Fastest Passages of the more Important Steamers between New York and English Ports during the Season of 1890.[5]

NameDimensions:
Length, Breadth, Depth
DisplacementPiston
Stroke
Boiler
Heating
Surface
New York and
Queenstown
Tons.Feet.Sq. Ft.
City of Paris560 × 63 × 4313,000550,265
City of New York560 × 63 × 4313,000550,040
Majestic582 × 5712 × 591812,000540,972
Teutonic582 × 5712 × 591812,000540,972
Etruria50112 × 57.2 × 38.210,500638,817
Umbria50112 × 57.2 × 38.210,500638,817
City of Rome546 × 52 × 583411,230629,286
New York and
Southampton
Inches
Columbia480 × 56 × 389,5006634,916
Normannia520 × 5714 × 3810,5006646,490
Augusta Victoria480 × 56 × 369,5006336,000
Lahn448 × 49 × 36127,70072
NameGrate AreaSteam
Pressure
I.H.P.Fastest
Trip
Direction
New York and
Queenstown
Square FeetLbs. D. H. M.
City of Pariswas 1,293
now 1,026
15018,3505 19 18Westward
City of New Yorkwas 1,080
now 1,096
15018,1005 21 19Westward
Majestic1,15418018,0005 21 20Westward
Teutonic1,15418018,0005 19 5Westward
Etruria1,60611014,3006 6 57Westward
Umbria1,60611014,3006 3 29Westward
City of Rome1,3989011,8906 22 30Eastward
New York and
Southampton
Columbia1,22615013,6806 15 0Eastward
Normannia1,45216016,3526 17 2Westward
Augusta Victoria1,12015014,1106 22 32Eastward
Lahn1509,5007 3 0Eastward
NameMonthDistanceAverage
Speed
Average
for
Eight
Months
Fastest
Day’s
Run
during
Season
New York and
Queenstown
KnotsKnotsKnotsKnots
City of ParisAugust2,78820.0119.02515
City of New YorkOctober2,77519.6419.02502
MajesticSeptember2,78019.6419.00
TeutonicAugust2,80620.1818.84512
EtruriaJuly2,84518.8018.29481
UmbriaAugust2,83519.2018.15498
City of RomeAug.-Sep.2,78716.7316.18424
New York and
Southampton
ColumbiaOctober3,04519.1518.68492
NormanniaAugust3,04518.9118.41486
Augusta VictoriaSeptember3,04918.3117.52470
LahnOctober17.29

Note.—The nautical mile is one-sixtieth of a degree of the Equator, and is usually reckoned 6,080 feet, the statute mile being 5,280; twenty nautical miles are thus about twenty-three statute miles. The shortest distance is the arc of the great circle of the Earth passing through the two ports; any deviation from this by varying the course on account of intervening land or ice increases the distance to be run.

The crown is thus for the moment with the White Star, nor is it likely to be torn away by anything short of the tremendous effort involved in putting afloat a new, a bigger, and a more costly ship. Owners must, of course, count the cost of such rivalry and must put against the gain of say sixteen hours, in order to come to the desired five days and twenty-three knots, the cost of the thousand or twelve hundred tons more of coal which will have to be burned, the doubled number of engine and fire-room force, the larger crew, the interest on the greater investment. It is a large price to pay for a gain of so small a bit of that we generally hold so cheap—but it will be paid.

It has been impossible, of course, in a single chapter to do more than touch upon the vast changes, and their causes, which have had place in this great factor of human progress. Higher pressures and greater expansions: condensation of the exhaust steam, and its return to the boiler without the new admixture of sea-water, and the consequent necessity of frequent blowing off, which comparatively but a few years ago was so common; a better form of screw; the extensive use of steel in machinery, by which parts have been lightened, and by the use of which higher boiler-pressures are made possible—these are the main steps. But in addition to steel, high pressures, and the several other elements named which have gone to make up this progress, there was another cause in the work chiefly done by the late W. Froude, to be specially noticed as being that which has done more than the work of any other man to determine the most suitable forms for ships, and to establish the principles governing resistance. The ship-designer has, by this work, been put upon comparatively firm ground, instead of having a mental footing as unstable, almost, as the element in which his ships are destined to float.

It is not possible to go below the surface of such a subject in a popular paper, and it must suffice to speak of Mr. Froude’s deductions, in which he divided the resistances met by ships into two principal parts: the surface or skin friction, and the wave-making resistance (which latter has no existence in the case of a totally submerged body—only begins to exist when the body is near the surface, and has its full effect when the body is only partially submerged). He showed that the surface friction constitutes almost the whole resistance at moderate speeds, and a very great percentage at all speeds; that the immersed midship section area which formerly weighed so much in the minds of naval architects was of much less importance than was supposed, and that ships must have a length corresponding in a degree to the length of wave produced by the speed at which they are to be driven.

The Chilian Cruiser Esmeralda.