CHAPTER VIII.
ASTRONOMY AND GEODESY IN AUSTRALIA : Part 7.
By Pietro Baracchi, F.R.A.S.,
Government Astronomer of Victoria.
“The Commonwealth of Australia; Federal Handbook, prepared
in connection with the eighty-fourth meeting of the
British Association for the Advancement of Science,
held in Australia, August, 1914.”
pg.326-390. (1914)
By British Association for the Advancement of Science.
Federal Council in Australia, Australia.
Commonwealth Bureau of Census and Statistics, George Handley
Knibbs
(2) GEODESY.
(a) Trigonometrical Surveys of High Precision.
Though many careful surveys have been effected in Australia,
chiefly with a view to laud settlement, trigonometrical surveys of
high precision are, so far, confined to the three Eastern States. Of
these only a brief description will now be given.
Queensland.
The trigonometrical survey in this State extends approximately
from 26° 30′ to 29° 30′ south latitude, and
from 151° 15′ to 153° 15′ east longitude. It
comprises 74 triangles and a base line of about 7 miles in length
situated at Jondaryan. Its terminals are Mount Irving and Mount
Maria, which are respectively 216 and 162 feet above the general
level of the intervening ground.
The measurement of this base was made in 1884 by means of two
steel tapes 100 feet long, about half-an-inch broad, and 0.01 inch
thick.
These were compared with a standard bar of steel octagonal in
section 1½ inches in diameter and 10 feet long, which was kept
floating when in use in a trough of mercury, with thermometers
plunged in it for obtaining the temperature of the bar. This bar was
compared in 1883 with the New South Wales Standard Bar 0.I.4, which
gave its standardised length at 62° F. as 9.9998581 feet, which
value was adopted throughout the operations of the trigonometrical
survey.
In the base measurements the two tapes were placed “in wooden troughs and shaded by a board, a
tension of 20 lbs. was applied by means of a spring balance, and five
thermometers, whose index errors had been determined by comparison
with a standard thermometer, were used along each 100 feet of tape.
The troughs were supported upon pegs driven in the ground and set on
even grade by means of a levelling instrument. Marks were made in
copper discs inserted in the pegs at each hundred feet, the distance
between the tape ends and the marks being measured by micrometer
microscopes.
Ten sections, the six central ones averaging nearly 1 mile and the
other two at each end being nearly half-a-mile mile long.
The terminal points of these sections were marked by stones sunk
into the ground and set in concrete. Each stone had a metal plug,
upon which a small mark was made denoting the terminal point of the
section.”
Three measurements were made with each tape, giving six
independent values.
The two sets of three values made with each tape gave two mean
results, which showed a difference of 0.117″ inches.
Ten-inch theodolites (Everest pattern), by Troughton and Simms,
provided with micrometer microscopes reading to one second of arc,
were generally employed on the survey, and a 12-in. altazimuth was
used at a few stations. The angular measurements were
obtained from two to eight readings made on each of eleven positions
of the circle. The closing errors were within 1″ for 29
triangles, from 1″ to 2″ for 29 other triangles, from
2″ to 3″ for 11 triangles, and upwards of 3′ for
the remaining 5 triangles. The greatest closing error was
3.90″, and the average 0.95″.
“The astronomical datum is the
position of the station at Jimbour as determined by Captain Morris,
R.E., and Lieut. Darwin, R.E., in 1882,” while they occupied this station for the
observation of the transit of Venus. [pg.376]
The longitude was determined by direct exchange of time signals
with the Sydney Observatory by telegraph. In deducing from this datum
the latitudes and longitudes of the trigonometrical stations, the
elements used by Colonel James in the Ordnance Survey of Great
Britain, in 1858, were adopted.
The azimuth datum was determined by astronomical observations made
with a 20-in. transit instrument at Bloodwood, this being the apex of
one of the triangles standing on the base line.
Astronomical observations for latitude and longitude were also
made at several stations.
A comparison of the astronomical with the geodetic values for the
four stations of Bloodwood, Brisbane, Haystack, and Mount Domville
gives the following differences respectively. (40)
Latitude (geodetic − astronomical)
−02″; +1.17″; +5.37″; −1.17″.
Longitude (geodetic − astronomical)
+6.57″; −0.05″.
A minor triangulation of the City of Brisbane was carried out in
1890.
The principal triangulation was discontinued in 1891.
Victoria.
The preliminary work of clearing mountain tops for a
trigonometrical survey of the State of Victoria was commenced in 1853
under Captain Andrew Clark, R.E., after his appointment as
Surveyor-General of Victoria, as already mentioned ; but the primary
triangulation was not actually commenced till seven years after.
In 1860 a base line was laid down on the Werribee Plains about
4.942 miles in length, which was subsequently extended by
triangulation to a further length of 5.651 miles, making a total
distance between the terminal points 10.593 miles.
“Each end of the measured base was
defined by a solid mass of masonry built 5 feet into the ground,
capped by a heavy stone with gun-metal plug and platinum centre, on
which the terminal dot was marked. A heavy protection stone was
placed over the cap stone, and this was surmounted by a timber
pyramid, with pinnacle accurately centred over the platinum
point.” (41)
The measurement of this base was made by three iron bars 10 feet
long and 1 inch square, with the ends turned round for about 4 inches
in length, one end of each bar being finished quite flat and
polished, and the other end being a segment of a sphere of 5-ft.
radius, also polished. They were encased in wooden troughs 6 inches
square, with hinged tops cut in three sections for the convenient
examination of the three thermometers resting on each bar, the steel
ends only being freely exposed 2½ inches out of the case.
The lengths of these bars were compared with due care “with a 10-ft. ordnance standard lent by the
New South Wales Government” (40) and
verified later by a similar standard obtained by the Government of
Victoria from the Ordnance Survey Department of England.
In the actual measurement the bars were supported on pine trestles
fitted with brass sockets on their top frames to receive a brass
tripod. These frames carried a brass “camel,”
provided with the requisite fittings for bringing the ends of the
bars accurately into juxtaposition. The three bars were placed in
series with distances of about ¼ inch between the spherical
[pg.377] end of one and the flat end of another, and the distance
between the two was obtained by passing between them a graduated
wedge of hard bell-metal 7 inches long and 2 inches broad, with faces
inclined at angle of one-half a degree.
The difference of level between the terminal of the base being
only 14 feet, and the intervening ground being fairly flat, the bars
were adjusted by levelling into a horizontal position throughout the
measurement.
A part of the southern portion of this base was re-measured to the
extent of 2.11 miles, and the difference between the two results was
found to be 0.308 inches, which was sufficiently small “ to justify the assumption that by the
original measurement the Werribee base was probably as accurate as
any measured up to that time.” (40)
The lengths of this base are as follow :—
(41) Measured base 26091.82 feet Extension by triangulation to
Green Hill terminal 29839.83 Total length 55931.65
The instruments used for angular observations were an 18-in.
altazimuth, by Troughton and Simms, and a 13-in. theodolite, by
Ertel, both being provided with micrometer microscopes by which the
circles were read to 1″ ; two 12-in. theodolites read by
micrometer microscopes to 4″ and 10″ respectively ; a
10-in. altazimuth and other theodolites of smaller size.
The triangulation was expanded in a decade throughout the extent
of the Colony south of the 36th parallel of south latitude.
In this survey 209 stations of the first order, 267 of the second
order, and a larger number of subsidiary points were connected and
marked.
An average number of 170 observations were made at each of the
primary stations to determine their positions. The triangulated area
is about 70,000 square miles. It was intended to measure a
very suitable base of verification to the westward of Mount Gambler
and Mount Schanck, in South Australia, these being the extreme
western points connected with Victorian triangulation, but the work
was not carried out.
A portion of the boundary line between the States of New South
Wales and Victoria is a straight line running from a point near the
source of the Murray River to Cape Howe on the east coast. The
terminals of this line were agreed upon in 1870, and in order to
determine their geographical co-ordinates with all possible accuracy,
they were connected with the primary triangulation which was, for
this purpose, extended to “The
Pilot” and Mount Kosciusko, in New
South Wales, these being the extreme eastern points of the
survey.
The true azimuth of the line having been deduced by calculation
from the co-ordinates of the terminal points, the line was ranged on
the ground to the computed bearing and marked in 1872, starting from
one marked terminal, and reaching the coast to within 17 inches of
the other marked terminal.
The line was run by Messrs. A. C. Allen and A. Black, and the
result is a fitting tribute to their skill, energy, and endurance in
the accomplishment of an exceedingly difficult undertaking with such
a remarkable success. [pg.378]
Colonel Clarke’s elements of the
figure of the earth were used in working out the results of the
Victorian survey.
New South Wales.
The territory of this State extends from the Murray River to the
29th parallel of south latitude, and from the eastern coast westward
to the 141st meridian of east longitude.
About one-fourth of its whole area has been covered with a
trigonometrical survey of high precision, which was initiated in
1867, carried on for a few years, suspended for some time, resumed in
1891, continued since over an extent of 43 million acres, and still
progressing.
The base line of this survey, 5½ miles in length, is
situated at Lake George, and a verification base of about 7 miles was
laid down and measured at Richmond.
The survey comprises 119 stations of the first order, 583 of the
second order, and 1,380 of the third order, all of which have been
very substantially and permanently marked and connected, and whose
geodetic co-ordinates are accurately known.
Some 490 additional stations have been piled and prepared for
observation, of which 15 are to be ranked as first order, 75 second
order, and 400 third order stations.
The stations of the first order constitute the primary skeleton of
the survey, being a net of fundamental triangles whose sides range
usually from 35 to 40 miles in length.
Astronomical observations for azimuth, latitude and longitude were
made at many of these primary stations.
The second order stations are distributed at distances varying
from 15 to 20 miles, this being the average length of the sides of
the secondary triangles. These stations were connected by actual
observations made upon them with smaller instruments than those used
at primary stations, but with sufficient precision to meet all the
practical requirements of a triangulation for the purpose of accurate
mapping. No astronomical observations were made at these
stations.
The sides of triangles connecting stations of the third order are
from 7 to 10 miles. The positions of these stations were fixed by
intersections based on observations made from surrounding stations of
higher order, and their accuracy is sufficient for connecting all
chain surveys on a uniform system.
The original base on Lake George was laid down and its measurement
commenced in 1868, under the superintendence of Mr. G.R. Smalley, but
it was abandoned before completion owing to an abnormal rise of the
water of the lake, which covered parts of the line to a depth of 2
feet.
A new site for the base was selected in 1870 by Mr. P.F. Adams,
the Surveyor-General at the time, under whose direction the
measurement of its length was made twice by Mr. A.C. Betts.
The adopted standard of length was that of “Standard Bar 0.I.4.” referred to at p.175 of Colonel Clarke’s work on the comparison of standards
published in 1866. (41)
This bar is of cast iron, 10 feet in length, the length being
defined by microscopical dots marked near its ends. It is encased,
and fitted with [pg.379] adequate support to prevent flexure, and
provided with thermometers and micrometer microscopes for the
observation of its marks. It was obtained many years before from the
Board of Ordnance in England.
The actual measurement of the base was made with three 10-ft. bars
of pine wood, encased and evenly supported, in wooden troughs 6
inches by 6 inches, and a little less than 10 feet in length, so as
to allow a short portion of the ends of the bars to project outside.
The ends were fitted with small brass plugs, upon each of which a
terminal microscopic dot was marked, the distance between the
terminal dots being the actual length of the bar. These lengths were
standardised each morning and evening during the progress of the work
by comparison with the Standard Bar 0.I.4.
Each trough was supported on two “camels”
provided with vertical, lateral, and longitudinal motion by means of
which the three bars could be accurately placed in series along the
line with the terminal dots of adjacent bars arranged in close pairs,
always at the same distance, leaving a small constant amount of free
space between the bars. This adjustment was made by means of a double
microscope attached to the leading end of each trough. The microscope
consisted of a single tube with two objectives at one end, rigidly
mounted side by side, and two parallel webs, fixed on a diaphragm, at
the upper end of the tube in the common focal plane of the
objectives. By adequate means of adjustment the pair of dots could be
brought in the fields of view and adjusted so as to bring each image
into accurate bisection with each respective wire. The adjustment for
parallelism of the optical axes and the distance between the webs
having been previously ascertained, it was assumed that a constant
distance between the adjacent bars was maintained throughout the
measurement.
“The difference between the length
of this base as found from the measurement and re-measurement was
0.542 inches in the total length of 5½- miles.”
The verification base at Richmond was measured in 1879-80 by Mr.
Conder twice. The first measurement was made with the same
three pine bars with which the Lake George base was measured, and in
the second three 10-ft. rods of steel 3/8 of an inch in
diameter were used. These rods were wrapped in blankets, and encased
in wooden troughs with glass windows for inspection of the attached
thermometers. The arrangement of terminal dots, the auxiliary
apparatus for support, adjustment, and observations, and the methods
employed in carrying out the work were in every respect similar for
both sets of bars, and throughout the base operations at Lake George
in 1870 and at Richmond in 1879-80. The length of both sets of bars
was again standardised by daily comparison morning and evening with
the same standard as adopted in 1870, namely, the Ordnance Bar
0.I.4
The results of the two measurements were as follow :—
By pine bars |
36989.33651 feet |
By steel rods |
36989.39166 feet |
Difference |
0.05515 = 0.662 inches< |
“The combined error of measurement
of the two bases and of the intervening triangulation produced an
apparent discrepancy of only If inches in the length of the Lake
George base. The bases were assumed to be correct, [pg.380] and an
adjustment of the triangles was made in order to eliminate this
small apparent difference.” (40)
The instruments employed in astronomical observations and angular
measurements were as follow :— Two altazimuth
instruments by Troughton and Simms, with object glasses of 3-in.
aperture, provided with filar micrometer and delicate levels for
latitude determinations by the Talcott method ; circles read by four
micrometer microscopes to 1″. All observations,
astronomical and geodetical, were made with these instruments at the
primary stations.
Theodolite by Troughton and Simms, object glass
2½−in. aperture and 26 inches focal length, horizontal
circle 10 inches in diameter read by two micrometer microscopes to
1″, and two parts of a vertical circle 10 inches in diameter
reading by vernier to 5″. Observations at second order
stations, and all vertical angles for the determination of relative
heights, were made with this instrument.
Recently a 10-in. Repsold theodolite, of the same pattern as that
used in the trigonometrical survey of South Africa, was procured,
and is intended to be employed in the future in place of the heavier
18-in. altazimuth. The observed directions from a primary
station to another station of the first and second order depended on
twenty pointings made in reversed positions of the instrument.
The number of pointings was reduced to ten for second order
stations, and to five for stations of the third order.
The great accuracy of these observations is shown by the
following statement of the closing error of triangles. In 171
triangles in which all angles have been observed with the large
altazimuth the closing error is 0.70″.
In 235 triangles, with two angles only observed with the larger,
and one angle observed with the smaller instrument the average
closing error is 1.15″.
In 245 triangles, in which only one angle was observed with the
18″ alt-azimuth, and the other two with the 10″
theodolite, the closing error is 1.29″. In 173
triangles, with all the angles observed with the smaller instrument
the closing error is 1.30″. The probable value of the
average closing error of the triangles, computed according to
General Ferrero’s formula, for the
primary triangulation of New South Wales is 0.54″, which is
less than the error similarly computed for the great trigonometrical
surveys of Great Britain, India, and most of the other countries,
and the closing error for triangles observed with the smaller
instruments is, on the same criterion, reduced to 1.00″.
Astronomical observations for latitudes were made at 74 stations
with the 18″ altazimuth by the Talcott method.
Azimuth was determined at 66 stations by meridian observations of
circumpolar stars, made with the same instrument.
The longitude of 10 primary stations, and of 29 other important
places in the State, were determined by the direct exchange of clock
signals with the Sydney Observatory.
For the calculation of geodetic latitudes and longitudes, the
co-ordinates of the Sydney Observatory adopted as the datum were :
— Latitude 33° 51′ 41.1″ ; longitude
141° 12′ 23.1″. [pg.381]
The elements of the figure of the earth adopted in the
calculations of the survey are those of a spheroid with—Major
axis a = 20923134 feet ; polar c = 20853429 feet.
Minor triangulations have been made around such important centres
of the State as Sydney, Albury, and Newcastle, which were afterwards
connected with the primary system.
Since the expansion of the geodetic survey of this State from the
Lake George base in 1876, the principal observers in charge of the
work were Messrs. W. J. Condor and J. Brooks. It was the former who
set the high standard of accuracy which was worthily maintained by
the latter.
Mr. T. F. Furber has been Director of the Survey for many years,
and to him is due much of the credit of having planned means and
methods by which this important undertaking has been brought to its
present state of general efficiency and exemplary precision.
Mr. Furber, in his valuable paper (40) from which the information
required or the above account was mainly drawn, mentions the names
of P. F. Adams, late Surveyor-General, “to whom the very existence of the survey is
in a large measure due,” and the late
H. C. Russell, who, during the whole progress of the survey, aided
in many ways where his scientific attainments were of the greatest
service.
In May, 1912, a Conference was held in Melbourne at which the
Director of Commonwealth Lands and Surveys, the Surveyor-General,
and the Government Astronomer of New Zealand, and the
Surveyors-General of the Australian States met to discuss, among
other things, the question of a Geodetic Survey of Australia.
The following resolutions bearing on this matter were passed by
the Conference :—
(41) “That, in the
opinion of this Conference, it is desirable that a Geodetic Survey
of Australia should be undertaken.
“ That, in order to
give effect to the foregoing resolution, this Conference
respectfully recommends that such survey be undertaken by the
Commonwealth Government, and submits in support thereof the
following reasons :—
“ (a) That the time has
arrived when the Commonwealth should take its place in the
scientific investigations of the world, not the least important of
which are the determination of the figure of the earth, its density,
and other cognate matters.
“ (b) That work of this
character, involving the highest form of survey should be effected
under the supreme authority of Australia, as it is essential that it
should be carried out with the greatest degree of accuracy on a
uniform basis and a definite plan the individual parts being
co-ordinated and eventually forming one homogeneous whole.
“ (c) That the system
which has hitherto prevailed by which the individual States carried
out this work with instruments of varying character has resulted in
divergent standards of accuracy, rendering the work to a great
extent unsatisfactory, and, though much of it is of high grade,
portions of it are impossible of reconciliation and co-ordination
with a continental scheme. [pg.382]
“ {d) That the
desirableness of this work being undertaken by the Commonwealth
Government is evidenced by the fact that the Geodetic Survey of the
United States is carried out under the direct control of the Federal
Government, and that the South African Geodetic Survey is also under
one central control.
“ (e) That such survey
is absolutely necessary for the production of accurate maps, will be
of high value in connexion with cadastral and geological surveys,
and form a basis for topographical work for defence and other
purposes. It will, moreover, provide a standard of accuracy for
surveys of every description throughout the Commonwealth.
“ (f) That it will
afford an invaluable base to which settlement surveys already
effected can be connected, providing data for reestablishing
boundaries, which, with increasing density of settlement, becomes a
matter of great importance. Further, as regards the sparsely
occupied areas of Australia, such a survey, if carried out in
advance of settlement, will be of the greatest utility and
assistance in effecting the settlement surveys which can at any
future time be reproduced with a minimum error and at a relatively
low cost, preventing litigation consequent upon other methods.”
It is earnestly to be hoped that the Commonwealth Government will
sanction the recommendations of this Conference, and that the
proposed undertaking may be carried out, so as to enable Australia
to furnish in due course a contribution which should prove itself to
be one of the greatest value and importance for the advancement of
modern geodesy.
(b) Pendulum Observations.
Determinations of the gravitational value of “g”
have been made in Australia at various times by different observers,
since the early years of the nineteenth century, generally, by
differential methods based on the swings of pendulums of the “invariable”
type, and, in one case, by the actual measurement of a “second’s
pendulum” of the reversible or
Bessell’s type.
The earliest gravimetric observations made in Australia seem to
be those of the French Expedition under Freycinet, who swung three
pendulums at Sydney in 1819, and the latest are those of Dr. Wright,
of Canada, which he made at Melbourne in April of this year (1913)
on his return from Scott’s Antarctic
Expedition.
During this period of 95 years, the value of “g” has
been determined at all the capitals of Australasia one or more times
independently, forming a series of 24 results, 9 of which are for
Sydney, 7 for Melbourne, 1 for Brisbane, 1 for Perth, 1 for Hobart,
4 for New Zealand, and 1 for Campbell Island.
The whole of this work has been discussed by the International
Geodetic Association, and a summary of it, with brief descriptions
of the observations made, apparatus employed, and estimated probable
error of each result, is published in the Reports of the 13th, 14th,
15th, and 16th Conferenz der internalionalen Erdmessung, from
which the appended table is taken. The table shows, by the
satisfactory agreement of the values obtained by several observers
at different times, that the gravitational constant “g” has
been well ascertained for the Australian stations. [pg.383]
DETERMINATION IN
AUSTRALIA OF THE VALUE OF “g”
REDUCED TO THE POTSDAM
SYSTEM.
Station. |
Latitude. |
Longitude. |
Height. |
g |
Observer. |
Year |
go′ |
γ |
go′ −
γo′ |
Campbell Island |
−52° 33.7′ |
169° 9′ |
(2?) |
981.238 |
Boquet de la Grye |
1874 |
981.239 |
981.293 |
−54 |
Christchurch |
−43° 31.8′ |
172° 38.2′ |
8 |
981.238 |
Bernacchi |
1901, 1904 |
980.514 |
980.483 |
+31 |
Auckland |
−36° 51.9′ |
174° 47′ |
80 |
979.938 |
Pritchett |
1882 |
979.955 |
979.890 |
+65 |
Auckland |
−36° 50.9′ |
174° 46.2′ |
3 |
979.962 |
von Elblein |
1893 |
979.963 |
979.888 |
+75 |
Doubtless Bay |
−34° 59.3′ |
173° 29′ |
7 |
979.839 |
Klotz |
1903 |
. . |
979.729 |
. . |
Hobart |
−42° 53.6′ |
147° 22.0′ |
58 |
980.441 |
Budik |
1897 |
980.453 |
980.425 |
+28 |
Melbourne Mont Pellier Par. |
−37° 49.9′ |
144° 59′ |
18 |
980.032 |
Neumayer |
1863 |
980.036 |
979.974 |
+62* |
Melbourne Observatory |
−37° 49.9′ |
144° 58.5′ |
26 |
979.991 |
von Elbein |
1893 |
979.996 |
979.974 |
+22 |
Melbourne Observatory |
−37° 49.9′ |
144° 59′ |
26 |
979.991 |
Baracchi |
1893 |
979.998 |
979.974 |
+24 |
Melbourne Observatory |
−37° 49.9′ |
144° 58.5′ |
26 |
979.997 |
Guberth |
1894 |
980.002 |
979.974 |
+28 |
Melbourne Observatory |
−37° 49.9′ |
144° 58.5′ |
23? |
979.985 |
Bernacchi |
1904 |
979.976 |
979.974 |
+ 2 |
Melbourne Observatory |
−37° 49.9′ |
144° 58.5′ |
27 |
979.990 |
Hecker |
1904 |
979.998 |
979.974 |
+16 |
Melbourne Observatory |
−37° 49.9′ |
144° 58.5′ |
27 |
979.985 |
Alessio |
1905 |
979.990 |
979.974 |
+16 |
Sydney |
−33° 51.6′ |
151° 13′ |
33 |
979.716 |
Freycinet |
1819 |
979.723 |
979.634 |
+92 |
Sydney Fort |
−33° 51.6′ |
151° 13′ |
6 |
979.693 |
Duperrey |
1824 |
979.694 |
979.634 |
+60 |
Sydney Observatory |
−33° 51.7′ |
151° 12.7′ |
43 |
979.687 |
Pritchett, etc. |
1882, 1894 |
979.695 |
979.634 |
+61 |
Sydney Observatory |
−33° 51.6′ |
151° 12.4′ |
43 |
979.678 |
von Elblein |
1893 |
979.687 |
979.634 |
+53 |
Sydney Observatory |
−33° 51.6′ |
151° 12.4′ |
43 |
979.698 |
Guberth |
1894 |
979.707 |
979.634 |
+73 |
Sydney Observatory |
−33° 51.6′ |
151° 12.4′ |
43 |
979.686 |
Budik |
1896 |
979.695 |
979.634 |
+61 |
Sydney Observatory |
−33° 51.6′ |
151° 12.4′ |
43 |
979.674 |
Budik |
1897 |
979.683 |
979.634 |
+49 |
Sydney Observatory |
−33° 51.6′ |
151° 12.4′ |
43 |
979.681 |
Hecker |
1904 |
979.690 |
979.634 |
+36 |
Sydney Observatory |
−33° 51.7′ |
151° 12.7′ |
43 |
979.675 |
Alessio |
1906 |
979.684 |
979.634 |
+50 |
Brisbane |
−27° 28.0′ |
153° 1.6′ |
40 |
979.148 |
Budik |
1896 |
979.160 |
979.129 |
+27 |
Perth |
−31° 57.1′ |
115° 50.5′ |
58 |
979.374 |
Alessio |
1905 |
. . |
. . |
. . |
* This value is without doubt erroneous, and should not be
used.
[pg.384] The values in the table are from Bericht über die
relativen Messungen der Schwerkraft mit Pendelapparaten in der Zeit
von 1808 bis 1909 E. Borrasa Verhandlungen 16ten allgemeinen
Conferenz der internationalen Erdmessung.
In the table “g” is the observed value reduced to the
Potsdam system.
Writing φ the latitude,
H the height in metres, θ the density of the local earth
formation, g′−g the topographical
reduction, then
go = g +
3086×10-7 H the value reduced to sea-level.
go′ =
go + [3θ / 4
× 5.52] (g−go) +
g′−g the value corrected for the
protuberant earth,
γo =
978.030 [1 + 0.005302 sin2 &minus 0.00007 sin2
2φ] the value computed from
Helmert’s formula. go′ − γo = the gravitational
anomaly.
I am indebted to the Government Astronomers and Surveyors-General
of the Australian States for supplying me with accounts of the work
of their respective departments ; to Professor Ernest Scott and Mr.
H. Wright for interesting historical notes on the astronomical work
of early navigators ; to Messrs. J. Tebbutt, C. J. Merfield, W.
Gale, and H. Wright for information in regard to amateur astronomy ;
to Dr. J. M. Baldwin for arranging the results of pendulum
observations ; to Mr. J. A. Maroney for preparing the list of papers
in Appendix B, and for giving valuable assistance in looking up
authorities ; and to some others who have helped me in various ways.
To all of these I tender my sincere thanks.
The length of the original article far exceeded the limits of
space prescribed by the Editor, and owing to my inability to deal
with the difficulty. Dr. E. F. J. Love undertook the heavy and
troublesome task of reducing to its present size, for which I am
very greatly obliged to him.
Last Update : 18th October 2014
Southern Astronomical Delights ©
(2014)
For any problems with this Website or Document please e-mail me.
|