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NASA's newest eye on the sky, the Nancy Grace Roman Space Telescope, has begun its journey to unravel the secrets of dark matter, dark energy and Earthlike planets — months ahead of schedule.

The 9-ton telescope rode to space today aboard a SpaceX Falcon Heavy rocket that was launched from NASA's Kennedy Space Center in Florida at 7:26 a.m. ET (11:26 UTC). The ascent went off without a hitch, setting up the telescope for a three-month cruise to a gravitational balance point known as Earth-sun L2, a million miles beyond our planet. The Falcon Heavy's two side boosters flew themselves back to landings on the Florida coast, near the launch site, while the center core booster splashed into the sea after stage separation.

NASA had originally scheduled liftoff for 2027, but the $4.3 billion mission came in ahead of schedule and under budget.

Here are five key facts about the Roman Space Telescope and its mission...

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It's amazing how much happens in the first few minutes of flight. An incredible opening sequence and Roman's journey is only just beginning!

The Nancy Grace Roman Space Telescope is set to launch [soon] aboard a SpaceX rocket from Kennedy Space Center in Florida. When it becomes operational early next year, it will transform our view of the universe.

With a mirror the same size as the one in the Hubble Space Telescope but a field of view more than 100 times larger, NASA's newest tool is designed to survey vast swaths of sky quickly. It will hunt for dark energy's fingerprints and detect perhaps 100,000 exoplanets.

In August 2018, just four months before she died on Dec. 25, I had the great fortune to fly from Sydney to Washington, D.C., to interview the woman this telescope is named after. She was 93 years old, and over the hours we spent talking, she shared her remarkable life story...

Two mirrors, each small enough to fit in the palm of your hand, are set to change how we understand the cosmos.

The launch window for NASA’s Nancy Grace Roman Space Telescope is about to open. The telescope’s primary instrument is due to inform practically every area of astrophysics, but also tucked inside the telescope is a specialized coronagraph, an experimental apparatus that will attempt to directly capture starlight reflected off a planet’s surface for the first time. It’s an ambitious project that NASA hopes will pave the way for a space telescope that can one day provide a glimpse of an Earthlike planet orbiting a sunlike star.

That’s a feat far beyond the power of current engineering—hence taking the basic technique for a spin on Roman. “We’ll test them in space for the first time, and we’ll understand what work still is left to go,” says Vanessa Bailey, an astrophysicist at NASA’s Jet Propulsion Laboratory and instrument scientist for the coronagraph.

At its core, a coronagraph is just a science-minded sunshade that can block out the light of a bright star and reveal a fainter object otherwise lost in the glare. Such instruments have flown in space before—both the Hubble and James Webb space telescopes carry coronagraphs. But Roman’s is light-years more sophisticated than its predecessors, thanks largely to technology called adaptive optics, which deforms a telescope’s mirror to cancel out these light distortions. It still faces a monumental challenge, though: NASA compares the task of Roman’s coronagraph to photographing a firefly perched next to a floodlight—from across the country.

The Nancy Grace Roman Space Telescope will settle essential questions in the areas of dark energy, exoplanets, and astrophysics.

Named after NASA’s first chief astronomer, the ‘mother of the Hubble Space Telescope,’ the Nancy Grace Roman Space Telescope will have a field of view at least 100 times larger than Hubble's, potentially measuring light from a billion galaxies in its lifetime. This observatory will also be able to block starlight to directly see exoplanets and planet-forming disks, complete a statistical census of planetary systems in our galaxy, and settle essential questions in the areas of dark energy, exoplanets, and infrared astrophysics.

🎯 NASA and SpaceX are targeting a 11:26 UTC liftoff on Sunday, Aug. 30.

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Watch the launch broadcast starting at 10:20 UTC

Learn more about Roman and how it will help us investigate some of the many mysteries of the universe in this video

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9 Things to Know About Roman

Planets form from disks of gas and dust around young stars, but the gas needed for growth does not last forever. New observations from NASA's James Webb Space Telescope (JWST) now offer a new view of how this gas escapes and how the process changes as young planetary systems develop.

The research, led by Naman Bajaj from the University of Arizona and co-authored by SETI Institute scientist Uma Gorti, looked at 72 young, sun–like stars and their protoplanetary disks. This is one of the largest planet-formation studies using JWST. The findings show that different types of winds are more important at different stages in a planetary system's early life.

A race against time
"What is exciting about this study is that we can now see, across a large sample of young systems, how the mechanisms that remove gas from planet-forming disks change with time. Disk dispersal sets a fundamental clock for planet formation: once the gas is gone, the opportunity to build gas-rich planets is essentially over," said Gorti.

Today, our solar system is about 4.5 billion years old and is mostly empty space. In its first few million years, though, the sun was surrounded by a thick protoplanetary disk with about 100 times more gas than dust. Most of that gas eventually vanished.

Figuring out how and when this happens is important because the gas in these disks is the main ingredient for giant planets like Jupiter and Saturn. If the gas goes away too soon, these planets might not have enough time to build up their thick atmospheres.