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Relevance: GS-III (Science & Technology: Space Exploration) Source: Space & Science Updates, August 2026

1 · The News

When we look up at the night sky, we only see a tiny fraction of what is actually there. Most of space is filled with invisible forces known as “dark matter” and “dark energy.” To solve this massive cosmic puzzle, NASA is launching the Nancy Grace Roman Space Telescope, a $4-billion next-generation observatory.
Named after NASA’s first female chief astronomer, this powerful satellite is the direct successor to the famous Hubble and James Webb telescopes. Set to launch on a SpaceX Falcon Heavy rocket, this mission aims to map out the expanding universe, trace invisible gravity, and hunt for thousands of new planets floating in deep space.

2 · The Cosmic Mission

Step 1: The Expansion Mystery
The telescope will survey over two billion galaxies to understand how “dark energy” is constantly forcing our universe to expand faster and faster.
Step 2: Mapping the Invisible
By watching how gravity slightly bends distant starlight, Roman will build a 3D map of “dark matter”—the invisible glue holding galaxies together.
Step 3: The Great Planet Hunt
The mission is expected to discover approximately 100,000 new exoplanets using microlensing and transit detection.
Step 4: The Deep Space Parking Spot
After launching, it will travel 1.6 million km away from Earth to a stable gravitational spot called Lagrange Point 2 (L2) to safely begin its work.

3 · Key Space Technological Terms

Wide-Field Instrument
The Big Picture Camera
This 300.8-megapixel camera has a 2.4-meter mirror matching Hubble’s size, but provides a field of view that is at least 100 times larger.
Coronagraph (CGI)
Cosmic Sunglasses
A special masking tool inside the telescope that completely blocks the blinding light of a host star, allowing scientists to directly photograph nearby hidden planets.
Gravitational Microlensing
Einstein’s Trick
A technique where a massive object acts like a magnifying glass in space. It bends space-time, magnifying the light behind it to reveal tiny, distant planets.
Lagrange Point 2 (L2)
The Stable Orbit
A perfect balancing point where the gravity of the Sun and Earth match. Telescopes parked here stay in a fixed position, completely shielded from solar radiation.

Prelims Quick Facts: Mission Details
Bipartisan Support Despite attempts by past US leadership to cut its funding entirely, the US Congress repeatedly saved the mission, proving strong support for space research.
The L2 Neighbourhood The Roman Space Telescope will share the exact same L2 operational orbit with the famous James Webb Space Telescope.
Naming Legacy The observatory is proudly named after Dr. Nancy Grace Roman, NASA’s first chief astronomer, often affectionately called the “Mother of Hubble.”
Synergy for ISRO Since NASA provides open-source data from this telescope, ISRO can strategically use this advanced deep-space information to boost its own Indian space missions.

MCQ Practice Question
Q. With reference to the Nancy Grace Roman Space Telescope, consider the following statements:

  1. It will operate from Lagrange Point 2 (L2), which is also the operational orbit for the James Webb Space Telescope.
  2. Its Wide-Field Instrument features a primary mirror that is physically much larger than the Hubble Space Telescope’s mirror.
  3. The mission aims to discover new exoplanets utilizing gravitational microlensing and transit detection methods.

Which of the statements given above is/are correct?
(a) 1 and 2 only    (b) 1 and 3 only    (c) 2 and 3 only    (d) 1, 2 and 3

Answer: (b) 1 and 3 only

  • Statement 1 — Correct: The Roman Space Telescope will travel 1.6 million km to the gravitationally stable Lagrange Point 2 (L2).
  • Statement 2 — Incorrect (the trap): The primary mirror is 2.4-meters, which matches the exact size of Hubble’s mirror, though its technological design provides a field of view at least 100 times larger.
  • Statement 3 — Correct: It aims to find approximately 100,000 new exoplanets using microlensing and transit detection techniques.

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