At 7:26 a.m. Eastern time on Sunday, NASA launched its latest space observatory, the Nancy Grace Roman Space Telescope, from Kennedy Space Center in Florida. Named after NASA’s first chief astronomer, Roman is designed to provide unprecedented wide-field infrared imaging to map the cosmos in exquisite detail. The $4.3 billion telescope was carried into orbit aboard a SpaceX Falcon Heavy rocket and is now en route to its operational position near the second Lagrange point (L2), about one million miles from Earth. This stable location balances gravitational forces from the Earth and Sun, allowing the telescope to conserve fuel during its mission.

Roman aims to survey a vast portion of the sky with an infrared resolution comparable to the Hubble Space Telescope but with a field of view more than 100 times wider, making it up to 1,000 times faster at capturing images. Equipped with a 300-megapixel infrared camera and a coronagraph instrument, Roman will chart billions of galaxies, study hundreds of black holes, and observe dusty disks around young stars where planets form. Scientists expect it to discover more than 100,000 exoplanets, significantly expanding the known population within the Milky Way.

One of the telescope’s primary scientific objectives is to investigate the nature of dark matter and dark energy—the invisible substances thought to compose most of the universe’s mass-energy content. By analyzing gravitational lensing effects, where the gravity of matter bends light from distant galaxies, Roman will map the distribution of dark matter across cosmic time. Concurrently, it will provide new insights into dark energy by measuring the universe's accelerated expansion rate through three independent methods: observations of specific types of exploding stars called supernovae, detailed galactic surveys, and tracking the growth and separation of cosmic structures.

The coronagraph aboard Roman will directly image known exoplanets by blocking out the stars’ light, a capability that improves upon previous instruments. This component serves as a testbed for future NASA missions, such as the proposed Habitable Worlds Observatory, which aims to image Earth-like planets beyond the solar system.

Roman joins a cohort of powerful observatories shaping modern astrophysics. Alongside the European Space Agency’s Euclid telescope—which launched in 2023 to survey about one-third of the sky—and the Vera C. Rubin Observatory in Chile, Roman will deliver higher-resolution data over a smaller portion of the sky. Experts anticipate that combining data from these instruments will lead to transformative discoveries about the structure, evolution, and fundamental composition of the universe.

The mission is part of a long legacy of space-based astronomy that began with the launch of the Hubble Space Telescope in 1990, which provided transformative insights into the expanding universe, the existence of black holes, and distant galaxies. Successive observatories, including Compton, Chandra, Spitzer, Kepler, and the James Webb Space Telescope, have expanded humanity’s cosmic horizon. Despite these advances, many mysteries remain, such as the exact properties of dark energy and the elusive nature of dark matter. Roman is expected to address these questions while also offering opportunities for unexpected discoveries.

After approximately 100 days of travel, Roman will begin its planned five-year science mission, transmitting around one terabyte of data daily to Earth. Scientists describe the launch as opening a new chapter in cosmic exploration, one that promises to deepen understanding of the universe’s origin, composition, and potential for hosting life beyond Earth.