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GS Paper: GS3-16.Achievements of Indians in Science & Technology

  • Plant ‘cries’: Recalling Jagadish Chandra Bose

    bose

    Central idea

    • A recent discovery by researchers from Tel Aviv University in Israel, that plants make distinct sounds in the ultrasonic range when faced with stress, made headlines around the world.
    • However, Indians who had grown up hearing about Jagadish Chandra Bose’s work, more than a century ago, on plant physiology and their ability to feel pleasure and pain, were not surprised.

     

    Details
    Who was JC Bose? – Born in 1858 in Mymensingh, Bengal.

    – A polymath who made significant contributions to physics, biophysics, and plant physiology

    – Graduated from Calcutta University with honors in physics and studied in London and Cambridge.

    Notable works – Developed sensitive instruments for wireless telegraphy and demonstrated the first-ever wireless transmission of microwaves in 1895.

    – Showed that plants produce electrical signals in response to stimuli and made significant contributions to biophysics.

    Recognition & Controversy – Despite his contributions, he was not awarded a Nobel Prize, which many believe he deserved.

    – Refused to obtain patents for his work and rejected the idea of making money from science.

    – Claimed that even inanimate inorganic matter could respond to stimulus and regarded plants as intermediates in a continuum between animals and non-living materials, which was not easily accepted by his contemporaries.

    Legacy and Significance – Founded the Bose Institute, a premier research institute in India.

    – The crater Bose on the Moon is named after him.

    – Regarded as one of India’s greatest scientists, and his legacy continues to inspire future generations of scientists.

    Significance – Bose’s work on plant physiology and biophysics was ahead of his time and not fully understood by his contemporaries.

    – However, over the years, much of his work has been confirmed.

     

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  • The Statistical Genius: C. R. Rao

    rao

    Central idea: Indian-American statistician Calyampudi Radhakrishna Rao has been awarded the 2023 International Prize in Statistics, which is considered the Nobel Prize for statistics.  He is 102 YO.

    Who is C. R. Rao?

    • R. Rao, is an Indian-American mathematician and statistician.
    • He is currently professor emeritus at Pennsylvania State University and Research Professor at the University at Buffalo.
    • Rao has been honoured by numerous colloquia, honorary degrees, and festschrifts and was awarded the US National Medal of Science in 2002.
    • The American Statistical Association has described him as “a living legend whose work has influenced not just statistics, but has had far reaching implications for fields as varied as economics, genetics, anthropology, geology, national planning, demography, biometry, and medicine.”
    • The Times of India listed Rao as one of the top 10 Indian scientists of all time.

    Rao’s Groundbreaking Paper

    • The research paper, “Information and accuracy attainable in the estimation of statistical parameters,” was published in 1945 in the Bulletin of the Calcutta Mathematical Society.
    • The paper provided a lower limit on the variance of an unbiased estimate for a finite sample, which has since become a cornerstone of mathematical statistics.

    Key outcomes of his research

    Rao’s 1945 paper has three outcomes-

    1. Cramer-Rao inequality: It provides a lower limit on the variance of an unbiased estimate for a finite sample.
    2. Rao-Blackwell Theorem: It provides a method to improve an estimate to an optimal estimate.
    3. Information geometry: It is a new interdisciplinary area called “information geometry,” which integrated principles from differential geometry into statistics, including the concepts of metric, distance, and measure.

  • ISRO’s Reusable Launch Vehicle Mission RLV LEX

    reus

    The Indian Space Research Organisation (ISRO) conducted a successful autonomous landing mission experiment for a Reusable Launch Vehicle (RLV) at the Aeronautical Test Range in Chitradurga, Karnataka.

    What is a Reusable Launch Vehicle (RLV)?

    • RLV is a type of spacecraft that is designed to be reused multiple times for launching payloads into space, instead of being discarded after a single launch like traditional rockets.
    • They are seen as a more cost-effective and sustainable option for space launches, as they reduce the need for manufacturing new rockets for each mission.
    • They typically consist of a reusable orbiter, similar to a space shuttle, and a reusable booster that provides the initial thrust needed to lift the orbiter and payload into space.
    • After the payload is released into orbit, the orbiter and booster return to Earth and land back on a runway, where they can be refurbished and reused for future launches.

    Why developing RLV is a big feat?

    Developing RLVs requires advanced technologies, including-

    1. Heat-resistant materials for protecting the spacecraft during re-entry into Earth’s atmosphere
    2. Advanced guidance and control systems for landing and
    3. Reliable propulsion systems for launching and landing

    ISRO’s RLV-TD project

    • ISRO is developing essential technologies for a fully reusable launch vehicle to enable low-cost access to space.
    • The RLV-TD is being used to develop technologies like hypersonic flight (HEX), autonomous landing (LEX), return flight experiment (REX), powered cruise flight, and Scramjet Propulsion Experiment (SPEX).
    • It looks like an aircraft and consists of a fuselage, a nose cap, double delta wings, and twin vertical tails.

    Development of RLV

    (1) First RLV experiment:

    • In 2016, the RLV-TD was launched into space on a rocket powered by a conventional solid booster (HS9) engine.
    • The spacecraft travelled at a speed of Mach 5 when re-entering the earth’s orbit and travelled a distance of 450 km before splashdown in the Bay of Bengal.
    • Critical technologies such as autonomous navigation, guidance and control, reusable thermal protection system, and re-entry mission management were successfully validated.

    (2) Second RLV experiment:

    • The RLV LEX test on April 2, 2023, involved a Chinook Helicopter lifting the RLV LEX to a height of 4.5 km and releasing the RLV.
    • After midair release, the RLV carried out an autonomous landing on the Aeronautical Test Range airstrip, under the exact conditions of a Space Re-entry vehicle’s landing.
    • It achieved landing parameters as might be experienced by an orbital re-entry space vehicle in its return path.

    Advantages of RLVs

    • Reusable launch vehicles are considered a low-cost, reliable, and on-demand mode of accessing space.
    • The cost of a launch can be reduced by nearly 80 percent of the present cost by using RLVs.

    Global RLV technologies

    • NASA space shuttles have been carrying out dozens of human space flight missions.
    • The private space launch services provider SpaceX demonstrated partially reusable launch systems with its Falcon 9 and Falcon Heavy rockets since 2017.
    • SpaceX is also working on a fully reusable launch vehicle system called Starship.
    • Several private launch service providers and government space agencies are working on developing reusable launch systems.

    Significance

    • RLVs have the potential to significantly reduce the cost of space launches, as a significant portion of the cost of traditional rockets comes from the need to manufacture new rockets for each mission.
    • By reusing spacecraft, the cost per launch can be significantly reduced.
    • Additionally, RLVs can provide greater flexibility and reliability for space launches, as they can be launched on-demand instead of needing to be manufactured and assembled for each mission.

     


  • Starberry-Sense: A low cost Star Sensor

    star

    Researchers at the Indian Institute of Astrophysics (IIA) have developed a low-cost star sensor for astronomy and small CubeSat class satellite missions.

    What is Starberry-Sense?

    • Based on commercial/off-the-shelf components, this star sensor costs less than 10% of those available in the market.
    • It is made from a single-board Linux computer called Raspberry Pi, which is widely used among electronics hobby enthusiasts.

    Benefits of Starberry-Sense

    • Starberry-Sense can help small CubeSat class satellite missions find their orientation in space.
    • The instrument can be used for CubeSats and other small satellite missions in the future.
    • The position of stars in the sky is fixed relative to each other and can be used as a stable reference frame to calculate the orientation of a satellite in orbit.

    Successful test

    • The star sensor has successfully undergone the vibration and thermal vacuum test that qualifies it for a space launch and operations.
    • These tests were conducted in-house at the environmental test facility located at the CREST Campus of IIA in Hosakote.

     


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  • APJ Abdul Kalam SLV: India’s 1st Hybrid Rocket launched

    rocket

    India’s first hybrid sounding rocket by private players was launched by some students from Pattipulam village off Tamil Nadu coast.

    About APJ Abdul Kalam SLV

    • Martin Foundation in association with Dr APJ Abdul Kalam International Foundation and Space Zone India successfully completed the project known as Dr APJ Abdul Kalam Satellite Launch Vehicle Mission 2023.
    • The student team included 200 from the fishermen community in Tamil Nadu and Pondicherry, 100 students from tribal communities across India, and 60 from Tamil Nadu.

    What is a Hybrid Rocket?

    • A hybrid rocket is a type of rocket engine that combines features of both liquid-fueled and solid-fueled rockets. In a hybrid rocket, a solid fuel is burned in combination with a liquid or gaseous oxidizer to produce thrust.
    • The solid fuel in a hybrid rocket is typically made of a polymer, such as hydroxyl-terminated polybutadiene (HTPB), which is cast into a cylindrical shape and placed inside the rocket motor.
    • The oxidizer, which is typically nitrous oxide (N2O), is stored in a separate tank and fed into the combustion chamber of the rocket motor.

    How does it work?

    • When the oxidizer is introduced into the combustion chamber, it reacts with the solid fuel, producing a hot gas that is expelled through a nozzle at the end of the rocket.
    • The combustion process can be controlled by adjusting the flow rate of the oxidizer, making hybrid rockets more controllable than solid rockets.

    Benefits offered over conventional rockets

    • Hybrid rockets are generally simpler and less expensive to manufacture than liquid rockets, while providing more control than solid rockets.
    • They are also safer than both liquid and solid rockets, since the fuel and oxidizer are stored separately and can be easily shut off in case of an emergency.

     

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  • InfoCrop v2.1: Indigenous Crop Simulator

    infocrop

    Central idea: Scientists at the Indian Agricultural Research Institute conducted an experiment using InfoCrop version 2.1 to quantify the impact of hot weather on crop yield in Punjab and Haryana.

    What is InfoCrop v2.1?

    • InfoCrop version 2.1 is India’s only dynamic crop simulation model developed and released by the IARI in 2015 to study the long-term impact of climate change and crop management practices on yield.
    • InfoCrop is more suited for India as it has the life cycle data for almost all the local varieties of 11 crops: paddy, wheat, maize, sorghum, pearl millet, pigeon pea, chickpea, soybean, groundnut, potato and cotton.

    How does it work?

    • In InfoCrop, the parameters are already calibrated to Indian crop varieties and they are updated at regular intervals by the institute.
    • The parameters deal with aspects of-
    1. Weather (precipitation, temperature, radiation and others)
    2. Crop growth (phenology, grain characteristics, leaf growth, temperature and flooding sensitivity and others)
    3. Soil (texture and organic carbon, water holding characteristics and pH levels) and
    4. Pests and crop management (organic matter, fertiliser and irrigation).

    Efficiency of InfoCrop model

    • The model has an 85 per cent accuracy rate.
    • This is on par with widely used dynamic models such as the Decision Support System for Agrotechnology Transfer model, developed by the US, and Agriculture Production Systems sIMulator, developed by Australia.

    Utility of this tool

    • Prevent on-field corruption: India currently relies on field trials, which are expensive and resource-intensive as well as highly corrupt practise.
    • Crop insurance prediction: Government and insurance companies can use this for climate impact projections and for pre- or in-season crop yield forecasts to improve accuracy.
    • Assess crop loss: Besides forecasting, simulation models can be used to assess crop loss in the aftermath of an extreme weather event, which can then be used to provide relief packages.

     

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  • Reconstructing past Deep-Water Circulations of Indian Ocean

    indian ocean

    Studies have indicated that tectonically driven changes in the ocean gateways such as the closure of the Central American Seaway, a body of water that once separated North America from South America, since the late Miocene period, had a dramatic impact on the Indian Ocean circulation.

    What is Global overturning circulation (GOC)?

    • It is the equatorward transport of cold, deep waters and the poleward transport of warm, near-surface waters.
    • It controls ocean heat distribution and atmospheric carbon dioxide levels, thus playing a critical role in global climate.

    Concept: Panama Closure Hypothesis

    • This news essentially talks about the Panama Closure Hypothesis.
    • Panama Hypothesis states that the gradual closure of the Panama Seaway, between 13 million years ago (13 Ma) and 2.6 Ma, led to decreased mixing of Atlantic and Pacific water Masses.
    • This led to the formation of North Atlantic Deep water circulation.
    • It strengthened the Atlantic thermohaline circulation, increased temperatures and evaporation in the North Atlantic, increased precipitation in Northern Hemisphere high latitudes.

    Impact of Panama closure

    • It is thought that tectonic changes might have led to the formation of two separate water bodies — northern component water in the North Atlantic and Antarctic Bottom Water (AABW) in the Southern Ocean.
    • Consequently, it is also hypothesised that there would have been large-scale changes in the Deep Water Circulation (DWC) in the oceans across the world.

    Impact on Indian Ocean gyre

    • The Indian Ocean does not have any major deep-water formations of its own.
    • It acts only as a host for NCW and AABW.
    • Further, the northern parts of the Indian Ocean are located at one of the terminal ends of the GOC, far away from the deep-water formation regions and oceanic seaways.

    What has the new research found?

    • The scientists have generated an authigenic neodymium isotope record from the Arabian Sea and reconstructed the DWC record of the Indian Ocean for the period from 11.3 million years ago (Miocene era) to 1.98 million years ago (Pleistocene era).
    • The record shows a clear shift from the Pacific water-dominated deep circulation system before about nine million years ago, to the onset of a modern-like deep water circulation system in the Indian Ocean.
    • It comprises of Antarctic bottom water and northern component water during the Miocene-Pliocene transition (about six million years ago).
    • This suggests a widespread impact of the late Miocene Central American Seaway closure on the evolution of ocean deep water circulation and validates the so-called Panama Closure Hypothesis.

    Back2Basics: Indian Ocean Circulation

    indian ocean

    • The Indian Ocean circulation/gyre, located in the Indian Ocean, is one of the five major oceanic gyres, large systems of rotating ocean currents, which together form the backbone of the global conveyor belt.
    • The Indian Ocean gyre is composed of two major currents: the South Equatorial Current, and the West Australian Current.
    • Normally moving counter-clockwise, in the winter the Indian Ocean gyre reverses direction due to the seasonal winds of the South Asian Monsoon.

    How does it function?

    • In the summer, the land is warmer than the ocean, so surface winds blow from the ocean to the land.
    • However, during the winter, these temperatures reverse, making the winds blow from the land to the ocean.
    • Because most of the air pressure gradient is retained behind the Tibetan plateau, air pressure gradients over the Indian Ocean and the gyre are small.
    • This results in winds of moderate strength, due to the protection from the full-force winds blowing off the Mongolian high-pressure region.
    • Because of these moderate, dry winds, the Winter Monsoon season in the Indian Ocean region is the dry season for most of Southern Asia.
    • Due to this seasonal wind cycle, the currents of the Indian Ocean, which make up the Indian Ocean gyre, are directly affected, causing reversal.

     

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  • 129th birth anniversary of Satyendra Nath Bose

    satyendra nath bose

    Born on January 1, 1894, Bose collaborated with Einstein to develop what we now know as the Bose-Einstein statistics. We take a look at the Indian physicist’s illustrious legacy and stellar achievements.

    Satyendra Nath Bose

    • Born on January 1, 1894, Bose grew up and studied in Kolkata, where he solidified his position as an exemplary academician.
    • His father, an accountant in the Executive Engineering Department of the East Indian Railways, gave him an arithmetic problem to solve every day before going to work, encouraging Bose’s interest in mathematics.
    • By the age of 15, he began pursuing a Bachelor of Science degree at the Presidency College, and later finished his MSc in Mixed Mathematics in 1915.

    Career as researchers

    • These were tough times for Indian researchers as World War I had broken out and, European scientific journals came to India quite infrequently.
    • Not only this, most of the research papers weren’t available in English and both Bose and Saha had to learn scientific terms in German and French languages to read published works.
    • However, the new skill came in handy for them in 1919, when they published English translations of Albert Einstein’s special and general relativity papers.
    • Two years later, Bose was appointed to the position of Reader in Physics at the University of Dhaka. It was here that he made his most significant contributions to physics.

    Association with Einstein

    • Bose wrote a letter to Albert Einstein in 1924 about his breakthrough in quantum mechanics.
    • He claimed that he had derived Planck’s law for black body radiation (which refers to the spectrum of light emitted by any hot object) without any reference to classical electrodynamics.
    • Impressed by Bose’s findings, Einstein not only arranged for the publication of the paper but also translated it into German.
    • This recognition catapulted Bose to fame and glory.

    Breakthrough in the invention of Boson

    • He went on to work with Einstein and together they developed what is now known as the Bose-Einstein statistics.
    • Today, in honour of his legacy, any particle that obeys the Bose-Einstein statistics is called a boson.
    • On his 129th birth anniversary, we take a look at the Indian physicist’s illustrious legacy and stellar achievements.

     

     

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  • What are Globular Clusters?

    cluster

    Astronomers and scientists at the Indian Institute of Astrophysics (IIA) while studying the Omega Centauri have found that hot stars and white dwarfs emitted less ultraviolet radiation than expected.

    Omega Centauri

    • It is the most massive globular cluster system in our galaxy.
    • It was first identified as a non-stellar object by Edmond Halley in 1677 and as globular star cluster orbiting Milky Way galaxy by John Herschel in 1830s.
    • It contains approximately 10 million stars and is about 16,000 light-years away.
    • It also includes stars of a variety of ages, whereas other globular clusters contain stars from only one generation.
    • It is the largest and brightest globular cluster in the Milky Way.

     What is a globular cluster?

    • A globular cluster is a spheroidal conglomeration of stars.
    • Globular clusters are bound together by gravity, with a higher concentration of stars towards their centres.
    • They can contain anywhere from tens of thousands to many millions of member stars.
    • They orbit mostly in the extended stellar halos surrounding most spiral galaxies.

    How are they formed?

    • No one knows precisely how globular clusters formed. Or what role, if any, they played in the development of galaxies.
    • We know globular clusters are the oldest, largest and most massive type of star cluster. And globular clusters contain the oldest stars.
    • Their age is determined by their almost complete lack of what astronomers call metals, the heavier elements forged in star interiors.

    Our Milky Way has over 150 globular clusters

    • Our own Milky Way has over 150 globular clusters, with perhaps more, hidden by galactic dust.
    • The Andromeda galaxy (M31), our neighboring spiral galaxy, appears to have around 300 globular clusters.

    Difference between a globular cluster and an open cluster

    • Globular clusters are big, symmetric and old. They can reach 300 light-years in diameter and contain 10 million stars.  On the other hand, open star clusters, contains sibling stars, scattered through the disk of our galaxy and presumably other galaxies.
    • Globular star cluster are very symmetrical in shape, and are densest toward their centers. Open star clusters are irregular in shape and loosely grouped together.
    • Globular clusters orbit in the halo of our galaxy. Plus, center around the galaxy’s core and expanding above and below the galactic disk. Open star clusters tend to orbit within the disk.
    • Globular star clusters contain million of stars. Yet some globular clusters, like Omega Centauri, contain millions of stars. Open star clusters contain only hundreds of stars.

     

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  • What is a Trisonic Wind Tunnel?

    tunnel

    The new trisonic wind tunnel at the Vikram Sarabhai Space Centre (VSSC) was inaugurated by conducting the first blow-down test successfully.

    What is a Wind Tunnel?

    • Wind tunnels are large tubes with air moving inside.
    • The tunnels are used to copy the actions of an object in flight.
    • Researchers use wind tunnels to learn more about how an aircraft will fly.
    • Space agencies uses wind tunnels to test scale models of aircraft and spacecraft. Some wind tunnels are big enough to hold full-size versions of vehicles.
    • The wind tunnel moves air around an object, making it seem like the object is really flying.

    How do Wind Tunnels work?

    • Most of the time, powerful fans move air through the tube.
    • The object to be tested is fastened in the tunnel so that it will not move.
    • The object can be a small model of a vehicle. It can be just a piece of a vehicle.
    • It can be a full-size aircraft or spacecraft. It can even be a common object like a tennis ball.
    • Smoke or dye can be placed in the air and can be seen as it moves. Threads can be attached to the object to show how the air is moving.
    • Special instruments are often used to measure the force of the air on the object.

    About Trisonic Wind Tunnel at VSCC

    • ‘Trisonic’ refers to the tunnel’s capability to test in three speed regimes—below the speed of sound (subsonic), at the speed of sound (transonic), and above the speed of sound (supersonic).
    • Its parts include air storage vessels, a settling chamber where the airflow is ‘smoothened’ out, and nozzles for releasing the air into the test section.
    • It is about 160 metres long and measures 5.4 metres at its widest part.
    • In a ‘blow down test’, stored gases are released and blown through the tunnel’s test section, simulating flight conditions.
    • The tunnel can simulate flight conditions from 0.2 times the speed of sound (68 metres per second) to four times the speed of sound (1,360 metres per second), according to the space agency.
    • Commissioned in 2017, this tunnel can simulate flow speeds up to Mach 12.

     

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