Ceres is a dwarf planet and the largest known object in the
asteroid belt between Mars and Jupiter.
And now we know it may be an ocean world with intriguing geologic activity taking place on and just below its surface, according to new research.
While this global ocean beneath the planet's surface likely froze over time, remnants of it may still be present beneath a large impact crater on Ceres.
False color was used to highlight the recently exposed brine, or salty liquids, that were pushed up from a deep reservoir under Ceres' crust in the Occator Crater. (CNN)
The presence of salts may have preserved the liquid as a brine, despite cold temperatures.
The suite of seven studies were published in the journals Nature Astronomy, Nature Geoscience and Nature Communications.
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Between 2011 and 2018, NASA's Dawn mission embarked on a 6.9 billion-kilometre journey to two of the largest objects in our solar system's main asteroid belt.
Bright pits and mounds in Occator Crater were formed by salty liquid released as Occator's water-rich floor froze after the crater-forming impact about 20 million years ago. (CNN)
Ceres is about 953 km across, 14 times smaller than Pluto.
NASA's Dawn mission visited Vesta and Ceres, becoming the first spacecraft to orbit two deep-space destinations.
False colour was used to highlight the recently exposed brine, or salty liquids, that were pushed up from a deep reservoir under Ceres' crust in the Occator Crater.
This new research is based on observations made during Dawn's orbit of Ceres between 2015 and 2018, including close passes it made of the
dwarf planet just 35 km above the surface toward the end of the mission.
During that time, Dawn was focused on the 93-km-wide Occator Crater, a 22-million-year-old feature that appeared to showcase bright spots.
These eye-catching characteristics were discovered to be sodium carbonate, or a compound including oxygen, carbon and sodium.
But it was unclear how those bright spots came to be in the crater.
Data from the end of Dawn's mission revealed an extensive and slushy reservoir of brine, or salty liquid, beneath the crater.
It's 40 km deep and extends out for hundreds of miles.
An artist's impression of Ceres. (Supplied)
When the impact that created the crater struck Ceres, it may have allowed the reservoir to deposit bright salts visible in the crater by fracturing the planet's crust.
As the fractures reached the salty reservoirs, the brine was able to reach the surface of the crater floor.
When the water evaporated, a bright, salty crust remained behind.
Brines still forming today
Brines may still be rising to the surface today which suggests the activity on Ceres is not due to melting that may have occurred when the planet was impacted.
In fact, Dawn's data also indicated the presence of hydrated chloride salts at the centre of the largest bright area at the crater's centre, called Cerealia Facula.
This hydrohalite compound is common in marine ice on Earth, but it's the first time hydrohalite has been found outside of our planet.
Ceres, Eris, Haumea, Pluto (L-R) (Getty, Wikipedia)
Bright pits and mounds in Occator Crater were formed by salty liquid released as Occator's water-rich floor froze after the crater-forming impact about 20 million years ago.
The salts appear to dehydrate quickly on the surface, at least, astronomically speaking.
This dehydration occurs over hundreds of years.
But the measurements taken by Dawn showed water was still present.
This suggests brine may still be rising to the surface of the crater and salty liquid could still exist inside of Ceres.
"For the large deposit at Cerealia Facula, the bulk of the salts were supplied from a slushy area just beneath the surface that was melted by the heat of the impact that formed the crater about 20 million years ago," Dawn's principal investigator at NASA's Jet Propulsion
Laboratory in California, Carol Raymond said in a statement.
"The impact heat subsided after a few million years; however, the impact also created large fractures that could reach the deep, long-lived reservoir, allowing brine to continue percolating to the surface."
3D visualisation of a mountain on the dwarf planet Ceres based on data from Nasa's Dawn satellite. (NASA)
There are also mounds and hills visible in the crater, likely created when flows of water froze in place, suggesting geologic activity on Ceres.
These conical hills are similar to pingos on Earth, or small mountains made of ice found in the polar regions.
Although features like this have also been found on Mars, it's the first time they've been spotted on a dwarf planet.
An unusual dwarf planet
The pingo-like structures and the water that pushes up through fractures in the crater revealed that Ceres experienced cryovolcanic activity, or ice volcanoes, beginning around 9 million years ago and the process is likely ongoing.
This kind of cryovolcanic activity has been witnessed on icy moons in the outer solar system, with plumes of material ejecting into space.
But it was never expected to occur on dwarf planets or asteroids in the asteroid belt, which are thought to be waterless and inactive.
Ceres changes that theory because it has proven to be water-rich and active.
An artist's concept shows the Dawn spacecraft approaching the dwarf planet Ceres. (NASA/JPL-Caltech) (NASA/JPL-Caltech)
A survivor from the earliest days of the solar system as it formed 4.5 billion years ago, Ceres was more of an "embryonic planet"; essentially, it started to form, but never finished.
Jupiter, the largest planet in our solar system, and the force of its gravity likely stunted Ceres' growth.
So around 4 billion years ago, Ceres found its home in the asteroid belt along with all of the other leftovers from the formation of the solar system.
The idea that liquid water can remain preserved on dwarf planets and asteroids is an intriguing one for scientists.
Unlike other icy ocean worlds in our solar system, such as Saturn's moon Enceladus and Jupiter's moon Europa, asteroids and dwarf planets don't experience internal heating.
Enceladus and Europa benefit from internal heating that occurs when they interact gravitationally with the massive planets they orbit.
The Dawn mission ended in 2018 when the spacecraft ran out of fuel and could no longer communicate with NASA.
It was placed into long-term orbit around Ceres to prevent impact, protecting its organic materials and subsurface liquid.
The unidentified bright spots snapped from the Dawn probe on approach to Ceres. (Associated Press)
The findings made possible by the Dawn mission have scientists eager to explore the dwarf planet and its potential for life in greater detail in the future.
While there is not currently another mission planned for exploring Ceres, two upcoming missions will explore Jupiter and its icy moons Ganymede, Callisto and Europa.
"Dawn accomplished far more than we hoped when it embarked on its extraordinary extra-terrestrial expedition," Dawn's mission director at JPL, Marc Rayman said in a statement.
"These exciting new discoveries from the end of its long and productive mission are a wonderful tribute to this remarkable interplanetary explorer."
https://www.9news.com.au/world/nasa...f-planet/87abc746-ae10-4baa-833a-2bc409d19cdd
