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Subject: Space Technology

  • What is Planetary Alignment?

    Why in the News?

    On February 29, 2024, skywatchers worldwide witnessed a rare planetary alignment (parade) with seven planets—Mars, Jupiter, Uranus, Neptune, Mercury, Saturn, and Venus—lining up in the night sky.

    What is Planetary Alignment?

    • A planetary alignment occurs when multiple planets in the Solar System appear to line up in the sky as seen from Earth.
    • This phenomenon happens because planets orbit the Sun in a flat, disc-shaped plane called the ecliptic.
    • Although planets remain millions of kilometers apart, they seem to form a straight line from Earth’s perspective due to optical illusion and perspective.
    • The term “planet parade” is also used to describe this occurrence when multiple planets become visible in the sky at the same time.
    • Types of Planetary Alignments:
    1. Conjunction: Two or more planets appear close to each other in the sky.
    2. Small Alignment: Three planets align in a visible line.
    3. Large Alignment: Four or more planets appear aligned from Earth’s perspective.
    4. Full Alignment: All eight planets of the Solar System appear in a single line (very rare).

    How often do Planetary Alignments occur?

    • Planetary alignments are not uncommon, but their rarity depends on the number of planets involved.
      • Two- or Three-Planet Alignments: Occur multiple times a year.
      • Four- or Five-Planet Alignments: Visible every few years.
      • Six- or Seven-Planet Alignments: Appear every few decades.
      • Full Alignment (All Eight Planets): Extremely rare, occurs once every 170–200 years.
    • Recent & Upcoming Alignments:
      • August 2025: Expected four-planet alignment.
      • May 2492: The next predicted full planetary alignment of all eight planets.

    PYQ:

    [2019] On 21st June, the Sun:

    (a) does not set below the horizon at the Arctic Circle
    (b) does not set below the horizon at Antarctic Circle
    (c) shines vertically overhead at noon on the Equator
    (d) shines vertically overhead at the Tropic of Capricorn

     

  • ‘Blue Ghost’ Mission 1

    Why in the News?

    US’s Firefly Aerospace’s Blue Ghost Mission 1 successfully landed on the Moon, becoming the second private mission to do so and the first to land upright.

    What is ‘Blue Ghost’ Mission 1?

    • Blue Ghost Mission 1 is a private lunar landing mission by Firefly Aerospace under NASA’s Commercial Lunar Payload Services (CLPS) program.
    • It was launched aboard a SpaceX Falcon 9.
    • It successfully landed on the Moon, at Mons Latreille, Mare Crisium.
    • The mission is designed to operate for 14 Earth days (one lunar day).

    Key Features of Blue Ghost Mission 1:

    • Carries 10 scientific instruments, including a lunar soil analyzer, a radiation-tolerant computer, and a GPS-based navigation experiment to test satellite navigation on the Moon.
    • Equipped with a high-definition imaging system to capture a lunar eclipse (March 14, 2024) and lunar sunset (March 16, 2024).
    • Successfully navigated a rocky and cratered surface using hazard-avoidance technology, slowing from thousands of miles per hour to just two mph before touchdown.
    • The lander is golden in color and about the size of a hippopotamus.
    • It supports Artemis missions by testing lunar technologies and reducing costs for future human exploration.

    PYQ:

    [2016] What is ‘Greased Lightning-10 (GL-10)’, recently in the news?

    (a) Electric plane tested by NASA

    (b) Solar-powered two-seater aircraft designed by Japan

    (c) Space observatory launched by China

    (d) Reusable rocket designed by ISRO

     

  • PUNCH Mission

    Why in the News?

    NASA is set to launch the Polarimetry to Unify the Corona and Heliosphere (PUNCH) mission on February 28, 2025, aboard a SpaceX Falcon 9 rocket.

    About the PUNCH Mission

    • PUNCH Mission is a groundbreaking solar mission designed to study the Sun’s corona and solar wind using advanced imaging techniques.
    • It will consist of 4 small satellites operating in Low Earth Orbit (LEO) for an expected two-year mission.
    • Unlike previous missions, PUNCH will use polarimetry (measurement of polarized light) to observe solar phenomena in 3D.
    • It allows scientists to study the origin and evolution of solar winds and Coronal Mass Ejections (CMEs), both of which impact space weather and Earth’s technological systems.
    • Focus Areas of the PUNCH Mission:
      • Study how the Sun’s outer corona transforms into the solar wind.
      • Observe how CMEs are formed, gain speed, and travel through space.
      • Improve space weather forecasting to protect satellites, astronauts, and power grids.
      • Provide real-time data to help scientists predict solar storms and geomagnetic disturbances.
      • Contribute to NASA’s Artemis program by ensuring safe deep-space exploration.

    Key Features of the PUNCH Mission:

    • 4 microsatellite weighs 64 kg each and works together to capture a wide-field view of the Sun’s corona.
    • Advanced Imaging Instruments:
      • Narrow Field Imager (NFI):  Captures high-resolution images of the inner corona.
      • Wide Field Imagers (WFIs):  Observe solar wind and CMEs across interplanetary space.
      • STEAM (X-ray spectrometer): Monitors coronal heating and solar flares.
    • Provides real-time data every four minutes.
    • Offers a 90° field of view, covering the Sun’s outer atmosphere and heliosphere.
    • Helps mitigate the effects of solar storms on Earth’s communication systems.
    • Aids in protecting astronauts and satellites from harmful solar radiation.

    PYQ:

    [2022] If a major solar storm (solar flare) reaches the Earth, which of the following are the possible effects on the Earth?

    1. GPS and navigation systems could fail.
    2. Tsunamis could occur at equatorial regions.
    3. Power grids could be damaged.
    4. Intense auroras could occur over much of the Earth.
    5. Forest fires could take place over much of the planet.
    6. Orbits of the satellites could be disturbed.
    7. Shortwave radio communication of the aircraft flying over polar regions could be interrupted.

    Select the correct answer using the code given below:

    (a) 1, 2, 4 and 5 only
    (b) 2, 3, 5, 6 and 7 only
    (c) 1, 3, 4, 6 and 7 only
    (d) 1, 2, 3, 4, 5, 6 and 7

     

  • SPHEREx Telescope

    Why in the News?

    NASA is set to launch its latest space telescope, SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) aboard a SpaceX Falcon 9 rocket from California.

    What is the SPHEREx Telescope?

    • SPHEREx is a new space telescope developed by NASA.
    • It is designed to map the entire sky in infrared light and provide insights into the origins of the universe, galaxy formation, and the distribution of life-forming molecules.
    • Its mission is expected to last 2 years, during which it will survey the sky 4 times.
    • Key Features of SPHEREx:
      • Infrared Spectroscopy: Unlike traditional optical telescopes, SPHEREx will capture the universe in 102 infrared colors, which are invisible to the human eye.
      • Wide-Sky Coverage: Unlike the James Webb Space Telescope (JWST), which focuses on narrow regions, SPHEREx will map the entire sky every 6 months.
      • High Data Output: It will collect data on one billion galaxies, 100 million stars, and 10,000 asteroids, creating an unprecedented cosmic map.
      • Study of Cosmic Inflation: SPHEREx will analyze the earliest moments after the Big Bang, helping scientists understand how the universe expanded rapidly in its infancy.
      • Search for Life-Forming Molecules: The telescope will identify biogenic molecules like water, carbon dioxide, and methanol in the Milky Way galaxy, revealing where the building blocks of life exist.

    SPHEREx Telescope

    How will SPHEREx Create the “Most Colourful” Map of the Cosmos?

    • Spectroscopic Imaging: SPHEREx will divide light from celestial objects into 96 infrared bands, significantly more than previous sky-mapping telescopes.
    • Mapping Galactic Evolution: By observing 450 million galaxies, SPHEREx will reveal how they evolved over cosmic history.
    • Identifying Cosmic Ice: The telescope will detect frozen water and organic molecules in interstellar dust clouds, essential for understanding planetary formation.
    • Unprecedented Infrared Insights: Unlike Hubble, which focuses on optical light, and JWST, which targets deep-space infrared observations, SPHEREx will capture broad infrared spectra across the entire sky, revealing hidden cosmic structures.

    PYQ:

    [2015] In the context of modern scientific research, consider the following statements about ‘IceCube’, a particle detector located at South Pole, which was recently in the news:

    1. It is the world’s largest neutrino detector, encompassing a cubic kilometre of ice.
    2. It is a powerful telescope to search for dark matter.
    3. It is buried deep in the ice.

    Which of the statements given above is/are correct?

    (a) 1 only

    (b) 2 and 3 only

    (c) 1 and 3 only

    (d) 1, 2 and 3

     

  • New Experiment to Test Quantum Gravity

    Why in the News?

    A new proposal published on October 29, 2024, suggests an experiment that could provide direct evidence for quantum gravity, unifying general relativity and quantum mechanics. A new experiment proposes testing weak gravitational fields at the quantum level, a historic breakthrough in physics if successful.

    What is Quantum Gravity?

    • Quantum Gravity is a theoretical framework that aims to unify general relativity (which explains gravity at large scales) and quantum mechanics (which governs subatomic particles).
    • Since gravity behaves differently from the other fundamental forces in quantum mechanics, physicists have been searching for a theory that integrates gravity into the quantum world.
    • General relativity treats gravity as the curvature of spacetime, while quantum mechanics describes forces through particle interactions.
    • Gravity has never been directly observed in quantum form, unlike the other fundamental forces.
    • Theories like String Theory and Loop Quantum Gravity attempt to explain quantum gravity but lack experimental validation.

    Significance of the Experiment

    • First Realistic Test for Quantum Gravity: Most quantum gravity theories rely on extreme conditions (e.g., black holes), making them impossible to test. This experiment provides a lab-based alternative.
    • Testing Gravity at the Quantum Level: If a small mass in quantum superposition is influenced by gravity, it could prove gravity itself is quantum in nature.
    • Weak Gravity Instead of Strong Gravity: Unlike previous studies focused on black holes, this experiment explores weak gravitational interactions, making it more feasible.
    • Towards a Unified Theory of Physics: Proving quantum gravity could merge general relativity and quantum mechanics, solving a major gap in modern physics.
    • Challenging Existing Theories: If results differ from both classical and quantum predictions, it could suggest a new force or a modified gravity theory.
  • First Detailed Map of Moon’s South Pole Area made from Chandrayaan Data

    Why in the News?

    Astronomers are studying the first detailed geological map of the Moon’s South Pole, created by India’s Chandrayaan-3’s Vikram lander, which landed on August 23, 2023.

    About the Geological Map of the Moon’s South Pole:

    • First High-Resolution Map:
      • This map is created by PRL Ahmedabad, Panjab University, and ISRO, using data from Chandrayaan-3’s Pragyan rover.
      • It offers new insights into the Moon’s formation and evolution.
    • Confirmation of a Magma Ocean:
      • Pragyan’s Alpha Particle X-ray Spectrometer detected molten rock beneath the surface.
      • This confirms a global magma ocean in the Moon’s early history.
    • Age and Crater Mapping:
      • Landing site estimated to be 3.7 billion years old, similar to Earth’s early evolution.
      • Schomberger Crater identified as the primary source of impact debris.
    • Importance for Lunar and Planetary Studies:
      • Preserved craters help understand the history of asteroid impacts.
      • Provides insights into the formation of the Earth-Moon system.

    Why is the Moon’s South Pole a Key Focus for Space Missions?

    • Water Ice Reserves:
      • Permanently shadowed craters hold large water ice deposits, first confirmed by Chandrayaan-1 (2009).
      • Crucial for future lunar colonies and deep-space missions.
    • Harsh but Valuable Environment:
      • Extreme cold (as low as -250°C) preserves ancient materials.
      • Continuous sunlight in some areas makes it ideal for solar power.
    • Scientific and Strategic Importance:
      • Craters contain pristine material from the early Solar System.
      • NASA, China, and Russia plan permanent research bases in the region.
  • New study challenges the age of Saturn’s Rings

    Why in the News?

    A new study has challenged previous assumptions, suggesting that Saturn’s rings could be as old as the Solar System (~4.5 billion years old).

    New study challenges the age of Saturn’s Rings

    About Saturn and Its Rings

    • Saturn, the sixth planet from the Sun, is famous for its iconic ring system, made up of billions of ice and rock particles ranging in size from tiny grains to massive chunks.
    • It is primarily composed of water ice (95%), with some dust and rocky debris.
    • The rings are divided into seven main sections (A to G), with gaps like the Cassini Division.
    • Scientists have debated whether the rings formed with Saturn (~4.5 billion years ago) or if they are only 100-400 million years old.
    • Over time, tiny space rocks should darken the rings, yet they remain surprisingly bright.

    Key Findings of the Study:

    • Earlier estimates, based on Cassini data, suggested the rings were 100-400 million years old because they looked clean and bright.
    • The new study suggests that micrometeoroid collisions remove dust efficiently, preventing the rings from darkening over time.
    • High-speed micrometeoroid impacts (~108,000 km/h) cause dust to vaporize, rather than accumulate.
    • The vaporized dust either escapes Saturn’s gravity, falls into the planet’s atmosphere, or gets ejected into space, keeping the rings pristine.
    • 100 million years ago, the Solar System was stable, making ring formation unlikely.
    • 4 billion years ago, the Solar System was chaotic, increasing the chances of violent planetary collisions that could have formed Saturn’s rings.

    Various Missions to Saturn

    Saturn has been explored by multiple spacecraft, each providing valuable insights into its rings, atmosphere, and moons.

    1. Pioneer 11 (1979)

    • First spacecraft to fly past Saturn, capturing basic images.

    2. Voyager 1 & Voyager 2 (1980-1981)

    • Discovered new moons and ring structures.
    • Provided detailed images of Saturn’s rings.

    3. Cassini-Huygens (1997-2017)

    • A NASA-ESA-ASI mission that orbited Saturn for 13 years.
    • Key discoveries:
      • Confirmed liquid oceans on Enceladus.
      • Found methane lakes on Titan.
      • Observed Saturn’s rings losing material into the planet’s atmosphere.

     

    PYQ:

    [2009] Which one of the following planets has largest number of natural satellites or moons?

    (a) Jupiter
    (b) Mars
    (c) Saturn
    (d) Venus

     

  • [pib] Matsya-6000

    Why in the news?

    India’s 4th generation deep-ocean submersible Matsya-6000 has successfully completed wet testing at Chennai harbor, paving the way for shallow-water demonstrations at depths of up to 500 meters by 2025.

    [pib] Matsya-6000

    About Matsya-6000

    • Made of titanium alloy to withstand extreme oceanic pressure.
    • Built with a 2.1-meter diameter sphere to accommodate three crew members.
    • Moves at speed of 5.5 km/hr using multidirectional thrusters.
    • Uses GPS, underwater acoustic positioning, and joystick-controlled maneuverability.
    • Operates for 12 hours, with an emergency endurance of 96 hours.
    • Includes emergency buoyancy modules and highpressure-resistant escape hatches.
    • Features robotic arms for sample collection.
    • Uses highresolution imaging and oceanographic sensors for deep-sea research.
    • Future Trials:
      • Shallow-water tests up to 500m planned by late 2025.
      • Full deep-sea trials at 6,000m scheduled for 2026.

    What is Deep Ocean Mission (DOM)?

      • The DOM launched by the Ministry of Earth Sciences (MoES) in 2021, aims to enhance India’s deep-sea exploration capabilities while supporting the Blue Economy policy.
      • It focuses on resource utilization, climate monitoring, and marine biodiversity conservation.
    • Objectives of DOM:
    • Develop advanced technologies for ocean mining, biodiversity assessment, and deep-sea surveillance.
      • Enable climate change research through real-time ocean data collection.
      • Establish a Marine Station for Ocean Biology for research on marine ecosystems and pharmaceuticals.
      • Support the Samudrayaan Mission, which includes the development of Matsya-6000, India’s first deep-ocean human submersible.
    • Structural Mandate of DOM:
      • Deep-ocean survey and identification of polymetallic nodule and sulfide deposits.
      • Harnessing ocean energy through wave, tidal, and thermal sources.
  • Scientists discover ‘Einstein Ring’

    Why in the News?

    The European Space Agency’s (ESA) Euclid Space Telescope has captured a rare Einstein Ring around a galaxy nearly 590 million light-years away from Earth.

    Scientists discover ‘Einstein Ring’

    What is an Einstein Ring?

    • An Einstein Ring is a circular ring of light caused by gravitational lensing, a phenomenon predicted by Einstein’s General Theory of Relativity.
    • It occurs when a massive celestial object (like a galaxy) bends and magnifies light from a more distant background galaxy that lies directly behind it.
    • The recent discovery by ESA’s Euclid telescope identified an Einstein Ring around NGC 6505, located 590 million light-years away, acting as a lens for a distant galaxy 4.42 billion light-years away.
    • Features of an Einstein Ring:
      • Perfect circular shape (only if source, lens, and observer align precisely).
      • Example of strong gravitational lensing, distorting background light.
      • Extremely rare (found in less than 1% of galaxies).
      • Not visible to the naked eye, observed only with advanced space telescopes like Euclid or Hubble.

    Significance of the Discovery:

    • Reveals Dark Matter: Helps indirectly map dark matter, which makes up 85% of the universe.
    • Magnifies Hidden Galaxies: Makes faint, distant galaxies visible for study.
    • Measures Universe’s Expansion: Tracks how light stretches over time, refining cosmological models.
    • Confirms Einstein’s Theory: Proves light bends in curved space-time, supporting gravitational lensing theory.
    • Demonstrates Euclid’s Capabilities: Shows Euclid’s high-resolution potential, promising more discoveries.

    PYQ:

    [2018] Consider the following phenomena:

    1. Light is affected by gravity.
    2. The Universe is constantly expanding.
    3. Matter warps its surrounding space-time.

    Which of the above is/are the prediction/predictions of Albert Einstein’s General Theory of Relativity, often discussed in media?

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

     

  • PARAS-2 Spectrograph

    Why in the News?

    Scientists at PRL, Ahmedabad, discovered the exoplanet TOI-6038A b, a dense sub-Saturn-sized planet with a mass of 78.5 Earth masses and a radius of 6.41 Earth radii, using the PARAS-2 spectrograph at Mount Abu Observatory.

    About TOI-6038A b

    • TOI-6038A b is a dense sub-Saturn-sized planet with a mass of 78.5 Earth masses and a radius of 6.41 Earth radii, orbiting a bright, metal-rich F-type star every 5.83 days in a circular orbit.
    • This is the 2nd exoplanet discovery using the PARAS-2 spectrograph.
    • It is also the 5th exoplanet detection combining efforts of PARAS-1 and PARAS-2, showcasing India’s growing expertise in astronomical instrumentation.

    About PARAS-2 Spectrograph:

    • PARAS-2 (PRL Advanced Radial-velocity All-sky Search-2) is a state-of-the-art high-resolution spectrograph designed for exoplanet detection.
    • The development of PARAS-2 began in mid-2018 and was successfully installed at the telescope site in mid-2022.
    • It is the highest-resolution stabilized radial velocity (RV) spectrograph in Asia, operating at a precision level of 30 cm/s.
    • It is installed at PRL’s 2.5-meter telescope at the Mount Abu Observatory, benefiting from high-altitude, clear sky conditions.
    • Key Features of PARAS-2:
      • Operates in the 380-690 nm waveband, making it suitable for studying a wide range of celestial objects.
      • Resolution of ~107,000, the highest in Asia, enabling ultra-precise exoplanetary studies.
      • Ultra-stable temperature and pressure environment: Maintained at 24 ± 0.001 °C and 0.005 ± 0.0005 mbar, ensuring minimal instrumental drift.
      • Uses a Uranium Argon Hollow Cathode Lamp (UAr HCL) for calibration, achieving a velocity precision of better than 2 m/s.
      • Advanced optical fiber system for capturing stellar light and spectral calibration data simultaneously.
    • It uses the radial velocity method, which detects tiny wobbles in a star’s motion caused by the gravitational pull of an orbiting planet.
    • These wobbles cause shifts in the star’s light spectrum, allowing scientists to determine a planet’s presence, mass, and orbital period.
    • It can detect minute stellar movements, making it ideal for finding low-mass exoplanets like super-Earths.

    PYQ:

    [2015] The term ‘Goldilocks Zone’ is often seen in the news in the context of:

    (a) the limits of habitable zone above the surface of the Earth
    (b) regions inside the Earth where shale gas is available
    (c) search for the Earth-like planets in outer space
    (d) search for meteorites containing precious metals