Tuesday, 5 June 2012

PLANETS


Planets

Year of the Solar System logo: silhouette of child with planets and stars
NASA is celebrating the Year of the Solar System! Spanning a Martian year (23 months), numerous missions will encounter their targets—the Moon and Mars, Mercury and Jupiter, and even comets and asteroids! It’s an unprecedented time in planetary sciences as we learn about new worlds and make new discoveries! Join the exploration at http://solarsystem.nasa.gov/yss/
PLANETS: New Worlds, New Discoveries
NASA is at the leading edge of a journey of scientific discovery that promises to reveal new knowledge of our Solar System’s content, origin, evolution and the potential for life elsewhere.  NASA Planetary Science is engaged in one of the oldest of scientific pursuits: the observation and discovery of our solar system’s planetary objects.  With an exploration strategy based on progressing from flybys, to orbiting, to landing, to roving and finally to returning samples from planetary bodies, NASA advances the scientific understanding of the solar system in extraordinary ways, while pushing the limits of spacecraft and robotic engineering design and operations. Since the 1960s, NASA has broadened its reach with increasingly sophisticated missions launched to a host of nearby planets, moons, comets and asteroids.
NASA Planetary Science continues to expand our knowledge of the solar system, with spacecraft in place from the innermost planet of our Solar System to the very edge of our Sun's influence. In 2010 the EPOXI spacecraft encountered Comet Hartley 2, returning the first images clear enough for scientists to link jets of dust and gas with specific surface cometary features.  In early 2011, the Stardust-NExTmission provided the planetary science community with a first-time opportunity to compare observations of a single comet (Temple 1) made at close range during two successive passages.  When the Stardust spacecraft was retired in March 2011, it had travelled over 3.5 billion miles in our solar system. In another first, in March of 2011 NASA Planetary Science inserted the spacecraft MESSENGERinto orbit around our solar system’s innermost planet, Mercury, providing unprecedented images of that planet’s topography and improved understanding of its core and magnetic field.
Also in this unprecedented productive year of planetary exploration, the spacecraft Dawn was inserted into orbit around the asteroid Vesta in July 2011, the Juno spacecraft was launched in August 2011 on a mission to Jupiter to map the depths of Jupiter’s interior to answer questions about how the gas giant was formed; the two GRAIL spacecraft were launched to the moon in September 2011, and the Mars Science Laboratory was launched in November 2011, on its voyage to Mars with Curiosity, the largest planetary rover ever designed, destined for the surface of Mars to continue the work begun by Spirit and Opportunity. And at the outer reaches of our solar system, New Horizonscontinues on its way to study Pluto and into the Kuiper Belt, birthplace of comets.
With the release of the Planetary Science Decadal Surveyin March 2011, NASA’s planetary scientists and engineers are preparing missions to every corner of the Solar System to seek out the discoveries needed to push the boundaries of planetary science further than ever before.
Our Solar System is a place of beauty and mystery, incredible diversity, extreme environments, and continuous change. Our Solar System is also a natural laboratory, on a grand scale, within which we seek to unravel the mysteries of the universe and our place within it.

Hubble Sees a Celestial Swan and Butterfly

Hubble Sees a Celestial Swan and Butterfly

This image from the Hubble Space Telescope shows planetary nebula NGC 7026. Located just beyond the tip of the tail of the constellation of Cygnus (The Swan), this butterfly-shaped cloud of glowing gas and dust is the wreckage of a star similar to the sun.

Planetary nebulae, despite their name, have nothing to do with planets. They are, in fact, a relatively short-lived phenomenon that occurs at the end of the life of mid-sized stars. As a star's nuclear fuel runs out, its outer layers are puffed out, leaving only the hot core of the star behind. As the gaseous envelope heats up, the atoms in it are excited, and it lights up like a fluorescent sign.

Fluorescent lights on Earth get their bright colors from the gases with which they are filled. Neon signs, famously, produce a bright red color, while ultraviolet lights (black lights) typically contain mercury. The same is true for nebulae: their vivid colors are produced by the mix of gases present in them.

This image was produced by the Wide Field and Planetary Camera 2 aboard the Hubble Space Telescope. A version of it was entered into the Hubble’s Hidden Treasures Competition by contestant Linda Morgan-O'Connor. Hidden Treasures is an initiative to invite astronomy enthusiasts to search the Hubble archive for stunning images that have never been seen by the general public.

The Mysterious Arc of Venus

Transit of VENUS

The Mysterious Arc of Venus

ScienceDaily (June 4, 2012) — When Venus transits the sun on June 5th and 6th, an armada of spacecraft and ground-based telescopes will be on the lookout for something elusive and, until recently, unexpected: The Arc of Venus.
"I was flabbergasted when I first saw it during the 2004 transit," recalls astronomy professor Jay Pasachoff of Williams College. "A bright, glowing rim appeared around the edge of Venus soon after it began to move into the sun."
For a brief instant, the planet had turned into a "ring of fire."
Researchers now understand what happened. Backlit by the sun, Venus's atmosphere refracted sunlight passing through layers of air above the planet's cloudtops, creating an arc of light that was visible in backyard telescopes and spacecraft alike.
It turns out, researchers can learn a lot about Venus by observing the arc. Indeed, it touches on some of the deepest mysteries of the second planet.
› View larger The arc of Venus photographed in 2004 by Riccardo Robitschek and Giovanni Maria Caglieris of Milan, Italy. "We do not understand why our sister planet's atmosphere evolved to be so different than Earth's," explains planetary scientist Thomas Widemann of the Observatoire de Paris.
Earth and Venus are similar distances from the sun, are made of the same basic materials, and are almost perfect twins in terms of size. Yet the two planets are wrapped in stunningly dissimilar blankets of air. Venus's atmosphere is almost 100 times more massive than Earth's and consists mainly of CO2, a greenhouse gas that raises the surface temperature to almost 900°F. Clouds of sulfuric acid tower 14 miles high and whip around the planet as fast as 220 mph. A human being transported to this hellish environment would be crushed, suffocate, desiccate, and possibly ignite.
For the most part, planetary scientists have no idea how Venus turned out this way.
"Our models and tools cannot fully explain Venus, which means we lack the tools for understanding our own planet," points out Widemann. "Caring about Venus is caring about ourselves."
One of the biggest mysteries of Venus is super-rotation. The whole atmosphere circles the planet in just four Earth days, much faster than the planet's spin period of 243 days. "The dynamics of super-rotation are still a puzzle despite a wealth of data from landmark missions such as NASA's Pioneer Venus, Russia's Venera and VEGA missions, NASA's Magellan and more recently ESA's Venus Express."
The arc of Venus as seen by NASA's TRACE spacecraft in 2004. Credit: NASA/Trace/LMSAL This is where the Arc of Venus comes in. The brightness of the arc reveals the temperature and density structure of Venus's middle atmosphere, or "mesosphere," where the sunlight is refracted. According to some models, the mesosphere is key to the physics of super-rotation. By analyzing the lightcurve of the arc, researchers can figure out the temperature and density of this critical layer from pole to pole.
When the arc appeared in 2004, the apparition took astronomers by surprise; as a result, their observations were not optimized to capture and analyze the fast-changing ring of light.
This time, however, they are ready. Together, Pasachoff and Widemann have organized a worldwide effort to monitor the phenomenon on June 5th, 2012. "We're going to observe the arc using 9 coronagraphs spaced around the world," says Pasachoff. "Observing sites include Haleakala, Big Bear, and Sacramento Peak. Japan's Hinode spacecraft and NASA's Solar Dynamics Observatory will also be gathering data."
Pasachoff has some advice for amateur astronomers who wish to observe the arc. "The best times to look are ingress and egress--that is, when the disk of Venus is entering and exiting the sun. Ingress is between 22:09 and 22:27 UT on June 5th; egress occurs between 04:32 and 04:50 UT. Be sure your telescope is safely filtered. Both white light and H-alpha filters might possibly show the arc."

Monday, 4 June 2012

NON INDIAN SCIENTISTS

ALBERT EINSTEIN
I CURIE
CHADWICK
COULOMB
GALILEO
HAWKING
HEISENBERG
KEPLER
M CURIE
ISAAC NEWTON
SCHRODENGER
SOMMERFELD
RUTHERFORD

INDIAN SCIENTISTS



APJ Abdul Kalam



Born - 15 October 1931
Achievements
This eminent scientist and engineer has also served as the 11th President of India from the period 2002 to 2007. APJ Abdul Kalam is a man of vision, who is always full of ideas aimed at the development of the country. He firmly believes that India needs to play a more assertive role in international relations.

Apart from being a notable scientist and engineer, Dr APJ Abdul Kalam served as the 11th President of India from the period 2002 to 2007. He is a man of vision, who is always full of ideas aimed at the development of the country and is also often also referred to as the Missile Man of India. People loved and respected Dr APJ Abdul Kalam so much during his tenure as President that was popularly called the People's President. Read more about the biography of Dr APJ Abdul Kalam here.

APJ Abdul Kalam was born on 15 October 1931 at the South Indian state of Tamil Nadu and received honorary doctorates from about 30 universities globally. In the year 1981, the Government of India presented him the nation's highest civilian honor, the Padma Bhushan and then again, the Padma Vibhushan in 1990 and the Bharat Ratna in 1997. Before Kalam, there have been only two presidents - Sarvepalli Radhakrishnan and Zakir Hussain - to have received the Bharat Ratna before bring appointed to the highest office in India.

Read on about the life history of Dr APJ Abdul Kalam, who's also the first scientist and bachelor to occupy the seat of the Rashtrapati Bhavan. His perspectives on important topics have been enunciated by him in the book 'India 2020'. It highlights the action plans that will help develop the country into a knowledge superpower by the time 2020. One thing for which he received ample kudos is his unambiguous statement that India needs to play a more assertive role in international relations.

And Dr APJ Abdul Kalam regards his work on India's nuclear weapons program as a way to assert India's place as a future superpower. Even during his tenure as President, APJ Kalam took avid interest in the spheres of India's science and technology. He has even put forward a project plan for establishing bio-implants. He is also an ardent advocate of open source software over proprietary solutions to churn out more profits in the field of information technology in India.



Birbal Sahni





Born - 14 November 1891
Died - 10 April 1949
Achievements - Birbal Sahni was a renowned paleobotanist and geologist of India. He is Sahni is credited for setting up the Birbal Sahni Institute of Palaeobotany at Lucknow in the state of Uttar Pradesh. In the year 1929, he received the degree of Sc. D. from the University of Cambridge. He was also appointed the Fellow of the Royal Society of London (FRS) in the year 1936, which is the biggest British scientific honor.

Birbal Sahni was a renowned paleobotanist of India, who studied the fossils of the Indian subcontinent. Also a great geologist, Sahni is credited for establishing the Birbal Sahni Institute of Palaeobotany at Lucknow in the state of Uttar Pradesh. Born on 14 November in the year 1891 at Behra in the Saharanpur District of West Punjab, Birbal was the third son of Ishwar Devi and Prof. Ruchi Ram Sahni. Some famous personalities who were regular guests of his parents were Motilal Nehru, Gopal Krishna Gokhale, Sarojini Naidu and others.

Read on further about the biography of Birbal Sahni, who received his education at the Government College University of Lahore and later from Punjab University. He attended the Emmanuel College at Cambridge in the year 1914. And after this, he pursued further studies under Professor A.C. Seward and was given the D.Sc. degree from London University in the year 1919. Birbal Sahni then came back to his native country India to work as the professor of Botany at the highly esteemed Banaras Hindu University at the holy city of Varanasi.

Sahni also taught at the Punjab University for about a year. Birbal Sahni's academic background was so strong that he was elected the head of the botany department in Lucknow University in the year 1921. There were numerous such landmarks in the life history of Birbal Sahni, whose fabulous research work was honored by the University of Cambridge that decided to present him with the degree of Sc. D. in the year 1929. In the coming time, Sahni not only continued his own study, but also appointed and guided a number of bright students under him.

He holds the credit of establishing the Paleobotanical Society that went on to set up the Institute of Palaeobotany on 10 September 1946. Professor Sahni was respected by all academicians and scholars of his time both in India and abroad. He was appointed the Fellow of the Royal Society of London (FRS) in the year 1936, which is the biggest British scientific honor. And for the first time since its inception, this award was given out to an Indian botanist.

C.V. Raman



Born: November 7, 1888
Died: November 21, 1970
Achievements: He was the first Indian scholar who studied wholly in India received the Nobel Prize.

C.V. Raman is one of the most renowned scientists produced by India. His full name was Chandrasekhara Venkata Raman. For his pioneering work on scattering of light, C.V. Raman won the Nobel Prize for Physics in 1930.

Chandrashekhara Venkata Raman was born on November 7, 1888 in Tiruchinapalli, Tamil Nadu. He was the second child of Chandrasekhar Iyer and Parvathi Amma. His father was a lecturer in mathematics and physics, so he had an academic atmosphere at home. He entered Presidency College, Madras, in 1902, and in 1904 passed his B.A. examination, winning the first place and the gold medal in physics. In 1907, C.V. Raman passed his M.A. obtaining the highest distinctions.

During those times there were not many opportunities for scientists in India. Therefore, Raman joined the Indian Finance Department in 1907. After his office hours, he carried out his experimental research in the laboratory of the Indian Association for the Cultivation of Science at Calcutta. He carried out research in acoustics and optics.

In 1917, Raman was offered the position of Sir Taraknath Palit Professorship of Physics at Calcutta University. He stayed there for the next fifteen years. During his tenure there, he received world wide recognition for his work in optics and scattering of light. He was elected to the Royal Society of London in 1924 and the British made him a knight of the British Empire in 1929. In 1930, Sir C.V. Raman was awarded with Nobel Prize in Physics for his work on scattering of light. The discovery was later christened as "Raman Effect".

In 1934, C.V. Raman became the director of the newly established Indian Institute of Sciences in Bangalore, where two years later he continued as a professor of physics. Other investigations carried out by Raman were: his experimental and theoretical studies on the diffraction of light by acoustic waves of ultrasonic and hypersonic frequencies (published 1934-1942), and those on the effects produced by X-rays on infrared vibrations in crystals exposed to ordinary light. In 1947, he was appointed as the first National Professor by the new government of Independent India. He retired from the Indian Institute in 1948 and a year later he established the Raman Research Institute in Bangalore, where he worked till his death.

Sir C.V. Raman died on November 21, 1970.

Dr. Shanti Swarup Bhatnagar





Born - 21 February 1894
Died - 1 January 1955
Achievements - A noted scientist of India, Dr Shanti Swaroop Bhatnagar was appointed the first director-general of the prestigious Council of Scientific and Industrial Research. He also hold the credit of building 12 national laboratories like Central Food Processing Technological Institute at Mysore, National Chemical Laboratory at Pune and so on.

Dr Shanti Swaroop Bhatnagar was a distinguished Indian scientist. He was born on 21 February 1894 at Shahpur, which is located in Pakistan in present times. His father passed away sometime after the birth of Shanti Swarup Bhatnagar. As such, he spent his childhood days with his maternal grandfather who was an engineer and it was here that he developed an interest in science and engineering. Read on this biography to know more about the life and professional history of Dr Shanti Swaroop Bhatnagar.

As a child, Bhatnagar loved to construct mechanical toys. In the home of his maternal family, he also developed an interest in writing poetry and his one act play in Urdu 'Karamati' won the first prize in a competition. After completing his master's in India, Shanti Swaroop Bhatnagar headed to England for a research fellowship. Here he got his D. Sc degree from the London University in the year 1921. When he came back to his native country, Bhatnagar was presented with a proposal of professorship at the renowned Benaras Hindu University.

Dr Bhatnagar was knighted by the British Government in the year 1941 as an award for his research in science, whereas, on 18 March 1943 he was selected as fellow of the Royal Society. Though his area of interest included emulsions, colloids, and industrial chemistry, but his primary contributions were in the spheres of magneto-chemistry. He also made a melodious kulgeet i.e. University song, which is still sung with great pride before any function in his university.

Prime Minister Jawaharlal Nehru himself was an advocate of scientific development. After India gained freedom from British rule in 1947, the Council of Scientific and Industrial Research was established under the chairmanship of Dr. Bhatnagar, who was appointed its first director-general. In the coming years, he set up 12 national laboratories like Central Food Processing Technological Institute at Mysore, National Chemical Laboratory at Pune, the National Metallurgical Laboratory at Jamshedpur and many others.

Har Gobind Khorana





Born - 9 January 1922
Achievements - Har Gobind Khorana is an American molecular biologist, who was born to an Indian Punjabi couple. For his work on the interpretation of the genetic code and its function in protein synthesis, he was awarded the Nobel Prize in the year 1968.

Har Gobind Khorana is an American molecular biologist born on 9 January 1922 to an Indian Punjabi couple. For his work on the interpretation of the genetic code and its function in protein synthesis, he was awarded the Nobel Prize in the year 1968. This award was, however, also shared by Robert W. Holley and Marshall Warren Nirenberg. The very same year, he received another award 'Louisa Gross Horwitz Prize' along with Nirenberg that was presented to them by the Columbia University.

Read this biography to learn more about Har Gobind Khorana, who became a citizen of the United States of America in the year 1966. In present times, he's residing at Cambridge in Massachusetts, United States as a part of the MIT Chemistry faculty. Har Gobind Khorana was also the first to produce oligonucleotides, which is chains of nucleotides. He was also the first person to segregate DNA ligase, an enzyme that connects sections of DNA together.

These custom-designed portions of artificial genes are extensively used in biology labs for sequencing, cloning and engineering new plants and animals. This invention by Dr. Khorana has become automated and commercialized so that anyone now can order a synthetic gene from any of a number of companies. Thus, this is the history of the life of Dr Har Gobind Khorana as a biologist.

Homi Bhabha





Born: October 30, 1909
Died: January 24, 1966
Achievements: Founded Tata Institute of Fundamental Research; was the first chairman of India's Atomic Energy Commission; was chairman of the first United Nations Conference on the Peaceful Uses of Atomic Energy, held in Geneva in 1955.

Homi Bhabha, whose full name was Homi Jehnagir Bhabha, was a famous Indian atomic scientist. In Independent India, Homi Jehnagir Bhabha, with the support of Jawaharlal Nehru, laid the foundation of a scientific establishment and was responsible for the creation of two premier institutions, Tata Institute of Fundamental Research and Bhabha Atomic Research Centre. Homi Bhabha was the first chairman of India's Atomic Energy Commission.

Homi Jehangir Bhabha was born on October 30, 1909, in Bombay in a rich Parsi family. After graduating from Elphinstone College and the Royal Institute of Science in Bombay, he went to Cambridge University. He received his doctorate in 1934. During this period he worked with Niels Bohr on the studies that led to quantum theory. Homi Jehnagir Bhabha also worked with Walter Heitler on the cascade theory of electron showers, which was of great importance for the understanding of cosmic radiation. He did significant work in identifying the meson.

Due to outbreak of Second World War, Homi Jehangir Bhabha, returned to India in 1939. He set up the Cosmic Ray Research Unit at the Indian Institute of Science, Bangalore under C. V. Raman in 1939. With the help of J.R.D. Tata, he established the Tata Institute of Fundamental Research at Mumbai. In 1945, he became director of the Tata Institute of Fundamental Research.

Apart from being a great scientist, Homi Bhabha, was also a skilled administrator. After independence he received the blessings of Jawaharlal Nehru for peaceful development of atomic energy. He established the Atomic Energy Commission of India in 1948. Under his guidance Indian scientists worked on the development of atomic energy, and the first atomic reactor in Asia went into operation at Trombay, near Bombay, in 1956.

Homi Bhabha was chairman of the first United Nations Conference on the Peaceful Uses of Atomic Energy, held in Geneva in 1955. He advocated international control of nuclear energy and the outlawing of atomic bombs by all countries. He wanted nuclear energy to be used for alleviating poverty and misery of people.

Homi Bhabha received many honorary degrees from Indian and foreign universities and was a member of numerous scientific societies, including the National Academy of Sciences in the United States. He also authored many articles on quantum theory and cosmic rays. Homi Bhabha died in an aeroplane crash in Switzerland on January 24, 1966.

Jagdish Chandra Bose

Born: November 30, 1858
Died: November 23, 1937
Achievements: He was the first to prove that plants too have feelings. He invented wireless telegraphy a year before Marconi patented his invention.

Jagdish Chandra Bose was an eminent Indian scientist. He was the first to prove that plants and metals too have feelings.

Jagdish Chandra Bose was born on November 30, 1858 in Mymensingh (now in Bangladesh). His father Bhagabanchandra Bose was a Deputy Magistrate. Jagadish Chandra Bose had his early education in village school in Bengal medium. In 1869, Jagadish Chandra Bose was sent to Calcutta to learn English and was educated at St.Xavier's School and College. He was a brilliant student. He passed the B.A. in physical sciences in 1879.

In 1880, Jagdishchandra Bose went to England. He studied medicine at London University, England, for a year but gave it up because of his own ill health. Within a year he moved to Cambridge to take up a scholarship to study Natural Science at Christ's College Cambridge. In 1885, he returned from abroad with a B.Sc. degree and Natural Science Tripos (a special course of study at Cambridge).

After his return Jagadish Chandra Bose, was offered lectureship at Presidency College, Calcutta on a salary half that of his English colleagues. He accepted the job but refused to draw his salary in protest. After three years the college ultimately conceded his demand and Jagdish Chandra Bose was paid full salary from the date he joined the college. As a teacher Jagdish Chandra Bose was very popular and engaged the interest of his students by making extensive use of scientific demonstrations. Many of his students at the Presidency College were destined to become famous in their own right. These included Satyendra Nath Bose and Meghnad Saha.

In 1894, Jagadish Chandra Bose decided to devote himself to pure research. He converted a small enclosure adjoining a bathroom in the Presidency College into a laboratory. He carried out experiments involving refraction, diffraction and polarization. It would not be wrong to call him as the inventor of wireless telegraphy. In 1895, a year before Guglielmo Marconi patented this invention, he had demonstrated its functioning in public.

Jagdish Chandra Bose later switched from physics to the study of metals and then plants. He fabricated a highly sensitive "coherer", the device that detects radio waves. He found that the sensitivity of the coherer decreased when it was used continuously for a long period and it regained its sensitivity when he gave the device some rest. He thus concluded that metals have feelings and memory.

Jagdish Chandra Bose showed experimentally plants too have life. He invented an instrument to record the pulse of plants and connected it to a plant. The plant, with its roots, was carefully picked up and dipped up to its stem in a vessel containing bromide, a poison. The plant's pulse beat, which the instrument recorded as a steady to-and-fro movement like the pendulum of a clock, began to grow unsteady. Soon, the spot vibrated violently and then came to a sudden stop. The plant had died because of poison.

Although Jagdish Chandra Bose did invaluable work in Science, his work was recognized in the country only when the Western world recognized its importance. He founded the Bose Institute at Calcutta, devoted mainly to the study of plants. Today, the Institute carries research on other fields too.

Jagdish Chandra Bose died on November 23, 1937.

M.Visvesvaraya





Born: September 15, 1860
Died: April 14, 1962
Achievements: Architect of Krishnarajasagar Dam; devised steel doors to stop the wasteful flow of water in dams; honored with Bharat Ratna.

Sir Mokshagundam Visvesvaraya was an eminent engineer and statesman and played a key role in building of modern India.

Sir M. Visvesvaraya was born on September 15, 1860 in Muddenahalli village in the Kolar district of the erstwhile princely state of Mysore (present day Karnataka). His father Srinivasa Sastry was a Sanskrit scholar and Ayurvedic practitioner. His mother Venkachamma was a religious lady. He lost his father when he was only 15 years old.

Visvesvaraya completed his early education in Chikkaballapur and then went to Bangalore for higher education. He cleared his B.A. Examination in 1881. He got some assistance from the Government of Mysore and joined the Science College in Poona to study Engineering. In 1883 he ranked first in the L.C.E. and the F.C.E. Examinations (equivalent to B.E. Examination of today).

When Sir M. Visvesvaraya cleared his engineering, Government of Bombay offered him a job and appointed him Assistant Engineer at Nasik. As an engineer, he achieved some marvelous feats. He planned a way of supplying water from the river Sindhu to a town called Sukkur. He devised a new irrigation system called the Block System. He devised steel doors to stop the wasteful flow of water in dams. He was the architect of the Krishnaraja Sagara dam in Mysore. The list is endless.

Sir M. Visvesvaraya lead a very simple life. He was a strict vegetarian and a teetotaler. He was known for his honesty and integrity. In 1912, Maharaja of Mysore appointed Visvesvaraya as his Dewan. Before accepting the position of Dewan of Mysore, he invited all his relatives for dinner. He told them very clearly that he would accept the prestigious office on the condition that none of them would approach him for favours. As Dewan of Mysore, he worked tirelessly for educational and industrial development of the state. When he was the Dewan many new industries came up. The Sandal Oil Factory, the Soap Factory, the Metals Factory, the Chrome Tanning Factory , were some of them. Of the many factories he started the most important is the Bhadravati Iron and Steel Works.

Sir M. Visvesvaraya voluntarily retired as Dewan of Mysore in 1918. He worked actively even after his retirement. Sir M. Visvesvaraya was honored with Bharat Ratna in 1955 for his invaluable contribution to the nation. When he reached the age of 100, the Government of India brought out a stamp in his honor. Sir Visvesvaraya passed away on April 14, 1962 at the age of 101.

Some of the honours and laurels conferred on Sir M. Visvesvaraya
  • 1904: Honorary Membership of London Institution of Civil Engineers for an unbroken period of 50 years
  • 1906: "Kaisar-i-Hind" in recognition of his services
  • 1911: C.I.E. (Companion of the Indian Empire) at the Delhi Darbar
  • 1915: K.C.I.E. (Knight Commander of the Order of the Indian Empire)
  • 1921: D.Sc. - Calcutta University
  • 1931: LLD - Bombay University
  • 1937: D.Litt - Benaras Hindu University
  • 1943: Elected as an Honorary Life Member of the Institution of Engineers (India)
  • 1944: D.Sc. - Allahabad University
  • 1948: Doctorate - LLD., Mysore University
  • 1953: D.Litt - Andhra University
  • 1953: Awarded the Honorary Fellowship of the Institute of Town Planners, India
  • 1955: Conferred ' BHARATHA RATNA'
  • 1958: 'Durga Prasad Khaitan Memorial Gold Medal' by the Royal Asiatic Society Council of Bengal
1959: Fellowship of the Indian Institute of Science, Bangalore

Meghnad Saha





Born: October 6, 1893
Died: February 16, 1956
Achievements: Made outstanding contribution to the field of Astrophysics. He put forward an "ionization formula" which explained the presence of the spectral lines.

Meghnad Saha was an outstanding Indian scientist. He made remarkable contribution to the field of Astrophysics.

Meghnad Saha was born on October 6, 1893 in Sheoratali, a village in the District of Dacca, now in Bangladesh. He was the fifth child of his parents, Sri Jagannath Saha and Smt. Bhubaneshwari Devi. His father was a grocer in the village. Meghnad Saha had his early schooling in the primary school of the village. As his family could hardly able to make both ends meet, Meghnad Saha managed to pursue his schooling only due to the generosity of a local medical practitioner, Ananta Kumar Das, who provided him with boarding and lodging in his house.

In 1905, British Government took the decision of partition of Bengal. There was great political unrest in Bengal as popular opinion was against the partition. Sir Bampfylde Fuller was governor of East Bengal at that time. One day he came to visit the Collegiate school. Meghnad Saha along with other students boycotted his visit. As a result he was suspended from the school and his scholarship was terminated. He took admission in the Kishorilal Jubili School and passed the Entrance Examination of the Calcutta University in 1909, standing first among the student from East Bengal obtaining the highest marks in languages (English, Bengali and Sanskrit combined) and in Mathematics. In 1911, he ranked third in the ISc exam while the first position went to another great scientist Satyendranath Bose.

Meghnad Saha took admission in Presidency College Calcutta. In 1913 he graduated from Presidency College with Mathematics major and got the second rank in the University of Calcutta while the first one was taken by S.N. Bose. In 1915, both S.N.Bose and Meghnad Saha ranked first in M.Sc. exam, Meghnad Saha in Applied Mathematics and S.N. Bose in Pure Mathematics.

While studying in Presidency College, Meghnad got involved with Anushilan Samiti to take part in freedom fighting movement. He also came in contact with nationalists like Subhash Chandra Bose and Rajendra Prasad.

In 1917, Meghnad Saha joined as lecturer at the newly opened University College of Science in Calcutta. He taught Quantum Physics. Along with S.N. Bose, he translated the papers published in German by Einstein and Minkowski on relativity into English versions. In 1919, American Astrophysical Journal published - "On Selective Radiation Pressure and it's application" - a research paper by Meghnad Saha. He put forward an "ionization formula" which explained the presence of the spectral lines. The formula proved to be a breakthrough in astrophysics. He went abroad and stayed for two years. He spent time in research at Imperial College, London and at a research laboratory in Germany. In 1927, Meghnad Saha was elected as a fellow of London's Royal Society.

Meghnad Saha moved to Allahabad and in 1932 Uttar Pradesh Academy of Science was established. He returned to Science College, Calcutta in 1938. During this time Saha got interested in Nuclear Physics. In 1947, he established Institute of Nuclear Physics which later was named after him as Saha Institute of Nuclear Physics. He took the first effort to include Nuclear Physics in the curriculum of higher studies of science. Having seen cyclotrons used for research in nuclear physics abroad, he ordered one to be installed in the institute. In 1950, India had its first cyclotron in operation.

In 1952 he stood as an independent candidate for Parliament and was elected by a wide margin. He died on February 16, 1956 due to a heart attack.

Satyendra Nath Bose





Born: January 1, 1894
Died: February 4, 1974
Achievements: Famous for "Bose-Einstein Theory". A subatomic particle Boson has been named after him. Honored with "Padma Bhushan".

Satyendra Nath Bose was an outstanding Indian physicist. He is known for his work in Quantum Physics. He is famous for "Bose-Einstein Theory" and a kind of particle in atom has been named after his name as Boson.

Satyendranath Bose was born on January 1, 1894 in Calcutta. His father Surendranath Bose was employed in the Engineering Department of the East India Railway. Satyendranath was the eldest of his seven children.

Satyendra Nath Bose had his schooling from Hindu High School in Calcutta. He was a brilliant student. He passed the ISc in 1911 from the Presidency College, Calcutta securing the first position. Satyendra Nath Bose did his BSc in Mathematics from the Presidency College in 1913 and MSc in Mixed Mathematics in 1915 from the same college. He topped the university in BSc. and MSc. Exams.

In 1916, the Calcutta University started M.Sc. classes in Modern Mathematics and Modern Physics. S.N. Bose started his career in 1916 as a Lecturer in Physics in Calcutta University. He served here from 1916 to 1921. He joined the newly established Dhaka University in 1921 as a Reader in the Department of Physics. In 1924, Satyendra Nath Bose published an article titled Max Planck's Law and Light Quantum Hypothesis. This article was sent to Albert Einstein. Einstein appreciated it so much that he himself translated it into German and sent it for publication to a famous periodical in Germany - 'Zeitschrift fur Physik'. The hypothesis received a great attention and was highly appreciated by the scientists. It became famous to the scientists as 'Bose-Einstein Theory'.

In 1926, Satyendra Nath Bose became a Professor of Physics in Dhaka University. Though he had not completed his doctorate till then, he was appointed as professor on Einstein's recommendation. In 1929 Satyendranath Bose was elected chairman of the Physics of the Indian Science Congress and in 1944 elected full chairman of the Congress. In 1945, he was appointed as Khaira Professor of Physics in Calcutta University. He retired from Calcutta University in 1956. The University honored him on his retirement by appointing him as Emeritus Professor. Later he became the Vice Chancellor of the Viswabharati University. In 1958, he was made a Fellow of the Royal Society, London.

Satyendra Nath Bose was honored with 'Padmabhusan' by the Indian Government in recognition of his outstanding achievement. He died in Kolkata on February 4, 1974.

Subrahmanyan Chandrasekhar





Born: October 19, 1910
Died: August 21, 1995
Achievements: Discovery of Chandrasekhar Limit; awarded Nobel Prize in Physics in 1983.

Subrahmanyan Chandrasekhar was one of the greatest scientists of the 20th century. He did commendable work in astrophysics, physics and applied mathematics. Chandrasekhar was awarded the Nobel Prize in Physics in 1983.

Subrahmanyan Chandrasekhar was born on October 19, 1910 in Lahore. His father, Chandrasekhara Subrahmanya Ayyar was an officer in Government Service in the Indian Audits and Accounts Department. His mother Sita was a woman of high intellectual attainments. C.V. Raman, the first Indian to get Nobel Prize in science was the younger brother of Chandrasekhar's father. Till the age of 12, Subramanyan Chandrasekhar had his education at home under his parents and private tutors. In 1922, at the age of 12, he attended the Hindu High School. He joined the Madras Presidency College in 1925. Subrahmanyan Chandrashekhar passed his Bachelor's degree, B.Sc. (Hon.), in physics in June 1930. In July 1930, he was awarded a Government of India scholarship for graduate studies in Cambridge, England.

Subrahmanyan Chandrasekhar completed his Ph.D. degree at Cambridge in the summer of 1933. In October 1933, Chandrasekhar was elected to a Prize Fellowship at Trinity College for the period 1933-37. In 1936, while on a short visit to Harvard University, Subrahmanyan Chandrasekhar, was offered a position as a Research Associate at the University of Chicago and remained there ever since. In September 1936, Subrahmanyan Chandra Shekhar married Lomita Doraiswamy. She was her junior at the Presidency College in Madras.

Subrahmanyan Chandrasekhar is best known for his discovery of Chandrasekhar Limit. He showed that there is a maximum mass which can be supported against gravity by pressure made up of electrons and atomic nuclei. The value of this limit is about 1.44 times a solar mass. The Chandrasekhar Limit plays a crucial role in understanding the stellar evolution. If the mass of a star exceeded this limit, the star would not become a white dwarf. It would continue to collapse under the extreme pressure of gravitational forces. The formulation of the Chandrasekhar Limit led to the discovery of neutron stars and black holes. Depending on the mass there are three possible final stages of a star - white dwarf, neutron star and black hole.

Apart from discovery of Chandrasekhar Limit, major work done by Subrahmanyan Chandrasekhar includes: theory of Brownian motion (1938-1943); theory of the illumination and the polarization of the sunlit sky (1943-1950); theory of the illumination and the polarization of the sunlit sky (1943-1950); the equilibrium and the stability of ellipsoidal figures of equilibrium, partly in collaboration with Norman R. Lebovitz (1961-1968); the general theory of relativity and relativistic astrophysics (1962-1971); and the mathematical theory of black holes (1974- 1983).

Subrahmanyan Chandrasekhar was awarded (jointly with the nuclear astrophysicist W.A. Fowler) the Nobel Prize in Physics in 1983. He died on August 21, 1995.

Vikram Sarabhai


Born: August 12, 1919
Died: December 31,1971
Achievements: Considered the Father of the Indian space program; instrumental in establishing the Physical Research Laboratory (PRL) in Ahmedabad in November 1947; was Chairman of the Atomic Energy Commission. He along with other Ahmedabad-based industrialists played a major role in the creation of the Indian Institute of Management, Ahmedabad.

Vikram Sarabhai was one of the greatest scientists of India. He is considered as the Father of the Indian space program. Apart from being a scientist, he was a rare combination of an innovator, industrialist and visionary.

Vikram Ambalal Sarabhai was born on August 12, 1919 at Ahmedabad in an affluent family of progressive industrialists. He was one of eight children of Ambalal and Sarla Devi. He had his early education in a private school, “Retreat” run by his parents on Montessori lines. Some of the great men of India such as Gurudev Rabindranath, J. Krishna Murthi, Motilal Nehru, V. S. Shrinivasa Shastri, Jawaharlal Nehru, Sarojini Naidu, Maulana Azad, C. F. Andrews, C. V. Raman et al. used to stay with the Sarabhai family when they visited Ahmedabad. Mahatma Gandhi also once stayed at their house while recovering from an illness. Visits by such great men greatly influenced Vikram Sarabhai.

After his matriculation, Vikram Sarabhai proceeded to Cambridge for his college education and took the tripods degree from St. John's college in 1940. When World War II began, he returned home and joined as a research scholar under Sir C. V. Raman at the Indian Institute of Science, Bangalore His interest in solar physics and cosmic ray led him to set up many observation stations around the country. He built the necessary equipment with which he took measurements at Bangalore, Poona and the Himalayas. He returned to Cambridge in 1945 and completed his Ph.D in 1947.

Vikram Sarabhai was instrumental in establishing the Physical Research Laboratory (PRL) in Ahmedabad in November 1947. The laboratory was established in a few rooms in M.G. Science Institute of the Ahmedabad Education Society, which was founded by his parents. Subsequently, it got support from the Council of Scientific and Industrial Research (CSIR) and the Department of Atomic Energy.

Vikram Sarabhai did research on the time variations of cosmic rays and concluded that meteorological effects could not entirely affect the observed daily variations of cosmic rays; further, the residual variations were wide and global and these were related to variations in solar activity. Vikram Sarabhai visualized a new field of research opening up in solar and interplanetary Physics.

The year 1957-1958 was designated as International Geo-physical year (IGY). The Indian program for the IGY had been one of the most significant ventures of Sarabhai. It exposed him to the new vistas of space science with the launching in 1957 of Sputnik-I. Subsequently, the Indian National Committee for Space Research was created, of which Vikram Sarabhai became Chairman.

With active support from Homi Bhabha, Vikram Sarabhai, set up the first Rocket Launching station (TERLS) in the country at Thumba near Thiruvananthapuram on the Arabian Coast, as Thumba is very close to the Equator. The first rocket with sodium vapour payload was launched on November 21, 1963. In 1965, the UN General Assembly gave recognition to TERLS as an international facility.

After the sudden death of Homi Bhabha in an air crash, Vikram Sarabhai was appointed Chairman, Atomic Energy Commission in May 1966. He wanted the practical application of science to reach the common man. He decided to acquire competence in advance technology for the solution of country’s problems based on technical and economic evaluation of its real resources. He initiated India’s space programme, which today is renowned all over the world.

Dr. Vikram Sarabhai was awarded with Shanti Swarup Bhatnagar Medal in 1962 and Padma Bhushan in 1966. Vikram Sarabhai passed away in his sleep on December 31,1971.


 

Anil Kakodkar





Born - 11 November 1943
Achievements - Dr Anil Kakodkar is a famous Indian nuclear scientist. Currently, he's the chairman of the Atomic Energy Commission of India (AECI) and the Secretary to the Government of India, Department of Atomic Energy. He was also the director of the Bhabha Atomic Research Centre at Trombay.

Dr Anil Kakodkar is a very distinguished nuclear scientist of India. He is presently the chairman of the Atomic Energy Commission of India (AECI) as well as the Secretary to the Government of India, Department of Atomic Energy. He was the director of the Bhabha Atomic Research Centre at Trombay from the year 1996-2000 before being granted the opportunity of leading India's nuclear programme. Read on more about the biography of Anil Kakodkar.

Anil Kakodkar was born on 11 November 1943 in the Barawani village located in the present day Indian state of Madhya Pradesh. He's the son of Mrs Kamala Kakodkar & Mr. P. Kakodkar, both of whom happen to be Gandhian freedom fighters. His early education happened here and at Khargoan. After this, Anil Kakodkar went away to Bombay to pursue his post-matriculation studies. He graduated from the Ruparel College there.

Kakodkar then joined VJTI in Bombay University in 1963 to obtain a degree in Mechanical Engineering. In the year 1964, Anil Kakodkar joined the Bhabha Atomic Research Centre (BARC). He also notched a masters degree in experimental stress analysis from the University of Nottingham in the year 1969. The life history of Anil Kakodkar's career as nuclear scientist further saw him join the Reactor Engineering Division of the BARC.

Anil Kakodkar also has the credit of being a member of the core team of architects of India's Peaceful Nuclear Tests that were conducted during the years 1974 and 1998. He also led the indigenous development of the country's Pressurised Heavy Water Reactor Technology. Anil Kakodkar's efforts in the rehabilitation of the two reactors at Kalpakkam and the first unit at Rawatbhatta is noteworthy as it were about to close down.

In the year 1996, Anil Kakodkar became the youngest Director of the BARC after Homi Bhabha himself. From the year 2000 onwards, he has been leading the Atomic Energy Commission of India and playing secretary to the Department of Atomic Energy. Dr Anil Kakodkar has been playing a crucial part in demanding sovereignty for India's nuclear tests. Infact, he is known for being a strong advocate of India's self-reliance by employing Thorium as a fuel for nuclear energy.


Srinivasa Ramanujan





Born: December 22, 1887
Died: April 26, 1920
Achievements: Ramanujan independently discovered results of Gauss, Kummer and others on hypergeometric series. Ramanujan's own work on partial sums and products of hypergeometric series have led to major development in the topic. His most famous work was on the number p(n) of partitions of an integer n into summands.

Srinivasa Ramanujan was a mathematician par excellence. He is widely believed to be the greatest mathematician of the 20th Century. Srinivasa Ramanujan made significant contribution to the analytical theory of numbers and worked on elliptic functions, continued fractions, and infinite series.

Srinivasa Aiyangar Ramanujan was born on December 22, 1887 in Erode, Tamil Nadu. His father worked in Kumbakonam as a clerk in a cloth merchant's shop. At the of five Ramanujan went to primary school in Kumbakonam. In 1898 at age 10, he entered the Town High School in Kumbakonam. At the age of eleven he was lent books on advanced trigonometry written by S. L. Loney by two lodgers at his home who studied at the Government college. He mastered them by the age of thirteen. Ramanujan was a bright student, winning academic prizes in high school.

At age of 16 his life took a decisive turn after he obtained a book titled" A Synopsis of Elementary Results in Pure and Applied Mathematics". The book was simply a compilation of thousands of mathematical results, most set down with little or no indication of proof. The book generated Ramanujan's interest in mathematics and he worked through the book's results and beyond. By 1904 Ramanujan had begun to undertake deep research. He investigated the series (1/n) and calculated Euler's constant to 15 decimal places. He began to study the Bernoulli numbers, although this was entirely his own independent discovery. He was given a scholarship to the Government College in Kumbakonam which he entered in 1904. But he neglected his other subjects at the cost of mathematics and failed in college examination. He dropped out of the college.

Ramanujan lived off the charity of friends, filling notebooks with mathematical discoveries and seeking patrons to support his work. In 1906 Ramanujan went to Madras where he entered Pachaiyappa's College. His aim was to pass the First Arts examination which would allow him to be admitted to the University of Madras. Continuing his mathematical work Ramanujan studied continued fractions and divergent series in 1908. At this stage he became seriously ill again and underwent an operation in April 1909 after which he took him some considerable time to recover.

On 14 July 1909 Ramanujan marry a ten year old girl S Janaki Ammal. During this period Ramanujan had his first paper published, a 17-page work on Bernoulli numbers that appeared in 1911 in the Journal of the Indian Mathematical Society. In 191,1 Ramanujan approached the founder of the Indian Mathematical Society for advice on a job. He got the job of clerk at the Madras Port Trust with the help of Indian mathematician Ramachandra Rao.

The professor of civil engineering at the Madras Engineering College C L T Griffith was interested in Ramanujan's abilities and, having been educated at University College London, knew the professor of mathematics there, namely M J M Hill. He wrote to Hill on 12 November 1912 sending some of Ramanujan's work and a copy of his 1911 paper on Bernoulli numbers. Hill replied in a fairly encouraging way but showed that he had failed to understand Ramanujan's results on divergent series. In January 1913 Ramanujan wrote to G H Hardy having seen a copy of his 1910 book Orders of infinity. Hardy, together with Littlewood, studied the long list of unproved theorems which Ramanujan enclosed with his letter. Hardy wrote back to Ramanujan and evinced interest in his work.

University of Madras gave Ramanujan a scholarship in May 1913 for two years and, in 1914, Hardy brought Ramanujan to Trinity College, Cambridge, to begin an extraordinary collaboration. Right from the start Ramanujan's collaboration with Hardy led to important results. In a joint paper with Hardy, Ramanujan gave an asymptotic formula for p(n). It had the remarkable property that it appeared to give the correct value of p(n), and this was later proved by Rademacher.

Ramanujan had problems settling in London. He was an orthodox Brahmin and right from the beginning he had problems with his diet. The outbreak of World War I made obtaining special items of food harder and it was not long before Ramanujan had health problems.

On 16 March 1916 Ramanujan graduated from Cambridge with a Bachelor of Science by Research. He had been allowed to enrol in June 1914 despite not having the proper qualifications. Ramanujan's dissertation was on Highly composite numbers and consisted of seven of his papers published in England.

Ramanujan fell seriously ill in 1917 and his doctors feared that he would die. He did improve a little by September but spent most of his time in various nursing homes. On February 18, 1918 Ramanujan was elected a fellow of the Cambridge Philosophical Society and later he was also elected as a fellow of the Royal Society of London. By the end of November 1918 Ramanujan's health had greatly improved.

Ramanujan sailed to India on 27 February 1919 arriving on 13 March. However his health was very poor and, despite medical treatment, he died on April 6, 1920.

Prasanta Chandra Mahalanobis
Date of Birth
:
Jun 29, 1893
Date of Death
:
Jun 28, 1972
Place of Birth
:
India


Prasanta Chandra Mahalanobis (June 29, 1893-June 28, 1972) was an Indian scientist and applied statistician. He is best known for the Mahalanobis distance, a statistical measure. He did pioneering work on anthropometric variation in India. He founded the Indian Statistical Institute, and contributed to large scale sample surveys. His father, Prabodh Chandra, was an active member of the Sadharan Brahmo Samaj. His mother, Nirodbasini, belonged to a family of considerable academic achievements. He graduated in Physics in 1912 from the Presidency College, Kolkata and completed Tripos at King's College, Cambridge. He then returned to Calcutta. Inspired by the Biometrika and mentored by Acharya Brajendranath Seal he started his statistical work. Initially he worked on analyzing university exam results, anthropometric measurements on Anglo-Indians of Calcutta and some metrological problems. He also worked as a meteorologist for some time. In 1924, when he was working on the probable error of results of agricultural experiments, he met Ronald Fisher, with whom he established a life-long friendship. He also worked on schemes to prevent floods. His most important contributions are related to large scale sample surveys. He introduced the concept of pilot surveys and advocated the usefulness of sampling methods. His name is also associated with the scale free multivariate distance measure, the Mahalanobis distance. He founded the Indian Statistical Institute on 17 December, 1931.

In later life, he contributed prominently to newly independent India's five-year plans starting from the second. His variant of Wassily Leontief's Input-output model was employed in the second and later plans to work towards rapid industrialisation of India and with his colleagues at his institute, he played a key role in developing the required statistical infrastructure. He also had an abiding interest in cultural pursuits and served as secretary to Rabindranath Tagore, particularly during the latter's foreign travels, and also his alma mater Visva Bharati University, for some time.He received one of the highest civilian awards Padma Vibhushan from the Government of India for his contribution to science and services to the country. He died on Jun 28, 1972, a day before his seventy-ninth birthday. Even at this age, he was still active doing research work and discharging his duties as the Secretary and Director of the Indian Statistical Institute and as the Honorary Statistical Advisor to the Cabinet of the Government of India. He had got Weldon Medal from Oxford University in 1944 and Padma Vibhushan in 1968. He was also elected a fellow of the Royal Society, London in 1945 and Honorary President of International Statistical Institute in 1957.