NASA’s revolutionary Dawn spacecraft enters the final stretch

The legacy of Dawn has taught astronomers remarkable things about the evolution of the inner Solar System

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Dawn arrived into orbit at Ceres on March 6, 2015, and continues to collect data about the mysterious and fascinating world. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

When Dawn launched from Cape Canaveral Air Force Station in Florida in September 2007, strapped on a Delta II-Heavy rocket, scientists and engineers had an idea of what Ceres and Vesta looked like. Thanks to ground- and space-based telescopes, including NASA’s Hubble Space Telescope, the bodies in the asteroid belt between Mars and Jupiter were visible – but even the best pictures were fuzzy.

From 2011 to 2012, Dawn swept over Vesta, capturing images that exceeded everyone’s imaginings – craters, canyons and even mountains. Then on Ceres in 2015, Dawn showed us a cryovolcano and mysterious bright spots, which scientists later found might be salt deposits produced by the exposure of briny liquid from Ceres’ interior. Through Dawn’s eyes, these bright spots were especially stunning, glowing like diamonds scattered across the dwarf planet’s surface.

“Dawn’s legacy is that it explored two of the last uncharted worlds in the inner Solar System,” says Marc Rayman of NASA’s Jet Propulsion Laboratory in Pasadena, California, United States, who serves as Dawn’s mission director and chief engineer. “Dawn has shown us alien worlds that for two centuries were just pinpoints of light amidst the stars. And it has produced these richly detailed, intimate portraits and revealed exotic, mysterious landscapes unlike anything we’ve ever seen.”

Dawn is the only spacecraft to orbit a body in the asteroid belt. And it is the only spacecraft to orbit two extraterrestrial destinations. These feats were possible thanks to ion propulsion, a tremendously efficient propulsion system familiar to science-fiction fans and space enthusiasts. Dawn pushed the limits of the system’s capabilities and stamina, showing how useful it is for other missions that aim to visit multiple destinations.

Pushed by ion propulsion, Dawn reached Vesta in 2011 and investigated it from surface to core during 14 months in orbit. In 2012, engineers maneuvered Dawn out of orbit and steered it through the asteroid belt for more than two years before inserting it into orbit around the dwarf planet Ceres, where it has been collecting data since 2015.

All the while, scientists gained new insight into the early stages of our Solar System, fulfilling Dawn’s objective. The mission was named for its purpose: to learn more about the dawn of the Solar System. It targeted Ceres and Vesta because they function as time capsules, intact survivors of the earliest part of our history. And the duo delivered, giving scientists insight into the original building blocks of the Solar System.

“Vesta and Ceres have each told their story of how and where they formed, and how they evolved – a fiery magmatic history that led to rocky Vesta and a cooler, water-rich history that resulted in the ancient ocean world Ceres,” says Carol Raymond of JPL, principal investigator of the Dawn mission. “These treasure troves of information will continue to help us understand other bodies in the Solar System far into the future.”

There was so much that scientists didn’t know about Ceres before Dawn arrived. Raymond wondered whether they might find Ceres covered with a smooth, young surface – an enormous cue ball with a frozen crust. Instead, they found the dwarf planet wearing the chemistry of its old ocean. “What we found was completely mind-blowing. Ceres’ history is just splayed all over its surface,” she says.

Some of the dazzling bright spots turned out to be brilliant salty deposits, composed mainly of sodium carbonate that made its way to the surface in a slushy brine from within or below the crust.

The findings reinforce the idea that dwarf planets, not just icy moons like Enceladus and Europa, could have hosted oceans during their history – and potentially still do. Analysis of Dawn data suggests there may still be liquid under Ceres’ surface and that some regions were geologically active relatively recently, feeding from a deep reservoir.

One of Dawn’s biggest reveals on Ceres lay in the region of Ernutet Crater. Organic molecules were found in abundance. Organics are among the building blocks of life, though Dawn’s data can’t determine if Ceres’ organics were formed by biological processes.

“There is growing evidence that the organics in Ernutet came from Ceres’ interior, in which case they could have existed for some time in the early interior ocean,” says Julie Castillo-Rogez, Dawn’s project scientist and deputy principal investigator at JPL.

At Vesta, Dawn’s investigation into the early Solar System found a 4.5-billion-year-old witness it could interrogate. Dawn mapped the craters of the planet-like world and revealed that its northern hemisphere had experienced more large impacts than expected, suggesting there were more large objects in the asteroid belt early on than scientists thought.

Vesta held other surprises as well. While it’s technically classified as an asteroid, that label belies the rich and varied terrain Dawn revealed, and the planet-like processes that Vesta experienced. Hubble had relayed images of a mountain at the centre of an enormous basin now called Rheasilvia. Dawn’s mapping showed it to be twice the height of Mount Everest, and it revealed canyons that rival the Grand Canyon in size. Dawn also confirmed Vesta as the source of a very common family of meteorites.

Now, near the end of Dawn’s second extended mission at Ceres, the spacecraft has continued to gather high-resolution images, gamma ray and neutron spectra, infrared spectra, and gravity data. Almost once a day, it will swoop over Ceres about 35 kilometres (22 miles) from its surface – only about three times the altitude of a passenger jet – gathering valuable data until it expends the last of the hydrazine that feeds thrusters controlling its orientation. Dawn’s reaction wheels failed earlier in the mission, leaving it heavily dependent on this key fuel. When Dawn runs out in the next month or two, the spacecraft will lose its ability to communicate with Earth, but it must not crash into Ceres.

Because Ceres has conditions of interest to scientists who study chemistry that leads to the development of life, NASA follows strict planetary protection protocols for the disposal of the Dawn spacecraft. Unlike Cassini, which deliberately plunged into Saturn’s atmosphere to protect the system from contamination – Dawn will remain in orbit around Ceres, which has no atmosphere.

Engineers designed Dawn’s final orbit to ensure it will not crash for at least 20 years – and likely decades longer.

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