New images from asteroid probe yield clues on planet formation (Update)

New images from asteroid probe offer clues on planet formation
The image shows the first image acquired by the DLR-developed MASCAM camera system during Hayabusa2's descent, shortly after separation from the landing module at a height of 41 meters with a viewing direction towards the south pole. Particularly striking is a huge block near the South Pole, which stands out clearly above the horizon line and which is named 'Otohime Saxum'. It is up to 100 meters tall. Credit: Jaumann et al., Science (2019)

Photographs snapped by a shoebox-sized probe that explored the near-Earth asteroid Ryugu offer new clues about its composition, insights that are expected to help scientists understand the formation of our solar system.

The German-French Mobile Asteroid Surface Scout (MASCOT) was dropped off by Japan's Hayabusa2 spacecraft on October 3, 2018, free-falling from a height of 41 meters (135 feet) for six minutes before it hit the surface.

It then bounced a couple of times—reaching a height of 17 meters on the first bounce—before coming to rest.

Ryugu is just 900 meters wide and so its gravity is 66,500 times weaker than Earth's. Had MASCOT been equipped with wheels, its forward motion would have launched it back into space.

Instead, it hopped around the surface using the tiny amount of momentum generated by a metal swing arm attached to its boxy body, which weighed 10 kilograms (22 pounds).

In addition to taking temperature readings and other measurements, MASCOT sent back a series of pictures showing the asteroid is covered with two types of rocks and boulders: dark and rough ones with crumbly surfaces resembling cauliflowers, and bright and smooth ones.

"The interesting thing there is, it really shows that Ryugu is the product of some kind of violent process," Ralf Jaumann of the German Aerospace Center told AFP. He is the lead author of a paper describing the findings, published Thursday in the journal Science.

On 3 December 2014, the Japanese space probe Hayabusa2 embarked on a sample return mission to asteroid (162173) Ryugu. On board is the Mobile Asteroid Surface Scout (MASCOT), a lander built by the German Aerospace Center (Deutsches Zentrum für Luft-und Raumfahrt; DLR) in collaboration with the French space agency CNES. The aim of the Hayabusa2 mission is to learn more about the origin and evolution of the Solar System. As asteroids account for some of the most primordial celestial bodies, researching them gives us a glimpse into our cosmic past. Furthermore, Ryugu is a near-Earth asteroid, which means it could pose a threat to Earth and must be investigated in order to reduce this threat. Credit: © DLR (CC-BY 3.0)

Ryugu may be the "child" of two parent bodies that collided, broke up and were then pulled back together by gravity, the researchers say.

Alternatively, it could have been struck by another body that created different interior temperature and pressure conditions, creating the two types of material.

Many of the rocks contain small blue and red "inclusions"—material trapped in the rock during its formation—much like a type of rare, primordial meteorites found on Earth called carbonaceous chondrites.

"This material is primitive material—it's the very first material of the solar nebula," or the cloud of interstellar dust and gas that formed the planets of our system, said Jaumann.

New images from asteroid probe offer clues on planet formation
The second image of the DLR-developed MASCAM camera is directed obliquely downward on the asteroid Ryugu and covers areas east of the descent route. Compared with the first image, it is clear that MASCOT moved turbulently towards Ryugu, as expected, thus performing turns and rollovers. The images show a huge boulder, which occupies the eastern (right) edge of the image and is several tens of meters in length. On the bottom left is MASCOT's shadow, which the Sun behind the landing probe is projecting onto the asteroid surface: MASCOT is 30 centimeters long. Ryugu is a body with no atmosphere, so the outlines of MASCOT are sharp in the shadows projected onto the asteroid surface. Credit: Jaumann et al., Science (2019)

Hayabusa2, which set off from Earth in 2014 and itself touched down twice on the asteroid's surface, most recently in July, will arrive home next year carrying samples for analysis in the lab.

MASCOT's observations provide, for the first time, information on the material's original geologic context, including how it is exposed to temperature changes and how it is "weathered" in space.

"We don't know how planets formed in the beginning," said Jaumann.

"And in order to understand this, (we must) go to the small bodies, these primitive bodies, primordial in their history in their evolution, in order to understand the first 10 to 100 million years of planetary formation."

New images from asteroid probe offer clues on planet formation
Before the first contact with a large rock on Ryugu, DLR's MASCAM camera photographed the area of the descent route with a backward-looking view. Credit: Jaumann et al., Science (2019)

A dust mystery, and a future threat?

MASCOT also presented scientists with a new mystery: its lack of fine particles, or interplanetary dust, which would normally accumulate through millions of years of space weathering.

The paper offered theories but no definitive conclusions.

The dust might have fallen into tiny holes in Ryugu's surface when the asteroid was struck by other bodies.

  • New images from asteroid probe offer clues on planet formation
    The fifth image acquired by the DLR-developed MASCAM camera system was taken shortly after the first contact with the ground, just a few meters above the surface of Ryugu. Just as in the images from higher altitudes, no fine material, known as regolith, can be seen, even in the immediate vicinity of the surface. Regolith is formed on atmosphere-less bodies due to their permanent exposure to high-energy particles from space or micrometeorites due to the weathering of coarser material into dust. Instead, the area is extremely rugged and full of sharp blocks. Credit: Jaumann et al., Science (2019)
  • New images from asteroid probe offer clues on planet formation
    Image acquired by the DLR-developed MASCAM camera system, taken at night. Credit: Jaumann et al., Science (2019)

Alternatively, temperature changes could have resulted in an electrostatic force that expelled the dust into space. Or water might once have existed on Ryugu, and its evaporation would have carried away the smaller particles.

There's another reason to study asteroids: humankind's survival could one day depend on it.

Ryugu's orbit places it mainly between Earth and Mars. Though it comes close, it's not thought to pose a danger to us, but other asteroids could.

If their composition is like Ryugu's, trying to take them out with a missile would probably just break them into smaller rocks still headed toward Earth.

Hayabusa2 space mission
Main stages of Japan's Hayabusa2 space mission to the Ryugu asteroid

One possibility would be to build a large, reflective solar sail and place it on the asteroid's surface, so that the pressure from solar radiation would gradually alter its course, said Jaumann.

Whatever strategy is adopted, he and other astronomers say it's clear these small, enigmatic bodies are of not-so-small importance in our solar neighborhood.


Explore further

Small fragments of carbon-rich asteroids too fragile to survive atmospheric entry

More information: R. Jaumann el al., "Images from the surface of asteroid Ryugu show rocks similar to carbonaceous chondrite meteorites," Science (2019). science.sciencemag.org/cgi/doi … 1126/science.aaw8627
Journal information: Science

© 2019 AFP

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