Free Topic-Wise General Studies MCQs
This module examines hypervelocity impact physics, graveyard orbit calculations, and passive mitigation tools like drag sails. Aspirants will analyze ISRO’s indigenous SSA capabilities including the Bengaluru Control Centre and regional optical telescopes.
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Explanation: Astroscale's ELSA-d mission tested the use of magnetic capture to dock with and remove satellites equipped with compatible docking plates.
Explanation: Deployable drag sails made of thin membranes increase the surface area of a satellite, significantly increasing atmospheric drag and shortening its orbital life.
Explanation: ADR involves missions specifically launched to capture and de-orbit large pieces of existing debris using nets, harpoons, or robotic arms.
Explanation: COLA (Collision Avoidance) maneuvers are the active changes in a satellite's path performed to avoid a predicted close approach (conjunction) with debris.
Explanation: Increased solar activity heats and expands the Earth's thermosphere, increasing drag on low-altitude debris and accelerating their re-entry into the atmosphere.
Explanation: A long conducting tether moving through Earth's magnetic field generates a Lorentz force that acts as drag, slowing the satellite without using propellant.
Explanation: Kinetic energy is proportional to the square of velocity (KE = 1/2 mv²). Doubling the speed increases the energy by a factor of four.
Explanation: Research into silica aerogel suggests it could be used to safely capture micro-debris without creating further fragmentation upon impact.
Explanation: The SSR, supported by the World Economic Forum, scores missions based on their debris mitigation and responsible orbital behavior.
Explanation: There are over 35,000 trackable objects, but estimated millions of smaller pieces (1cm and below) that are untrackable but still lethal.
Explanation: Objects in LEO must travel at roughly 7.8 km/s (approx. 28,000 km/h) to maintain their orbit, giving even tiny fragments massive kinetic energy.
Explanation: Chemical energy stored in batteries can lead to overcharging or thermal runaway years after a mission ends, making electrical discharge a key part of passivation.
Explanation: If the probability of a conjunction with the International Space Station is greater than 1 in 10,000, a Debris Avoidance Maneuver (DAM) is typically executed.
Explanation: The International Liquid Mirror Telescope (ILMT) uses a rotating pool of mercury to scan for space objects, though it is fixed to look only at the zenith.
Explanation: The Yarkovsky effect involves the force exerted by the emission of photons as heat; it can cause small debris to drift inward or outward over long periods.
Explanation: The Convention on International Liability for Damage Caused by Space Objects makes the 'launching state' strictly liable for damage on the surface of the Earth.
Explanation: While they may not shatter a satellite, millimeter-sized debris can puncture fuel lines, damage sensors, or degrade solar panels over time.
Explanation: The European Space Agency (ESA) commissioned the ClearSpace-1 mission to capture and de-orbit a Vespa payload adapter.
Explanation: Ground-based radar and optical sensors can reliably track objects about 10 cm and larger in LEO, and roughly 1 meter in higher orbits.
Explanation: The Vega Secondary Payload Adapter (Vespa) is an upper stage component from a 2013 launch, chosen as a representative target for removal technology.
Explanation: Project West Ford placed 480 million copper needles into orbit to create a permanent radio-reflecting belt, many of which clumped together and still orbit Earth.
Explanation: The 800 to 1000 km altitude range is the most congested due to its historical use for sun-synchronous meteorological and surveillance satellites.
Explanation: Hypervelocity impacts generate localized plasma that can create conductive paths, leading to an Electrostatic Discharge (ESD) that can short-circuit satellite electronics.
Explanation: As more satellites are launched and more debris is created, the MTBC is decreasing, meaning collisions are becoming more frequent events.
Explanation: The Inter-Agency Space Debris Coordination Committee (IADC) is an international governmental forum for the worldwide coordination of activities related to man-made and natural debris.
Explanation: Satellites at the end of their life in GEO are moved roughly 300 km higher into a 'super-synchronous' graveyard orbit to clear the valuable GEO belt.
Explanation: While orbits vary, relative velocities above 5 km/s typically ensure that the energy of impact exceeds the structural binding energy, causing complete fragmentation.
Explanation: Internal energy sources, like leftover fuel or pressurized batteries, are the leading cause of satellite breakups in orbit.
Explanation: The intentional destruction of Fengyun-1C created more than 3,000 pieces of trackable debris and tens of thousands of smaller fragments.
Explanation: The 'Big Sky Theory' argued that space is so vast that the chances of two objects ever hitting each other were negligible, a belief debunked by increasing congestion.
Explanation: Molniya orbits are highly elliptical (eccentric); debris in these orbits spend most of their time at high altitudes and dive quickly through LEO, making tracking inconsistent.
Explanation: ClearSpace-1 uses four robotic arms (pincers) to grab a defunct payload adapter, ensuring a secure grip on a spinning, uncooperative target.
Explanation: A state maintains legal ownership and responsibility for a space object indefinitely, regardless of whether it is active or defunct debris, as long as it is registered.
Explanation: The KITE (Kounotori Integrated Tether Experiment) on the HTV-6 cargo ship attempted to use a tether to generate electricity and drag via Earth's magnetic field.
Explanation: Passive mitigation involves 'passivating' the spacecraft by venting leftover fuel or discharging batteries to prevent future accidental explosions.
Explanation: The area-to-mass ratio accounts for the effect of solar radiation pressure; high area-to-mass objects require a higher graveyard orbit to ensure they don't drift back.
Explanation: Proposed by Donald Kessler in 1978, this scenario suggests that the accumulation of space junk could eventually make certain orbital planes unusable for generations.
Explanation: A Whipple shield uses a thin outer layer to break up a small piece of debris into a cloud of even smaller particles before they hit the main hull.
Explanation: Even at 400 km, there is a trace atmosphere that creates drag, causing objects to lose speed and eventually fall back to Earth.
Explanation: The re-entry of Cosmos 954 scattered radioactive debris over northern Canada, highlighting the risks of complex debris components.
Explanation: Many CubeSats lack propulsion systems, meaning they cannot perform collision avoidance or actively de-orbit, relying solely on natural decay.
Explanation: The ballistic coefficient (mass divided by the product of drag coefficient and area) determines how much atmospheric drag affects an object’s orbital lifespan.
Explanation: In 1996, the Cerise satellite’s gravity-gradient stabilization boom was struck by a fragment from an Ariane 1 rocket upper stage that had exploded ten years earlier.
Explanation: The Orbital Debris Engineering Model (ORDEM) is NASA’s primary software tool for estimating the debris population and risk in Earth's orbit.
Explanation: The RemoveDEBRIS satellite successfully deployed a net to capture a simulated target and fired a harpoon at a structural panel.
Explanation: Nextel is a ceramic fabric used in advanced Whipple shields; it is highly effective at shocking and vaporizing debris particles upon impact.
Explanation: Soviet Radar Ocean Reconnaissance Satellites (RORSATs) ejected their reactor cores at the end of life, releasing NaK (Sodium-Potassium) coolant droplets that remain in orbit today.
Explanation: The Lockheed Martin-built 'Space Fence' (AN/FSY-3) provides high-frequency S-band radar surveillance to track much smaller objects than traditional L-band systems.
Explanation: For collisions in space, the convention requires proof of fault. Conversely, for damage on the Earth's surface, the launching state is 'absolutely' liable.
Explanation: The 1967 Outer Space Treaty provides the basic framework for space activities, emphasizing that space should be used for peaceful purposes.
Explanation: Ground-based lasers suffer from atmospheric distortion, making it difficult to maintain the beam focus required to vaporize debris surfaces.
Explanation: The collision between the active Iridium 33 and the defunct Cosmos 2251 created over 2,000 pieces of trackable debris in LEO.
Explanation: Passivation is the process of removing any stored energy (chemical, electrical, or kinetic) to prevent an explosion after the mission ends.
Explanation: Controlled re-entry uses the remaining fuel to push the satellite into the atmosphere over an unpopulated area (like the South Pacific) to burn up.
Explanation: The Inter-Agency Space Debris Coordination Committee (IADC) '25-year rule' is the international standard for post-mission disposal in LEO.
Explanation: The Orbital Footprint measures how much space a satellite 'occupies' in terms of its size, altitude, and probability of colliding with other objects over its lifetime.
Explanation: UNOOSA maintains the Register of Objects Launched into Outer Space to identify which state is responsible for each satellite.
Explanation: The 'Bumper' is the thin outer plate placed at a distance from the main wall; its job is to break up the projectile before it reaches the main structure.
Explanation: Radar power drops off according to the inverse fourth power of the distance ($1/r^4$), making it extremely power-intensive to detect small objects at 36,000 km.
Explanation: The GRAVES radar (Grand Réseau Adapté à la Veille Spatiale) is a French system used to track and catalog objects in orbit over Europe.