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GS Paper: GS3-17.Awareness in the fields of IT, Space, Computers, Robotics, Nano-technology, Bio-technology and issues relating to Intellectual Property Rights.

  • International Moon Day

    Why in the News?

    Observed every year on July 20, the International Moon Day marks the historic first human landing on the Moon by the Apollo 11 mission in 1969.

    moon day

    About International Moon Day:

    • Date & Purpose: Observed annually on July 20 to mark the Apollo 11 Moon landing in 1969.
    • UN Recognition: Declared by the UN General Assembly in 2021 on the recommendation of COPUOS.
    • First Observance: Officially celebrated for the first time on July 20, 2022.
    • Activities: Includes sky-gazing, science outreach, and student competitions to promote space awareness.
    • Date Controversy: While the lunar module landed on July 20, Neil Armstrong stepped onto the Moon at 2:56 UTC on July 21—yet July 20 remains the official date.

    Significance:

    • Historic Milestone: Celebrates Apollo 11 and humanity’s first step on the Moon by Neil Armstrong and Buzz Aldrin.
    • Peaceful Space Use: Promotes the Moon as a shared heritage and fosters international cooperation in outer space.
    • Sustainability Focus: Encourages responsible and eco-friendly exploration of lunar resources.
    • Global Unity: Reflects the UN’s vision of peaceful space collaboration under themes like “One Moon, One Vision, One Future”.
    [UPSC 2009] India has recently landed its Moon Impact Probe on the Moon. Among the following countries, which one landed such probe on the Moon earlier?

    Options: (a) Australia (b) Canada (c) China* (d) Japan

     

  • Successful trial of Akash Prime Air Defence System

    Why in the News?

    India successfully tested the Akash Prime Missile System in Ladakh, neutralizing two high-speed aerial targets at high altitude.

    About Akash Prime:

    • What It Is: Akash Prime is an upgraded version of the Akash Surface-to-Air Missile (SAM) system.
    • High-Altitude Capability: Designed to operate effectively above 4,500 metres.
    • Development: Developed by DRDO with BDL, BEL, and Army Air Defence.
    • Operational Use: Proven in Operation Sindoor against aerial threats.
    • Production Trials: Validated through First of Production Model (FoPM) firing trials.
    • Deployment: Already in use at IAF bases and forward posts along the LAC in Ladakh.

    Key Features:

    • Seeker Upgrade: Equipped with an indigenous active Radio Frequency (RF) seeker for better accuracy.
    • Altitude Adaptability: Engineered for high-altitude, cold-climate operations.
    • Multi-Target Engagement: Capable of engaging multiple aerial threats at once.
    • Speed & Accuracy: Travels at Mach 2.5 with up to 90% kill probability.
    • Electronic Warfare: Equipped with ECCM features to resist electronic jamming.
    • Radar Integration: Uses Rajendra radar for detection, targeting, and tracking.
    • Operational Range: Effective engagement range of 25–30 km.

    Other Variants of Akash:

    • Akash Mark-I (1990–2005): First version under IGMDP; achieved successful dual-target intercepts by 2005.
    • Akash-1S (2019): Enhanced version with 30 km range and 60 kg warhead; effective against aircraft and drones; tested successfully in May 2019.
    • Akash Prime (2021 onwards): Added active RF seeker and altitude/weather resistance; tested on September 27, 2021.
    • Akash-NG (Next Generation): Approved in 2016 with ₹470 crore funding; offers faster response and improved aerial threat protection.

     

    [UPSC 2009] In the context of Indian defence, consider the following statements:

    1. The Shourya missile flies with a speed of more than 8 Mach. 2. The range of Shourya missile is more than 1600 km. Which of the statements given above is/are correct ?

    Options: (a) 1 only (b) 2 only (c) Both 1 and 2 (d) Neither 1 nor 2*

     

  • IIST Scientists detected Circular Polarisation near massive Protostar

    Why in the News?

    Researchers at the Indian Institute of Space Science and Technology (IIST) has detected radio emissions with circular polarisation near a massive young protostar, IRAS 18162-2048.

    About Protostars:

    • Definition: Early-stage stars formed by the gravitational collapse of dense regions in molecular clouds.
    • Accretion Phase: They actively gather gas and dust but have not yet begun sustained nuclear fusion.
    • Jet Ejection: Bipolar jets—high-speed streams of particles—are commonly emitted from their poles.
    • Massive Protostars: Expected to evolve into stars with masses over 8–10 times that of the Sun.
    • Role of Magnetism: Magnetic fields likely influence both jet formation and ejection mechanisms.

    About the Protostar IRAS 18162-2048:

    • Overview: Situated about 4,500 light years away in the Milky Way.
    • Jet Feature: Powers the HH80-81 jet—one of the galaxy’s largest and brightest protostellar jets.
    • Magnetic Detection: First direct evidence of magnetic fields from the protostar itself, not just its jet.
    • Observation Challenges: Heavily shrouded in dense gas and dust, making traditional observation difficult.
    • Jet Dynamics: Suggests that magnetic fields and rotational energy drive its development.

    Recent Observations:

    • Detection Method: Observed circular polarisation in radio waves—where electromagnetic fields rotate along their path.
    • Rarity: Circular polarisation is extremely faint and seldom detected, even in intense sources like active galactic nuclei.
    • Scientific Milestone: First-ever estimation of magnetic field strength near a massive protostar using circular polarisation.
    • Magnetic Field Strength: Estimated to be 100 times stronger than Earth’s magnetic field.
    • Theoretical Support: Findings reinforce the theory that magnetic fields power jets from both stars and black holes.
    [UPSC 2023] Consider the following pairs:

    Objects in space :: Description

    1. Cepheids : Giant clouds of dust and gas in space

    2. Nebulae : Stars which brighten and dim periodically

    3. Pulsars : Neutron stars that are formed when massive stars run out of fuel and collapse How many of the above pairs are correctly matched?

    Options: (a) Only one* (b) Only two (c) All three (d) None

     

  • GW231123: Biggest Black Hole Merger Detected

    Why in the News?

    Researchers have reported the detection of an exceptionally massive black hole merger, labelled GW231123.

    GW231123: Biggest Black Hole Merger Detected

    About Black Holes and Black Hole Merger:

    • Overview: Black holes are extremely dense celestial objects whose gravitational pull is so strong that even light cannot escape.
    • Types of Black Holes:
      1. Stellar-mass: Around 20 times the mass of the Sun or more.
      2. Intermediate-mass: Between 100 and 100,000 times the mass of the Sun.
      3. Supermassive: From 100,000 to several billion times the mass of the Sun.
    • Black Hole Merger:
      • Occurs when two black holes orbit each other, lose energy via gravitational waves, and merge into a larger black hole.
      • The GW231123 event involved black holes of approximately 140 and 100 solar masses, forming a final black hole of 225 solar masses — the largest detected through gravitational waves.
      • Scientists suggest such massive black holes may form via hierarchical mergers (successive black hole mergers).
      • Supports theories on the formation of supermassive black holes, often found at galactic centers.

    Recent Observations:

    • Event Timing: The GW231123 event was detected on November 23, 2023, though it occurred billions of years ago.
    • Signal Characteristics:
      • Lasted only a tenth of a second but matched Einstein’s predictions under General Relativity.
      • Both black holes were rapidly spinning, hinting at a complex formation history.
    • Scientific Significance:
      • Involved intermediate-mass black holes, rarely observed in nature.
      • Challenges existing models of black hole formation via stellar collapse.
      • Indicates the presence of black holes in the so-called “forbidden mass gap”.
    • Conference Presentation:
      • Findings to be presented at the 24th International Conference on General Relativity and Gravitation (GR24) and the 16th Edoardo Amaldi Conference on Gravitational Waves, held in Glasgow, UK (July 14–18, 2025).
    • Broader Implications:
      • Opens new questions about the origin of massive black holes.
      • Offers insights into gravitational physics, cosmology, astrophysics, and potentially particle physics or cosmic string theory.
      • Model refinements are ongoing to better understand such extreme cosmic phenomena.

    Gravitational Wave Detection Network:

    • Nature of Gravitational Waves: Invisible ripples in spacetime caused by cataclysmic cosmic events like black hole collisions; predicted by Einstein in 1916.
    • Global Detection Network (LIGO–Virgo–KAGRA):
      • Laser Interferometer Gravitational-Wave Observatory (LIGO):
        • Operates two detectors in the United States (in the states of Louisiana and Washington).
        • First detected gravitational waves in 2015, leading to a Nobel Prize in Physics in 2017.
      • Virgo Observatory: Located near Pisa, Italy and operated by the European Gravitational Observatory.
      • Kamioka Gravitational Wave Detector (KAGRA): Located underground in the Kamioka mine, Japan, and notable for its cryogenic mirror technology.
    • LIGO-India:
      • Under construction in Hingoli, Maharashtra in partnership with the US National Science Foundation.
      • Involves scientists from 17 Indian institutions.
    [UPSC 2019] Recently, scientists observed the merger of giant ‘blackholes’ billions of light-years away from the Earth.

    What is the significance of this observation?

    Options: (a) Higgs boson particles’ were detected. (b) Gravitational waves’ were detected * (c) Possibility of inter-galactic space travel through ‘wormhole’ was confirmed. (d) It enabled the scientists to understand ‘singularity’.

     

  • Mysterious Antimatter Physics discovered at CERN Large Hadron Collider

    Why in the News?

    CERN scientists have detected a tiny but significant difference in how matter and antimatter versions of baryons behave — offering clues to why matter dominates the universe, despite both being created equally after the Big Bang.

    What is CERN’s LHCb Experiment?

    • Location: At the Large Hadron Collider near Geneva, on the France–Switzerland border.
    • Name: LHCb = Large Hadron Collider beauty; focuses on beauty (bottom) quarks.
    • Started: Built in early 2000s; began collecting data in 2009.
    • Purpose: Studies particle decay, especially of beauty quark-containing particles, to test the Standard Model and search for small anomalies.

    Matter vs Antimatter – The Big Puzzle:

    • Matter: Everything around us is made of it.
    • Antimatter: Mirror image of matter, with opposite charges.
    • Big Bang Theory: Both should have been produced equally — and destroyed each other.
    • But…: Only matter remains — a mystery science is still trying to solve.
    • CP Symmetry: Physics expects matter and antimatter to behave identically (Charge-Parity symmetry).
    • CP Violation: When this symmetry breaks — possibly explaining why matter survived.

    What did Scientists Discover?

    • Focus: Lambda-b baryons and their antimatter versions.
    • Finding: A small but clear CP violation — they decayed differently.
    • Significance: First such discovery in baryons (previously seen only in mesons).
    • Certainty: Highly reliable — only 1 in 3.5 million chance it’s random.

    Why is this Important?

    • Helps explain why the universe is made of matter.
    • Expands discovery of CP violation to heavier particles.
    • Could hint at physics beyond the Standard Model.
    • Moves us closer to solving one of the universe’s biggest mysteries.
    [UPSC 2013] The efforts to detect the existence of Higgs boson particle have become frequent news in the recent past. What is/are the importance/importances of discovering this particle?

    1. It will enable us to under-stand as to why elementary particles have mass. 2. It will enable us in the near future to develop the technology of transferring matter from one point to another without traversing the physical space between them. 3. It will enable us to create better fuels for nuclear fission.

    Select the correct answer using the codes given below.

    Options: (a) 1 only* (b) 2 and 3 only (c) 1 and 3 only (d) 1, 2 and 3

     

  • [pib] Breakthrough in Quantum Noise Research

    Why in the News?

    Researchers at the Raman Research Institute (RRI) found that quantum noise—usually seen as a problem—can sometimes help connect particles in a special way called entanglement, which is important for future quantum technologies.

    What is Quantum Noise?

    • Overview: Quantum noise refers to random disturbances that affect quantum systems, often causing loss of coherence or decoherence.
    • Traditional View: It is typically seen as harmful, especially for quantum entanglement, which is crucial for quantum computing and communication.
    • Entanglement Concept: It is a phenomenon where particles are so correlated that the state of one instantly affects the state of another, even at a distance.
    • Effect of Decoherence: Noise-induced decoherence breaks this entanglement, thereby reducing the efficiency of quantum technologies.

    Key Findings:

    • Observation: Found that quantum noise can generate or revive entanglement, contrary to its typical reputation as destructive.
    • Focus Area: Studied intraparticle entanglement, which involves internal properties (like spin and path) of a single particle.
    • Contrast with Interparticle Entanglement: Unlike interparticle entanglement (between separate particles), intraparticle entanglement showed resilience under noise.
    • Types of Noise Studied:
      • Amplitude Damping: Energy loss
      • Phase Damping: Loss of phase information
      • Depolarizing Noise: Random changes in quantum state
    • Major Observation: Under amplitude damping, intraparticle entanglement showed delayed decay, revival, and even creation from unentangled states.
    • Interparticle Comparison: In contrast, interparticle entanglement exhibited steady decay with no revival or generation.

    Scientific Implications:

    • New Perspective: Challenges the assumption that quantum noise is purely harmful, showing it can be a resource in certain contexts.
    • Technological Potential: Intraparticle entanglement is more noise-resilient, making it valuable for stable quantum devices.
    • Application Areas: Findings are relevant to quantum communication, QKD (quantum key distribution), quantum computing, and quantum sensing.
    • Predictive Advantage: The new formula allows precise prediction of entanglement behavior, aiding the design of robust systems.
    • Platform Independence: Results are platform-agnostic, applicable to photons, neutrons, trapped ions, etc.
    [UPSC 2025] Consider the following statements:

    I. It is expected that Majorana 1 chip will enable quantum computing. II. Majorana 1 chip has been introduced by Amazon Web Services (AWS). III. Deep learning is a subset of machine learning.

    Which of the statements given above are correct?

    (a) I and only I (b) II and III only (c) I and III only * (d) I, II and III

     

  • Scientists decode Locust Pheromones for Eco-Friendly Control

    Why in the News?

    Researchers in China have discovered a method to curb locust swarming by manipulating their pheromones, paving the way for eco-friendly locust control.

    What are Locust Swarms?

    • Locusts are large grasshoppers capable of forming massive swarms, consuming up to their body weight in food daily, and travelling 150 km/day with favourable winds.
    • They are highly destructive, stripping crops and threatening food security. A single swarm can consume food equivalent to the daily needs of 35,000 people.
    • In India, Locust Control and Research (LC&R) oversees locust management.
    • The Locust Warning Organisation (LWO), established in 1939, monitors and controls locust activity in states like Rajasthan, Gujarat, Punjab, and Haryana.
    • The 2019-2022 desert locust outbreak was one of the worst in decades, devastating India, Pakistan, and East Africa, destroying over 200,000 hectares of crops.
    • Despite existing control measures, locust outbreaks remain difficult to manage due to their rapid breeding capabilities.

    About Locust Pheromones:

    • Locust Behavioural Phases: Locusts exhibit two behavioural phases—solitary (non-swarming) and gregarious (swarming). The shift to gregariousness leads to swarm formation.
    • Key Pheromone – 4-Vinylanisole (4VA):
      • Identified in 2020 by Chinese researchers.
      • Released from locusts’ hind legs after feeding, especially due to the digestion of phenylalanine (a plant compound).
      • Acts as an aggregation pheromone, attracting other locusts and triggering group behaviour.
    • Biochemical Pathway:
      • Enzymes 4VPMT1 (dominant) and 4VPMT2 convert a precursor molecule (4VP) into 4VA.
      • This process is crucial in converting solitary locusts into swarm-forming gregarious ones.

    Recent Breakthrough and Its Implication:

    • Discovery: Researchers at the Chinese Academy of Sciences genetically blocked 4VPMT1, preventing locusts from producing 4VA and stopping swarm formation.
    • Limitations: 4NP is toxic and environmentally persistent, raising concerns for large-scale deployment.
    • Strategy Proposed: RNA interference (RNAi)-based biopesticides targeting 4VPMT genes to prevent 4VA production without toxicity.
    • Wider Implications:
      • Marks the first pollution-free molecular approach to locust control.
      • Can reduce reliance on synthetic pesticides, protect crops, and support sustainable agriculture.
      • Offers a precision pest control model based on insect behavioural biochemistry.
    [UPSC 2001] American multinational company, Monsanto has produced an insect-resistant cotton variety that is undergoing field- trials in India. A toxin gene from which ONE of the following bacteria has been transferred to this transgenic cotton ?

    Options: (a) Bacillus subtilis (b) Bacillus thurigiensis* (c) Bacillus amyloliquifanciens (d) Bacillus globlii

     

  • What are Optical Atomic Clocks?

    Why in the News?

    Researchers conducted the most precise global comparison of 10 Optical Atomic Clocks to pave the way for redefining the second by 2030, replacing Caesium Clocks with more accurate Optical ones.

    Definition of a Second:

    • The current SI unit of time is based on caesium-133 (Cs) atomic clocks.
    • In 1967, one second was defined as the duration of 9,192,631,770 cycles of radiation corresponding to the transition between two hyperfine levels of the ground state of a Cs-133 atom.
    • In these clocks, a microwave signal is tuned until Cs atoms react maximally, ensuring the frequency is precisely 9,192,631,770 Hz.
    • Frequency dividers count this microwave frequency, providing one tick per second, thus realizing the SI second.

    About Caesium Atomic Clocks:

    • Overview: Caesium atomic clocks are devices that define the current SI unit of time (second) using the oscillation frequency of caesium-133 atoms.
    • SI Second Standard: One second is defined as the duration of 9,192,631,770 cycles of microwave radiation corresponding to the transition between two energy levels of the caesium-133 atom.
    • Working Principle: These clocks work by tuning microwave signals to resonate with caesium atoms and then counting the resulting waves to measure time precisely.
    • Stability and Usage: They are highly stable and have been used since 1967 to set international time standards.
    • Applications: They are used in GPS systems, telecommunications, scientific research, and by national metrology institutions like India’s National Physical Laboratory (NPL).
    • Accuracy: A typical caesium atomic clock loses about one second every 300 million years.

    What are Optical Atomic Clocks?

    • Overview: They are advanced timekeeping devices that use optical (visible light) frequency transitions in atoms like Strontium (Sr) or Ytterbium (Yb).
    • Measurement Basis: These clocks measure time based on the oscillation of light emitted when atoms transition between energy levels at hundreds of trillions of Hz.
    • Example Frequencies:
      • Strontium: ~429 trillion Hz
      • Ytterbium ions: over 642 trillion Hz
    • Precision Tools: They require lasers and optical frequency combs to count these rapid oscillations accurately.
    • Future Standard: They are being tested worldwide and are expected to replace caesium clocks by 2030 for redefining the SI second.

    How Optical Atomic Clocks are Better than Caesium ones?

    • Higher Frequency Operation: Optical clocks operate at much higher frequencies, allowing division of time into finer intervals.
    • Improved Precision: By counting 10,000 times more oscillations per second, optical clocks achieve significantly higher precision and stability.
    • Unmatched Accuracy: An optical atomic clock using strontium reportedly drifts by less than one second in 15 billion years, compared to 300 million years for caesium clocks.
    • Advanced Applications: Their precision is critical for: Next-gen GPS systems, Gravitational wave detection, Climate monitoring and research etc.
    • Ultra-High Synchronization: Optical clocks enable cross-continental synchronization at 18 decimal place accuracy, essential for global time coordination.
    • Noise Resilience: They offer greater resistance to environmental noise and external disturbances, improving long-term reliability.
    [UPSC 2023] Which one of the following countries has its own Satellite Navigation System?

    Options: (a) Australia (b) Canada (c) Israel (d) Japan*

     

  • Vera C Rubin Observatory 

    Why in the News?

    The Vera C. Rubin Observatory has recently begun a 10-year project to study dark matter and dark energy using a 3,200-megapixel camera (of the Simonyi Survey Telescope) from its site in the Chilean Andes.

    Vera C Rubin Observatory 

    About Vera C. Rubin Observatory:

    • Location: The Vera C. Rubin Observatory is situated on Cerro Pachón in the Chilean Andes, at an altitude of 8,684 feet.
    • Naming: It is named after Vera C. Rubin, the astronomer who first provided robust observational evidence for the existence of dark matter in the 1970s.
    • Survey Duration: The observatory will carry out a 10-year continuous survey of the entire southern sky.
    • Data Volume: It is designed to collect approximately 20 terabytes of astronomical data per night.
    • Observation System: The telescope operates using an automated scripting system that selects observation targets dynamically, rather than through manual scheduling.
    • Objectives: Its key goals include understanding the formation of galaxies, identifying a possible ninth planet, detecting potentially hazardous asteroids, and studying the nature of dark matter and dark energy.

    Key Features:

    • Telescope Design: The observatory uses the Simonyi Survey Telescope, which features a three-mirror optical system for wide-field imaging.
    • How big is it: It has a field of view of 9.6 square degrees (compared to 0.04 sq. deg. for Hubble and 0.11 sq. deg. for James Webb), a 3,200-megapixel camera (vs. Hubble’s ~1.0 MP).
    • Field of View: It can capture a field of view equivalent to 40 full Moons in a single exposure — far wider than traditional space telescopes.
    • Spectral Filters: The camera includes six optical filters that capture data from across the electromagnetic spectrum, including ultraviolet and infrared light.
    • Slewing Speed: The telescope is the fastest-moving large telescope, capable of repositioning and stabilizing in just 5 seconds.
    • Imaging Frequency: It can take up to 1,000 images per night, allowing it to scan the entire sky every three nights.
    • Change Detection: Its automated software compares new and old images to detect changes, issuing up to 10 million alerts per night for transient astronomical events.

    Breakthrough Discoveries:

    • First Light: The observatory released its first test images on June 23, 2025.
    • Initial Discoveries: Within 10 hours of collecting engineering data, it identified 2,104 new asteroids, including 7 near-Earth objects (NEOs).
    • Expected Discoveries: Over the full 10-year mission, it is projected to discover over 5 million asteroids and around 100,000 NEOs.
    • Impact on Database: These findings would triple the current global inventory of known asteroids.
    • Universe Mapping: The observatory will produce the most detailed map of the large-scale structure of the universe to date.
    • Dark Matter Study: The data will support analysis of dark matter, which constitutes 27% of the universe’s composition.
    • Dark Energy Study: It will also help scientists understand dark energy, which makes up 68% of the universe and drives cosmic expansion.
    • Visible Matter Context: Only 5% of the universe is composed of visible matter, making the observatory’s data essential to studying the remaining 95%.
    [UPSC 2002] The world’s highest ground-based telescopic observatory is located in:

    Options: (a) Colombia (b) India (c) Nepal (d) Switzerland

     

  • How Heat led to Protocells formation on Earth?

    Why in the News?

    A new Nature Physics study suggests that warm volcanic rock surfaces may have concentrated organic molecules in watery cracks, triggering life-like chemistry—offering a clue to how protocells formed without membranes before life began.

    What are Protocells?

    • Overview: Protocells are primitive, cell-like bubbles believed to be early precursors of real biological cells. They were not fully alive but provided a space for early chemical interactions.
    • Lack of Complexity: These structures lacked complex parts like organelles or DNA systems but could hold important molecules like RNA and amino acids together.
    • Membrane Role: Protocells often formed simple membranes or boundaries, which allowed molecules to stay enclosed and interact more easily—helping early reactions like protein synthesis happen.
    • Importance: Although not living, they offered a model of how basic chemistry could evolve into biology, bridging the gap between non-living and living systems.

    History of Formation of Protocells:

    • Early Earth Conditions: Over 3.5 billion years ago, Earth’s surface had warm water pools and volcanic cracks filled with organic molecules made by natural processes like lightning.
    • Compartmentalization: The first step toward life was concentrating useful molecules in one place, so they could start reacting—this led to the idea of bubble-like protocells.
    • Old Theories: In the 1920s, Oparin and Haldane proposed that life began in a “primordial soup” with spontaneous chemical reactions in early Earth’s oceans.
    • Modern Insights: Newer research suggests cracks in volcanic rock or hydrothermal vents created temperature gradients and water flows that helped form protocells—no complex membranes were needed.

    Key Findings in the 2025 Study:

    • Lab Setup: Scientists created a 170-micrometre chamber with a warm top (40°C) and cool bottom (27°C), simulating early Earth rock cracks.
    • DNA Test: They added DNA and a protein-making kit (PURExpress). Only in the warm-cool chamber did the DNA make green fluorescent protein (GFP), showing real protein synthesis.
    • Molecule Gathering: Essential items like DNA, magnesium, and phosphate ions gathered more at the bottom—up to 70 times more concentrated than at the top.
    • Cell-Like Behavior: Even without a membrane, the system kept useful molecules inside while letting waste escape, mimicking real cell selectivity.
    • Big Implication: This experiment supports the idea that life could start in simple natural environments using just heat, flow, and basic chemicals—long before full cells appeared.
    [UPSC 2018] Consider the following statements:

    1. The Earth’s magnetic field has reversed every few hundred thousand years.

    2. When the Earth was created more than 4000 million years ago, there was 54% oxygen and no carbon dioxide.

    3. When living organisms originated, they modified the early atmosphere of the Earth. Which of the statements given above is/are correct?

    Options: (a) 1 only (b) 2 and 3 only (c) 1 and 3 only * (d) 1, 2 and 3