk
Avt..Cklcsis.
The Uaslai attest
if Ummtmmi DMaitl Art. BiltJ mlmint
Inn I'arlvalfiS rrw ASvsntss. Teachers trsini n
ri.i.rlni.nt. Ii nlnnmi. (Tsrt I Ot'atAS. fr and DArtin
tciQnlsrehipt. Fs) I term basins Sept. 11. IS. Ontalnf ua
mulled (rw, liuu
BURN AIR-IT'S CHEAP
('tmM see narreia at sir w
vn'l sielodt, ssvss work ts4
Ke cost, wood. 4 in, sshot-se
wlok, bo vsJvss, s7 opsrstsd,
htaasosu, danbls. dull
tmmktr. o.ilok war.
'oool slthns. liOOO ""J
sa V leklcM. v si
iiM ll Air fit A
"Jto ' .klr. i RKATaST
nraDM t OR. BU V trlol onsp. An.irw w"i. ... .
World Mf OS World ,ld,. Claolasau. w.
MOKE Y MA!
tosd, all .1st, ssnt anrwhoro. SS .
IT.H. OptrtB.
Writs. FKEB
First National Bank
UNITED STATES DEPOSITORY
Omaha. Nebraska
Capital 1500,000.00
Surplus and Undivided Profits. . 1329,357.65
Deposits 9,800,.73.39
Herman KounUe, President. John A. Cwlgbton. Vic- PweitdsBt
F. H. Darts, Cash!. t
. ... nahier I I KountM. Asst-OasIjln
" 'BpacmVrur.. tems oBwd for ntU. 4
Unking accounts. Your business solicited.
Three per cent on Time Deporita.
1
$
r i
oo FOR A FEW HOURS' WORK
WE WILL PAY sio.o6'NOASH.or7oiu'boicoofs4iroBSofBu
"lbl. "-It. of nUrLJU. sues M Sowlp, llsoklnos, OuBfc Swvst
suruiMirn. utv r vsbsbs mum
SUr viuUs wUolst, BllTlTSB trot of Mr 00.1 o ny m.n, , or boj
mrt..rll irTl sss, wbo will hud out at at our W11 s;r.ertl d
oLSluTlli'r telr trtsnot pd BolsSeors. wEjoJl to tUe vsry
a . . I.I In oil r artani'Lavi fCiik i4V
bTn't onm Man j o pf t
tmm nolhlDir for fbrm; lhr r
Toa utuiuir dintu iM Iko1um wadlrol,Ml tot Ws
Sum. sswiNe iiACMiNt rthsv . j-bWs ln F.rl BoosLtf
out t . . 'ir:5LJAb.?l7TtilM UI .n r. iTsoslsl Sootlot , r.ur mm.
Heat electric light janitor service
all night and Sunday elevator ser
vice a fire proof building all cost
the tenant of The Bee Building
nothing extra.
