NASA
NASA is set to launch its Nancy Grace Roman Space Telescope on August 30 aboard a SpaceX Falcon Heavy rocket from Kennedy Space Center in Florida.
Why it matters for sellers
New product = GTM investment and tooling needs
Signal details
- Counterparty
- SpaceX
- Event date
- August 30, 2026
- Reported
- August 8, 2026
- Source
- forbes.com
From the coverage · forbes.com
By Jamie Carter , Senior Contributor. NASA's Nancy Grace Roman Space Telescope is set to launch on August 30 aboard a SpaceX Falcon Heavy, nine months ahead of schedule. This flagship observatory, named after NASA's first chief astronomer, aims to revolutionize astronomy by creating vast panoramic maps of the universe, unlike Hubble's detailed close-ups. 4-meter mirror and a Wide Field Instrument covering 100 times Hubble's view, allowing it to map billions of galaxies and survey the Milky Way in just one month. It's expected to discover 100,000 new cold exoplanets and rogue planets, significantly expanding our understanding of planetary systems.
Additionally, Roman will tackle mysteries of dark energy and dark matter by mapping galaxy positions and gravitational lensing. Operating from the Sun-Earth L2 point alongside the James Webb Space Telescope, Roman will identify intriguing targets for Webb's closer examination, providing complementary views of the cosmos. NASA’s next flagship space observatory has a launch date. The Nancy Grace Roman Space Telescope is scheduled to launch from Kennedy Space Center in Florida on Sunday, Aug. 30, aboard a SpaceX Falcon Heavy rocket. The launch comes roughly nine months ahead of NASA’s previous schedule, an unusually early milestone for a flagship astrophysics mission after years of development.
Named after the late Dr. Nancy Grace Roman — NASA’s first chief astronomer who championed space telescopes — Roman is expected to transform astronomy in much the same way the Hubble Space Telescope did more than three decades ago. However, instead of producing exquisitely detailed close-up images of individual objects, it will create enormous panoramic maps of the universe. Rather than studying one galaxy at a time, Roman will map billions of them, giving astronomers an entirely new perspective on how the universe is structured and how it has evolved over cosmic history.
9-foot) primary mirror as Hubble, but its Wide Field Instrument will capture images covering more than 100 times Hubble’s field of view, allowing it to survey vast areas of sky at speed. During its five-year prime mission, Roman is expected to collect around 20 petabytes of science data — and image more sky than Hubble has observed during decades of operations, according to NASA. One month of Roman observations could survey our own Milky Way, resulting in the detection of up to half the stars in our own galaxy,” said Julie McEnery, Roman telescope senior project scientist, NASA Goddard, in a NASA press conference on July 29.
” She added that it would take over half a million 4K TVs to fully display the single Roman image from its largest survey — enough to cover El Capitan in Yosemite National Park. Perhaps most exciting is Roman’s status as an exoplanet hunter. Unlike NASA’s Kepler and TESS missions that could only find planets that orbit close to their host stars, Roman is expected to discover 100,000 colder exoplanets orbiting far away — planets like most of those in our own solar system. That’s up to 40 times more than we know of today. It’s also likely going to find large populations of rogue planets drifting through the Milky Way without orbiting any star at all.
“Roman’s vast reach will allow us to find the weird, the rare, and the unusual,” said McEnery, citing things like exoplanets with disks, isolated black holes and neutron stars in our galaxy, and runaway supermassive black holes. ” Roman will also carry a coronagraph, a disk to block the glare from a star, to help it photograph giant exoplanets. It’s hoped that it will prove out the tech for a future space telescope to photograph Earth-sized planets around nearby sun-like stars. One of Roman’s goals is tackling one of modern astronomy’s biggest mysteries — why the universe’s expansion is accelerating.
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