Eternal India
encyclopedia
Ancient Concepts, Sciences & Systems
Crosswires are stretched from north to south and from east to
west. The shadow of the intersection of these wires, falling on the
.surface of the hemisphere, indicates the position of the Sun in the
sky. Other celestial bodies can be observed directly by 'placing the
eye' at the corresponding shadow cast by the object. That is, the ce-
lestial object, the intersection of the- crosswires and the eye should
be in one straight line.
In this figure, the outer circle represents the horizon and is
graduated in degrees. From the centre, which represents the zenith
(denoted by Z), azimuth lines and altitude circles are drawn (not all
are shown). The pole P is at a point on the meridian line BD, at a
distance from the point B equal to the latitude of the place. It may be
recalled here that the latitude of the place is equal to the altitude of
the pole above the horizon of that place. The equator AEC and the
tropics fff (Capricorn), ggg (Cancer) and intermediate circles are
drawn at appropriate distances from the pole to facilitate the meas-
urement of declinations. Through the pole, hour circles are drawn.
The circles hh, ii, jj and kk are circles of the zodiacal signs, and are
drawn such that when the shadow of the interesection of the
crosswires cast by the Sun falls on any one of them, the corre-
sponding sign is on the meridian.
Only the Delhi and Jaipur observatories are fitted with a Jai
Prakash dial. The diameter of the Delhi instrument is 27.5" and that
at Jaipur is 17.10"
The Ram Yantra
is a
cylindrical
instrument
which is open at the top and
has a central pillar. The in-
side circular wall and the
floor are graduated and the
wall broken up into a se-
lected number of sections
to
facilitate
observations.
Wall sections are provided
with
notches
in
which
sighting bars can be fitted
horizontally.
This
instru-
ment also is in the Delhi
and Jaipur observatories only.
The Misra Yantra
: This is the mixed instrument and is so
named because it combines four separate instruments in one struc-
ture. Of these, the Niyat Chakra occupies the middle of the building
and consists of a gnomon with two graduated semicircles on either
side. These semicircles lie in planes inclined to the plane of the
Delhi meridian at angles of 77°16' W, 68°34W, 68°01'E and 75° 54'
E. The planes of these semicircles may be said to correspond to
meridians at places whose longitudes differ from that of Delhi by
these angles. They seem to be matching respectively with
Greenwich Observatory, Zurich Observatory a village in Japan and
a town on Pic Island in Lake Superior, Canada. However It is
obvious that these are coincidences rather than premeditated
thoughts considering the fact that the Zurich Observatory came
into existence some sixteen years after Jai Singh's death!
Of these instruments, it is claimed that Jai Singh devised the
Samrat Yantra, the Jai Prakash and the Ram Yantra. He reasoned
that the smaller brass instruments were faulty because their axes
became worn and their graduations were too small for fine meas-
urements. His remedy thus was to make large and immovable
instruments. But by doing so he unfortunately sacrificed any facility
for improvement, like adding a vernier scale, for example, for accu-
racy.
His object was the rectification of star catalogues, the calen-
dar, prediction of eclipses and so on. His scheme of astronomical
work was truly notable and his observatories form noble monu-
ments of a remarkable personality.
While Jai Singh's efforts were mainly in the northern part of
India, there are records to show that for the first time on Indian soil
a telescope was used to make stellar observations in Pondicherry,
a coastal town in South India, thirty five years before Jai Singh
founded his observatories. On December 19, 1689, Father
Richaud, a member of the Society of Jesus focussed his small
telescope towards the sky from Pondicherry and in course of time
discovered a comet as well as the binary nature of the bright star
Alpha Centauri.
Later in 1786, a private observatory was set up in Madras by
William Petrie, a small telescope being the main instrument. In
1790 the observatory was taken over by the East India Company
with one Michael Topping as the Company astronomer. In 1792 the
observatory building came up at Nungambakkam, Madras. It made
important contributions for well over a century and paved the way
for the establishment of the solar physics laboratory at Kodaikanal
in 1900.
(J.C.B.) & (G.S.D.B.)
SELECTED REFERENCES
Scientists
(Dhanvantri, Cavaka, Susruta, Varahamihira, Ar-
yabhata, Bhaskaracharya) New Delhi 1990.
D.M.Bose (Chief Ed)
A Concise History of Science
in India. New
Delhi 1971.
S.K. Biswas (Ed.) Cosmic Perspectives, Cambridge 1989.
B.V. Subbarayappa and K.V. Sarma (Eds).
Indian Astronomy. A
Source Book.
Bombay 1985.
N. Kameswara Rao, V. Vagiswari and Christina Lousis, "Father J.
Richaud and early telescope observations in India",
Bulletin of
the Astronomical Society of India
(1984).
Astronomy in Indus civilisation and during Vedic times
by A.K.
Beg and
Post-Vedic Astronomy
by S.D. Sharma in Indian Jour-
nal of History of Science, Nos-1-4 Vol. 20. Jan-Dee 1985,
Indian National Science Academy, New Delhi.
Schematic diagram for the markings on the Jai
Prakash
The Jai Prakash : This
instrument consists of two
complementary
concave
hemispheres,
situated
im-
mediately
south
of
the
Samrat Yantra. It is also
called the ’crest jewel of all
instruments'. The surface of
each hemisphere is marked
with several lines for meas-
uring the altitude, azimuth,
declination, hour angle, etc.
of any object in the sky.




