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‘Meghnad Saha’s place in the history of astrophysics
and in the history of modern science in India is unique’, wrote
Subrahmanyan Chandrasekhar (1910-95). Saha’s theory of thermal ionisaiton,
which explained the origin of stellar spectra, was one of India’s
most important contributions to world science during the 20th century.
It was an epoch-making discovery. Arthur Stanley Eddington (1882-1944),
while writing on stars in the Encyclopaedia Britannica, described
Saha’s theory of thermal ionisaiton as the twelfth most important
landmark in the history of astronomy since the first variable star
(Mira Ceti) discovered by Saha made important contributions in different
branches of physics. Saha (jointly with B.N. Srivastava) wrote the
renowned textbook, entitled, Treatise on Heat, which was originally
published in 1931 under the title, A Text Book on Heat. It was Saha
who first started the teaching and training in nuclear physics in
the country. The first cyclotron in the country was built with Saha’s
initiatives. Saha was a great institution builder. Among the institutions
that he built were: National Academy of Sciences, India, at Allahabad,
Indian Physical Society, Kolkata, National Institution of Sciences
of India (which was later renamed Indian
National Science Academy), New Delhi, Indian Science News Association,
Kolkata, and Saha Institute of Nuclear Physics, Kolkata. Saha was
an active member of the National Planning Committee constituted
by the Indian National Congress in 1938 with Jawaharlal Nehru as
its Chairman. He was the Chairman of the Indian Calendar Reform
Committee constituted by the Council of Scientific and Industrial
Research in 1952. He was an elected Independent Member of the Indian
Parliament. He advocated large-scale industrialisation for social
development.
Meghnad Saha was born on October 06, 1893 in
the village of Seoratali in the Dhaka (then Dacca) district (now
in Bangladesh) of undivided India. He was the fifth child of his
parents, Jagannath Saha and Bhubaneswari Devi. His father, Jagannath,
was a petty shopkeeper. Given their social and economic background
his parents had neither the means nor the inclination for educating
their children beyond the primary education. Saha’s elder brother
Jainath, after failing to pass the matriculation examination, started
working in a jute company on a monthly salary of Rs.20. His second
brother had to discontinue his school education in order to help
his father in running the shop. At the age of seven Saha joined
the village primary school and from the very beginning he demonstrated
an unusual aptitude for learning.
Radharani Saha, wife of Saha,
After the completion of his primary education there
was no certainty that his education would continue further. Their
parents would have preferred to have him work in the family’s grocery
shop. In any case they did not see any use of further education
in running the shop. Moreover there was no middle school nearer
to his village. The nearest middle school was at Simulia, which
was 10 kms away from his village. Saha’s parents did not have the
means to take care of the expenses of his boarding and lodging.
At this stage his elder brother Jainath came in his rescue by locating
a sponsor in Ananta Kumar Das, a local doctor. The kind-hearted
doctor agreed to provide Saha free boarding and lodging in his house
provided Saha washed his own plates (a condition that reflected
the prevailing rigid caste system) and attend minor household works
including the taking care of the cow. Saha readily accepted all
the conditions as he had a strong urge to continue his studies further.
Every weekend he used to visit his village. When the village became
flooded he would row all the way, otherwise he would simply walk
down. Saha completed his middle school by topping the list of successful
candidates in the entire district of Dhaka. As a result he secured
a scholarship of Rs.4 per month. In 1905 Saha came to Dhaka, where
he joined the Collegiate School, a government school. His elder
brother sent him a monthly allowance of Rs.5, it was indeed a great
sacrifice on his part, as his total monthly salary was Rs.20. The
Purba Banga Baisya Samiti gave another Rs.2 per month. So Saha had
Rs.11 to manage his food, lodging and other expenses.
There were widespread political disturbances in
Bengal in 1905. In this year Lord Curzon, the then Viceroy of British
India, had decided to partition Bengal. Saha, like many others,
was affected by this political upheaval. He, along with some other
students, were rusticated from the Collegiate School, because of
their participation in the demonstration against the visit of the
Bengal Governor, Sir Bamfylde Fuller, to the school. It is not certain
whether Saha actually participated in the demonstration or not,
because there is another version of the story. According to this
version, Saha did not take part in the demonstration. On that fateful
day as usual he had gone to school barefooted. For Saha it was a
usual practice, as he had not enough money to buy shoes. But on
that day the authorities took it as a deliberate insult directed
against the Governor. Besides being rusticated Saha was deprived
of his scholarship. Fortunately a private school, named Kishori
Lal Jubilee School, accepted Saha with a free studentship and a
stipend. In 1909 Saha passed the Entrance Examination from Kishori
Lal Jubilee School standing first amongst all the candidates from
erstwhile East Bengal.
In school Saha’s favourite subject was mathematics
and he also liked history. He was particularly fond of reading Todd’s
Rajasthan. He used to be fascinated by the heroic tales of Rajput
and Maratha warriors. Among his favourite books were Rabindranath
Tagore’s Katha O Kahini, which glorifies the values of the Rajput
and Maratha warriors and Madhusudan Dutt’s epic poem Meghnad Badh.
During his school days Saha also attended the free Bible classes
conducted by the Dhaka Baptist Mission. He stood first in one of
the competitive examinations of Bible conducted by the Mission and
received a cash prize of Rs.100.
After passing the Intermediate Examination of the
Calcutta University in 1911 from the Dhaka College, Dhaka, Saha
joined the Presidency College at Kolkata (then Calcutta). Among
his classmates was Satyendranath Bose, of the Bose-Einstein Statistics
fame. Prasanta Chandra Mohalanobis, the founder of the Indian Statistical
Institute, was his senior by a year. His teachers included Prafulla
Chandra Ray in chemistry and Jagadis Chandra Bose in physics. Saha
passed his BSc Examination with Honours in Mathematics in 1913 and
MSc (Applied Mathematics) Examination in 1915. Saha stood second
in order of merit in both the examinations. The first position in
both cases went to S.N. Bose.
With President Rajendra Prasad
Saha was appointed lecturer in the Department of
Applied Mathematics in 1916 in the University College of Science.
The foundation stone of the University College of Science was laid
down on 27 March 1914 just four days before Asutosh Mookerjee laid
down his office as Vice Chancellor of the University. It may be
noted here that Mookerjee who was the Vice Chancellor of the Calcutta
University during 1906-14 and then again during 1921-23. Both Saha
and S.N. Bose, who also joined the Department as a lecturer, got
themselves transferred to the Physics Department, where a year later
C.V. Raman joined as Palit Professor of Physics. After joining the
physics department Saha started giving lectures to the post-graduate
classes on topics like hydrostatics, the figure of the Earth, spectroscopy
and thermodynamics. For teaching physics to the postgraduate classes,
Saha had to learn it himself first, as he studied physics only in
the undergraduate classes. It was a great challenge indeed. Besides
teaching Saha also started doing research. It was not an easy task.
In those days there was no experimental laboratory in the Department
of Physics of the University College of Science. He had only one
‘research facility’ that is the wellequipped Library of the Presidency
College. Saha had no guide for supervising his research work. He
totally depended on his knowledge acquired from private studies.
During this period Saha did not have enough money to pay for publication
of his research paper in foreign journal. To quote Saha :
“By the end of 1917, I had written a long essay
on `Selective Radiation Pressure’ elaborating on theory of the role
of radiation pressure’ acting on the atom selectively and compensating
the action of gravity on solar atoms. This paper was sent to the
Astrophysical Journal for publication, but the editors replied that
as the paper was rather long, it could be published only if I were
willing to bear a part of the printing costs which ran to three
figures in dollars. Much as I would have liked to do so, it was
not possible me to find out so much money as my salary was small
and I had to maintain my old parents and a younger brother who was
studying within this salary. So I wrote to the editors of the Astrophysical
Journal expressing my inability to pay the costs of printing, but
never heard anything more about the publication of this paper nor
was it returned to me. Years afterwards, in 1936, when I visited
Yerkes Observatory, Dr. Morgan showed me the manuscript which was
still being kept there. I got a short note published in the Astrophysical
Journal, Vol. 50,220 (1919) and submitted a duplicate of the original
article on `selective radiation pressure and problem of solar atmosphere’
( Journal of the Department of Science, Calcutta University, 1919)
sometime afterwards for publication in our own university journal
which had no circulation worth mentioning. I am mentioning these
facts because I might claim to be the originator of the Theory of
Selective Radiation Pressure, though an account of above discouraging
circumstances, I did not pursue the idea to develop it. E.A. Milne
apparently read a note of mine in Nature 107, 489 (1921) because
in his first paper on the subject `Astrophysical Determination of
Average of an Excited Calcium Atom, in Month. Not. R. Ast. Soc.,
Vol.84, he mentioned my contribution in a footnote, though nobody
appears to have noticed. His exact words are: `These Paragraphs
develop ideas originally put forward by Saha’.”
Initially Saha worked on diverse topics as reflected
from the titles of his published research papers as indicated below:
-
“On Maxwell’s Stresses” ( Philosophical Magazine, 1917), this
paper was based on his studies of the electromagnetic theory
of radiation;
-
“On the Limit of Interference in the Fabry-Perot Interferometer”
( Physical Review, 1917),
-
“On A New Theorem in Elasticity” ( Journal of the Asiatic Society,
Bengal, 1918),
-
“On the Dynamics of the Electron” ( Phil. Mag. 1918)
-
“On the Pressure of Light” ( Journal of the Asiatic Society,
Bengal, 1928)
- “On
the Influence of Finite Volume of Molecules on the Equation
of State” ( Phil. Mag , 1918). This paper was jointly written
with S.N. Bose.
-
“On the Mechanical and Electro-dynamical Properties of the Electron”
( Physical Review, 1919);
-
“On the Radiation Pressure and the Quantum Theory” ( Astrophysical
Journal, 1919);
-
“On the Fundamental Law of Electrical Action” ( Phil. Mag. 1919).
Based on his above work Saha submitted his thesis
for the degree of Doctor of Science of the Calcutta University in
1918. He was awarded the degree in 1919. The same year he was awarded
the Premchand Roychand Scholarship for his dissertation on the ‘Harvard
Classification of Stellar Spectra’. While working on diverse topics
he was also preparing for his main work in astrophysics. For this
work he profited from reading Agnes Clarke’s two popular books on
astronomy and astrophysics. He had also read Planck’s Thermodynamics
and Nernst’s Das Neue Warmestaz and research papers of Niels Bohr
and Arnold Sommerfeld on the quantum theory of atom. He published
four papers on his astrophysical research in the first six months
of 1920 in the Philosophical Magazine viz. “Ionisation of the Solar
Chromosphere” (March 04, 1920), “On the Harvard Classification of
Stars” (May 1920), “On Elements in the Sun” (22 May 1920) and “On
the Problems of Temperature-Radiation of Gases” (25 May 1920). In
these papers Saha formulated his Theory of Thermal Ionisation. His
thesis on the ‘Origin of Lines in Stellar
Spectra’ won him the Griffith Prize of the Calcutta University in
1920.
It is interesting to note here that Saha, jointly
with S.N. Bose prepared an English translation of Einstein’s papers
on theory of relativity and got it published in a book form. Incidentally
their translation of Einstein’s work on the theory of relativity
happens to be the first on record. Chandrasekhar wrote : “…In 1919,
only three years, after the founding of the general theory of relativity,
Saha and S.N. Bose should have taken the time and the effort to
translate and publish Einstein’s papers which have since become
epochal. At a celebration of the Einstein centennial at Princeton
University, three years ago, reference was made to a Japanese translation
of Einstein’s papers as the first on record and I was glad that
I was able to correct the impression. A Xerox copy of the Saha-Bose
translation is now in the Einstein Achieves at Princeton”.
The Premchand Roychand Scholarship of the Calcutta
University awarded in 1919 enabled Saha to spend about two years
in Europe. He first went to London where he spent about five months
in the laboratory of Alfred Fowler (1868-1940). From London he moved
to Berlin where he worked in Walther Nernst’s Laboratory.
For a long time after Saha published his work on
thermal ionization theory, the European scientific community used
to believe that Saha did this work under the supervision of Albert
Fowler. For example in 1972 while commenting on Saha’s paper on
the ionization in the solar chromosphere, A.J. Meadows in his biography
of Sir Norman Lockyer wrote : “Shortly after Lockyer’s death, an
Indian physicist M.N. Saha, came to work under Fowler at Imperial
College. The paper he wrote during this visit … showed how the spectra
of stars could be understood in terms of the new quantum theory
of the atom together with the dissociation hypothesis. After some
initial opposition, his results were rapidly accepted. The theory
showed that both temperature and pressure affected the dissociation
of atoms in stellar atmospheres. So both Lockyer and his opponents
had been partly right. It is only fair to Lockyer to add that the
influence of temperature on stellar spectra is much more marked
than of pressure.”
Medows’ observation was far from truth. To quote
D. S. Kothari : “It is pertinent to remark that the ionization theory
was formulated by Saha working by himself in Calcutta, and the paper
quoted above was communicated by him from Calcutta to the Philosophical
Magazine - incorrect statements to the contrary have sometimes been
made. (Saha’s first visit to Europe was made a couple of months
later.) Further papers soon followed. It is not too much to say
that the theory of thermal ionization introduced a new epoch in
astrophysics by providing for the first time, on the basis of simple
thermodynamic consideration and elementary concepts of the quantum
theory, a straight forward interpretation of the different classes
of stellar spectra in terms of the physical condition (temperature
and to a lesser extent pressure) prevailing in the stellar atmospheres.”
To describe how Saha got the idea of working on
this topic and when he completed his work we quote Saha rather extensively:
“It was while pondering over the problems of astrophysics,
and teaching thermodynamics and spectroscopy to the MSc classes
that the theory of thermal ionization took a definite shape in my
mind in 1919. I was a regular reader of German Journals, which had
just started coming after four years of first world war, and in
course of these studies, I came across a paper by J.Eggert in the
Physikalische zeitschrifts (p.573) Dec. 1919, “ Uber den Dissociationzustand
der Fixterngase” in which he applied Nernst’s Heat Theorem to explain
the high ionization in stars due to high temperatures, postulated
by Eddington in course of his studies on stellar structure.
Eggert, who was a pupil of Nernst and was at the
time his assistant, had given a formula for thermal ionization,
but it is rather strange that he missed the significance of ionization
potential of atoms. Importance of which was apparent from the theoretical
work of Bohr, and practical work of Franck and Hertz which was attracting
a good deal of attention in those days…Eggert used Sackur’s formula
of the chemical constant for calculating that of the electron, but
in trying to account for multiple ionization of iron atoms in the
interior of stars on this basis, he used very artificial values
of ionization potential.
While reading Eggert’s paper I saw at once the
importance of introducing the value of ionization potential in the
formula of Eggert, for calculating accurately the ionization, single
or multiple, of any particular element under any combination of
temperature and pressure.
I thus arrived at the formula which now goes by
my name. Owing to my previous acquaintance with chromospheric and
stellar problems, I could at once see its application. I prepared
in the course of six months of 1919 (February to September) four
papers and communicated them for publication in the Philosophical
Magazine from India within August to September.” “I had no personal
acquaintance with Prof. A. Fowler except that I had read his paper
on the spectrum of ionized helium. “On my arrival in England, I
saw Prof. Albert Fowler who at first thought that I had come to
work for the DSc degree of the London University like other Indian
students working under him. But when I explained to him that I wanted
to work there only for a short period to obtain verification of
my theory, he did not show himself very enthusiastic, but allowed
me to read and work in his laboratory. Probably he had not much
time to listen to me at the first meeting. This was in November
of 1920. If you look at the records of Imperial College, you will
find that I never got my name registered for my degree work. In
the meantime, my first paper “Ionization in the Solar Chromosphere”
communicated from India had appeared in Phil. Mag, thanks to a personal
call which I made on Mr. Francis, the publisher of the journal.
After its publication, Prof. Fowler began to take a more lively
interest in my work and in my views.”
In November 1921 Saha returned to India and joined
the University of Calcutta as Khaira Professor of Physics, a new
Chair created from the endowment of Kumar Guruprasad Singh of Khaira.
But Saha did not stay long in Kolkata. He moved to Allahabad in
1923 as Head of the Department of Physics. Saha’s decision to move
out of Kolkata was mainly because there were no financial grants
for carrying out research. Though Asutosh Mookerjee could create
additional chairs out of donations but the Government did not approve
his plan for expansion. The then Governor Lord Ronaldshay, while
praising the work done in the post-graduate departments of the Calcutta
University, said: “In a poor country there are obvious limits to
the extent to which such studies can be financed by public funds.
The legislature will, I hope, be prepared to make some additional
contribution towards the university in the present difficulties.
But the legislature itself with extremely exiguous resources is
faced with many urgent demands. And under the circumstances it appears
to me that the university may have to consider whether it is bound
to provide post-graduate teaching on every subject in which it is
prepared to examine and confer awards…” Irrespective of Governor’s
assurance there was no increase in the funds allocated to the Calcutta
University. In 1922 the Government was willing to give an additional
grant of two-and-a-half lakh. But the grant was subjected to certain
conditions and which were not acceptable to Asutosh Mookerjee. While
declining the offer Mookerjee said: “We will not take the money.
We shall retrench and we shall live within our means. We shall go
from door to door and make the people of Bengal realise their responsibility.
Our Post-graduate teachers will starve themselves rather than give
up their freedom.” Under these circumstances Saha’s decision to
leave Calcutta evoked adverse feelings. The Calcutta Review made
scathing attack on Saha’s decision to leave Kolkata. However, it
may be noted that Saha before leaving the Calcutta University wrote
to its Syndicate : “I am however, willing to continue to serve my
alma mater, provided the university is willing to grant me a graded
scale of pay namely Rs. 650-50-1000 plus Rs. 15,000 to be placed
immediately at my disposal as my personal research grant.” The Syndicate
rejected his request stating that “….in view of the present financial
position of the university and in view of the claims of other university
teachers, his request cannot be complied with.” And so finally Saha
went to the Allahabad University. At Allahabad before he could start
research work he had to improve the workshop, the laboratory and
the library. Moreover, he found hardly any time for research after
discharging heavy teaching responsibilities. But Saha was not to
be detracted by adverse conditions. And very soon research papers
started appearing from Saha and his students. Among his collaborators
at Allahabad were N.K. Sur, P.K. Kichlu, D.S. Kothari, R.C. Majumdar,
Atmaram, K.B. Mathur and B.D. Nag Choudhary. After his becoming
Fellow of the Royal Society in 1927, the Governor of the United
Province, Sir William Morris provided a research grant of Rs. 5,000
per year to Saha’s Department. At Allahabad, besides continuing
his research work on astrophysical problems, he initiated and organized
research in several other branches of physics viz. statistical mechanics,
atomic and molecular spectroscopy, electron affinity of electro-negative
elements, active modification of nitrogen, high temperature dissociation
of molecules propagation of radio waves in ionosphere and physics
of the upper atmosphere. It is here that Saha wrote his famous textbook,
A Treatise on Heat, which was first published in 1931 under the
title of A Textbook of Heat. The book was written jointly with B.N.
Srivastava. C.V. Raman in his foreword to the book wrote : “By undertaking
the necessarily laborious task of producing a systematic and up-to-date
treatise on the theory of heat, Prof. Saha has earned a claim to
the gratitude of the wide circle of readers both in and outside
of India, who it is confidently hoped, will study this book and
appreciate its merits.” A concise version of this book was published
for science graduates. It was tilted Junior Text Book of Heat. He
wrote another book (jointly with N.K. Saha ) titled Treatise on
Modern Physics. At Allahabad Saha established the United Province
Academy of Sciences in 1930. Interestingly the suggestion for establishing
such an Academy had come from the Governor of the United Province,
Sir Malcolm Hailey. While addressing the scientists of the United
Province gathered at Allahabad on the occasion of the Indian Science
Congress Association Malcolm said : “Now I am well aware that there
are definite limits to the extent to which the efforts of our research
workers or students can be directed to these problem (of economic
and utilitarian value), and I am also well aware that coordination
of their labours cannot be directed from outside. It must be voluntary
effort, or at the most, it must be advice given by some Academy
of Science which will contain authoritative representatives of all
the specialized branches of scientific activity now at work in the
province. But if some form of visible co-ordination could be attempted,
and if it could be proved to the public that science workers were
contributing at least some of their energies in the direction I
have suggested, then I believe we should have a far more effective
case in calling for that public support and private liberality on
which the further progress of scientific work must depend.”
Saha returned to the Calcutta University in July
1938. He became the Palit Professor and Head of the Department of
Physics. At that time Shyama Prasad Mookerjee was the Vice Chancellor
of the University and who was soon to be succeeded by Sir Mahammed
Azizul Haque. After joining Saha immediately got involved in organizing
research in the Palit Laboratory. He also took the task of remodeling
the MSc syllabus in physics. Saha introduced a general and a special
paper in nuclear physics in 1940. One may note that, the phenomenon
of the fission, was discovered in 1939 by Otto Hahn (1879-1968)
and Fritz Strassmann (1902-80). Saha also added a general paper
in quantum mechanics. Commenting on Saha’s research work at the
Calcutta University D.S. Kothari wrote: “His researches in Calcutta
were concerned largely with the systematics of atomic nuclei, particularly
beta-activity, the propagation of electromagnetic waves in the ionosphere,
and the problem of the solar corona.”
Saha was a great institution builder. He made the
Physics Department of the Allahabad University, which he joined
in 1923, as one of the most active centres of research in the country,
particularly in the field of spectroscopy. The Department attracted
students from all over the country. In 1911 Saha founded the UP
Academy of Sciences at Allahabad, which was later renamed as National
Academy of Sciences, India. The Academy, which was inaugurated on
March 1, 1932, was modelled on the lines of the Asiatic Society
of Bengal. Saha was its first President. In 1933 Saha founded the
Indian Physical Society at Calcutta. The Society published the Indian
Journal Physics. Eminent scientists like Raman, Saha and Krishnan
regularly contributed their important papers to the Indian Journal
of Physics. With Saha’s initiative National Institute of Sciences
of India was established in Calcutta. Its formation was formally
announced on January 7, 1935 in the Senate Hall of the Calcutta
University under the Chairmanship of the J.H. Hutton. L.L. Fermor
was elected the first president of the Institute. The formation
of such an All India Academy of Sciences was first proposed by Saha
in his Presidential Address of the Indian Science Congress Association
in Mumbai (Bombay) in 1934. The National Institute of Sciences was
later renamed as the Indian National Academy of Sciences and its
headquarters were transferred to New Delhi. Saha was closely associated
with the planning and establishment of the Central Glass and Ceramic
Research Institute, a constituent laboratory of the Council of Scientific
and Industrial Research, at Kolkata. In 1944 Saha was elected the
Honorary Secretary of the Indian Association for the Cultivation
of Science and he was its President during 1946- 50. Saha became
the full-time Director of the Laboratories of the Association in
1952, a post he held till his death. Under the leadership of Saha,
there was a large-scale expansion of the activities of the Association.
As President of the Indian Association for the Cultivation of Science
he built its modern laboratories.
Saha played a significant role in the establishment
of departments of Radio Physics and Electronics and Applied physics
of the Calcutta University.
In 1950 Saha founded the Institute of Nuclear Physics.
The Foundation Stone of the Institute was laid by Dr. Shyama Prasad
Mookherjee the then Civil Supply Minister of the Government of India.
The institute, which was formally inaugurated by Irene Joliot-Curie
on January 11, 1950, was originally situated in the campus of the
Calcutta University. Among those who attended the inauguration ceremony
were Robert Robinson and J.D. Bernal.
It was Saha, who first introduced nuclear physics
in the MSc physics syllabus of the Calcutta University in 1940.
He also started a post-MSc course in nuclear science for the country.
He initiated steps for building a cyclotron, the first of its kind
in the country.
The Conference of Scientific workers in Britain
held in July 1946 led to the formation of the World Federation of
Scientific Workers. Saha had participated in this Conference and
after coming back to India he wrote editorials in the Science and
Culture urging Indian scientific workers to form a similar kind
of organisation. Explaining the objectives of such an Association
Saha wrote: “the aim and objects of the Association are for fuller
use of science for national life – for education through meetings
and for action in public field.” On some other occasion he wrote:
“It is high time for the scientific workers in India that they exert
their inherent right to live like decent citizen and shoulder responsibilities
for the betterment of their motherland.” The Association for Scientific
Workers (India) was eventually formed an 7th July 1947
Saha founded the Indian Science News Association
at Calcutta in 1935. Its main objective was to disseminate science
amongst the public. The Association started publishing its journal
called Science and Culture. On receiving, a copy of the first issue
of the Journal, Netaji Subhash Chandra Bose wrote: “The appearance
of Science and Culture is to be warmly welcomed not only by those,
who are interested in abstract science but also by those who are
concerned with nationbuilding in practice. Whatever might have been
the views of our older “Nation builders” we younger folk approach
the task of nation building in a thoroughly scientific spirit and
we desire to be armed with all the knowledge which modern science
and culture can afford us. It is not possible however, for political
workers with their unending preoccupations to glean that knowledge
themselves, it is therefore, for scientists and scientific investigators
to come in their rescue.” Saha himself wrote more than 200 articles
in Science and Culture on a wide range of topics which included:
organization of scientific and industrial research, atomic energy
and its industrial use, river valley development projects, planning
the national economy, educational reforms and modification of Indian
calendar. The journal is presently running in its 68th volume.
Saha wrote extensively on his vision of scientific
economic planning for India. It was Saha who persuaded Netaji Subhash
Chandra Bose, then President of the Indian National Congress, to
set up a National Planning Committee. At the beginning M. Visvesvaraya,
the most celebrated Indian engineer, was the Chairman of the Committee.
However, Saha thought that to have its impact the Committee should
be headed by a powerful Congress leader and he persuaded Rabindranath
Tagore to convince Jawaharlal Nehru to accept the Chairmanship of
the Committee.
Saha was an advocate of the peaceful use of nuclear
energy. He had initiated the first Parliament debate on this subject
on 10th May 1954. Saha was against the establishment of the Atomic
Energy Commission. He was of the view that the researches on nuclear
energy could be undertaken in the university sector. In fact he
wanted the ‘Indian Atomic Energy Act’ to be scrapped altogether.
Saha wanted that the Government should first build up necessary
infrastructure and trained manpower before it undertook such a programme.
However, in spite of Saha’s opposition the Atomic Energy Commission
was created in 1948 under the chairmanship of Homi J. Bhabha. Many
people may agree with what D. M. Bose had to say in 1967. “The decision
of the Prime Minister (Jawaharlal Nehru) to locate the Department
of Atomic Energy and Atomic Energy Commission with Bhabha as Secretary
of the former and Chairman of the latter must have caused some disappointment
to Saha. Since 1935 Nehru and Saha cooperated in many fields of
common interest, including the formation of the planning committee
in 1938 by Subhash Chandra Bose with Nehru as Chairman and Saha
as an important member. A growing estrangement with the Prime Minister
with some of the later decisions may have been one of the factors,
which decided Saha to enter politics in 1952. There can be no doubt,
however, as the events shaped subsequently that the Prime Minister
Nehru was undoubtedly right in entrusting Bhabha with the development
of India’s plan for utilization of atomic energy. Bhabha identified
himself completely with the development of atomic energy in India.
Saha’s interest was many and varied.”
Saha was deeply concerned with the recurring disastrous
floods in many Indian rivers. The extensive damage caused by floods
in North Bengal in 1923 prompted Acharya Prafulla Chandra Ray to
organize relief operation under the aegis of North Bengal Relief
Committee. Ray was able to collect a large fund from the general
public for the relief work and he was assisted by Subhash Chandra
Bose, Meghnad Saha and Satish Chandra Dasgupta. And it was while
carrying out the relief work Saha got a first hand experience of
the devastating power of floods. Saha wrote about his experience
in newspapers and magazines. In his Presidential address to the
Indian Science Congress in Mumbai in 1934 he drew specific attention
to serious problems caused by floods. He also emphasized the need
for a River Research Laboratory. Again in 1938, in his presidential
address to the National Institute of Sciences of India he highlighted
the danger posed by recurrent floods in Indian rivers particularly
in the deltaic ones. In 1943 the flood in Bengal isolated Kolkata
from rest of India and Saha wrote extensively on the issue. Saha’s
writings and speeches made the government realize the gravity of
the situation. As a result the Damodar Valley Enquiry Committee
came into being in 1943. The Committee was chaired by the Maharaja
of Burdwan. Saha was also a member of the Committee. Saha presented
a plan for handling the Damodar river system before the Committee.
He also wrote extensively on river control based on modern science
and technology. He argued that the model of Tennessee river system
under the Tennessee Valley Authority (TVA) in USA could be adapted
to the Damodar Valley. At the instance of Dr. B. R. Ambedkar, the
then member-in-charge of power and works in the Viceroy’s cabinet,
the Government adopted a resolution to set up a Damodar Valley Corporation
(DVC) after the model of TVA. The DVC was set up in March 1948.
Saha’s interest was not confined to Bengal rivers alone.
Saha’s work relating to reform of Indian calendar
was very significant. Saha was the Chairman of the Calendar Reform
Committee appointed by the Government of India in 1952 under the
aegis of the Council of Scientific and Industrial Research. Other
members of the Committee were: A. C. Banerjee, K. K. Daftari, J.
S. Karandikar, Gorakh Prasad, R. V. Vaidya and N. C. Lahiri. It
was Saha’s effort, which led to the formation of the Committee.
The task before the Committee was to prepare an accurate calendar
based on scientific study, which could be adopted uniformly throughout
India. It was a mammoth task. The Committee had to undertake a detailed
study of different calendars prevalent in different parts of the
country. There were thirty different calendars. The task was further
complicated by the fact that with calendar religion and local sentiments
were involved. Nehru, in his preface to the Report of the Committee,
which was published in 1955, wrote: “They (different calendars)
represent past political divisions in the country…now that we have
attained Independence, it is obviously desirable that there should
be a certain uniformity in the calendar for our civic, social and
other purposes and this should be done on a scientific approach
to this problem.” Some of the important recommendations of the Committee
were:
- The Saka era should be used in the unified national calendar.
(The year 2002 corresponds to the Saka era of 1923-24.)
- The year should start from the day following the vernal equinox
(occurs about March 21) day.
- A normal year would consist of 365 days while a leap year would
have 366 days. After adding seventy-eight to the Saka era, if
the sum is
divisible by four, then it is a leap year. But when the same becomes
a multiple of 100 it would be a leap year when it is divisible
by 400, otherwise it would be a common year.
- Chaitra should be the first month of the year. From Chaitra
to Bhadra each month would have thirty-one days and the rest to
have thirty days.
According to Saha, large-scale industrialization
was the only answer for improving the quality of life. He thought
that India had no hope if she failed to develop science and technology.
Saha wrote: “The philosophy of kindliness and service to our fellow-men
was preached by all founders of great religions, and no doubt some
great kings and ministers of religions in every country and at all
ages tried to give effect to this (altruistic) philosophy. But the
efforts were not successful, for the simple reason that the methods
of production of commodities were too indifferent to yield plenty
for all, which is an indispensable condition for practical altruism.
We can, therefore, hold that so far as individual life is concerned,
science has achieved a target aimed at by the great founders of
religions in advanced countries of the world. The effects of maldistribution
of wealth, due to historical causes, are being rapidly cured by
introduction of social laws.”
In 1952 Saha was elected Member of the Parliament
as an independent candidate from the North-West Calcutta constituency.
Welcoming Saha’s election JBS Haldane said: “May I also be allowed
to congratulate him on his recent successful reentry recently into
politics. India (and Britain too) needs men who will bring some
understanding of science to the government of the country. Even
those who do not share his political views may rejoice that he can
make his voice heard in the council of the people.” Many
wonder why Saha, an internationally known scientists decided to
fight election.
Saha died suddenly due to a massive heart attack
on his way to the office of the Planning Commission on 16 February
1956. As D. S. Kothari one of Saha’s illustrious students, wrote:
“The life of Saha was in a sense an integral part of the growth
of scientific research and progress in India and the effect of his
views and personality would be felt for a long time to come in almost
every aspect of scientific activity in the country. His dedication
to science, his forthrightness and utter disregard of personal comforts
in the pursuit of his chosen vocation will long remain an inspiration
and an example.”
Books written by Meghnad Saha
- The Principles of Relativity (with S.N. Bose) Calcutta University,
Calcutta, 1920. (It was a translation of Einstein’s papers on
theory of relativity).
- Treatise on Heat (with B.N. Srivastava), Indian Press, Allahabad,
1931.
- Junior Text-Book on Heat (with B.N. Srivastava), Indian Press,
Allahabad, 1932.
- Treatise on Modern Physics, Vol-1 (with N.K. Saha) Indian Press,
Allahabad, 1934.
- My Experience in Soviet Russia, Bookman Inc, Calcutta, 1947.
For Further Reading
- Meghnad Saha by Santimay Chatterjee and Enakshi Chatterjee,
National Book Trust, New Delhi 1984.
- Meghnad Saha by S.B. Karmohapatra, Publications Division, Govt.
of India, New Delhi, 1997
- Meghnad Saha by D.S. Kothari in biographical Memoirs of Fellows
of the National Institute of Sciences of India (Vol. 2), New Delhi
1970.
- Professor Meghnad Saha, His Life, Work and Philosophy, Edited
by Samarendra Nath Sen, Meghnad Saha 60th Birthday Committee,
Calcutta, 1954.
- Thirty Years of the Institute of Nuclear Physics, Saha Institute
of Nuclear Physics, 1981.
- Collected Scientific Papers of Meghnad Saha, Edited by Santimay
Chatterjee, Council of Scientific and Industrial Research, New
Delhi 1969.
- Collected Works of Meghnad Saha Edited by Santimay Chatterjee,
Orient Longman Ltd., Calcutta, 1982-1993.
- Science and Culture, Golden Jubilee Volume, Indian Science
News Association, Calcutta, 1985
- Science & Culture, Vols. 1-21, Indian Science News Association,
Calcutta, 1936-55.
- Jawaharlal Nehru on Science, Edited by Baldev Singh, Nehru
Memorial Museum and Library, New Delhi 1986.
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