NASA's next flagship observatory, the Nancy Grace Roman Space Telescope, is set to launch on 30 August 2026 on a SpaceX Falcon Heavy from Kennedy Space Center.
It will operate around the second Sun-Earth Lagrange point (L2) on a five-year primary mission, studying dark energy, dark matter and exoplanets.
Its 2.4-metre primary mirror matches Hubble's in size, but its field of view is at least 100 times wider.
The two instruments are the Wide Field Instrument, a 300-megapixel infrared camera, and the Coronagraph Instrument, a technology demonstration for direct imaging of exoplanets.
The mission was earlier called WFIRST and was renamed in May 2020 after Nancy Grace Roman, NASA's first chief astronomer and the 'Mother of Hubble'.
Lagrange points are five positions in a two-body system where the gravitational pull of the two large bodies and the centripetal force on a small object balance, so a spacecraft placed there keeps station with relatively little fuel. L2 lies about 1.5 million km from Earth, directly away from the Sun. A telescope parked there has the Sun, Earth and Moon all in roughly the same direction, so a single sunshield can block all three at once and keep the instruments cold and stable - essential for infrared observation. India's Aditya-L1 uses the corresponding L1 point on the Sun-facing side, and the James Webb Space Telescope also operates at L2.
Simple Analogy: L2 is like a parking spot that moves with the car it is parked beside - the spacecraft orbits the Sun in step with Earth instead of drifting away from it.
Also operates around Sun-Earth L2, but is a deep-field, narrow-view observatory; Roman is the wide-survey complement to it.
Same 2.4-metre mirror diameter as Roman; Nancy Grace Roman's leadership in getting Hubble built is why the new telescope carries her name.
India's solar observatory is stationed at Sun-Earth L1, the mirror-image point on the Sun-facing side - a standard prelims pairing with L2 missions.
The detection method Roman will use for its exoplanet census, distinct from the transit method used by Kepler and TESS and the radial-velocity method used from the ground.
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General Awareness > Science and Technology > Space missions
General Awareness > Current affairs in science and technology
The term 'Goldilocks Zone' is often seen in the news in the context of
Answer: search for the Earth-like planets in outer space
One of five positions in a two-body system where gravitational and centripetal forces balance, allowing a spacecraft to hold station with minimal fuel.
A detection method in which the gravity of a foreground star and its planets briefly magnifies the light of a background star, revealing planets that never transit their host.
An instrument that blocks the light of a bright central source so that much fainter nearby objects, such as planets, can be imaged.
A stellar explosion of predictable intrinsic brightness, used as a 'standard candle' to measure cosmic distances and the expansion history of the universe.
The unexplained component driving the accelerating expansion of the universe.