Raumfahrt - Mission zur Metallwelt von Asteroid Psyche -Update-2


Psyche: Metal world mission targets 'iron volcanoes'


Artwork: The Psyche mission will launch towards its target in 2022

Up until now, the worlds we've visited with robotic spacecraft have been composed largely of rock, ice and gas.

But a Nasa mission due to launch in 2022 will visit an object thought to be made largely of metal.

16 Psyche is part of the asteroid belt - the sprawling mass of planetary leftovers that orbits the Sun between Mars and Jupiter.

About the size of the US state of Massachusetts, Psyche is the largest metallic asteroid known to science.

But how did this 200km-wide metal world come to be?

As planetary building blocks joined together to form bigger and bigger objects in the early Solar System, some became so large and hot that they melted. This process, called differentiation, allowed heavier constituents like iron to sink to the interior.

This resulted in some objects, like Earth, forming a rocky crust and mantle around an iron-nickel core. The core is the source of our planet's magnetic field, which protects the atmosphere from being stripped away by charged particles from space.

A widely held idea is that 16 Psyche is the exposed core of an extinct world, perhaps as large as Mars. This proto-planet must have been pounded by other objects, removing the rocky outer layers and leaving just the iron-nickel innards prone to the vacuum of space.


Prof Elkins-Tanton says the first task for the mission is to test whether Psyche is indeed a planetary core

Lindy Elkins-Tanton is principal investigator for Nasa's mission to Psyche. She said the first task for the mission after arriving in 2026 was to test the idea 16 Psyche was indeed a planetary core.

"It might be solid metal, or it might be a pile of rubble that's mostly metal," Prof Elkins-Tanton told BBC News.

"So there are a bunch of different hypotheses over what it might be and how it might have formed."

After that, "we will go on to understand what its composition is", she explained. "Would it be compositionally similar to what we think the Earth's core is, or very different from that?"

The mission will seek to understand the asteroid's surface features, or topography. It's not known whether metallic objects like 16 Psyche are covered in a superficial layer of regolith - the dust, soil or bashed-up rock that's found at the surface of the Earth, the Moon, Mars and some asteroids. In addition, says Prof Elkins-Tanton, "we don't know what impacts into metal look like - they could look very different from impacts into rock or ice".

Scientists want to understand whether the metal asteroid produced a magnetic field as it cooled. If the asteroid froze from the inside out, similar to the cores of Earth and Mercury, there will be no record of one. But if Psyche froze from the outside in, as scientists hope, its crust may retain a magnetic memory, allowing the spacecraft to measure and map the asteroid's remnant magnetic field.

Outside-in cooling would also open the door to a process never before seen before on a celestial body: sulphur-iron volcanism.

"One of the things that happens when metal freezes is that it loses about 7% of its volume. So we have a crust that's solid and the inside is continuing to solidify, but it's losing its volume as it solidifies," said Prof Elkins-Tanton, from Arizona State University (ASU) in Tempe. "The crust has to crack and settle to accommodate the loss of volume during freezing."


A 3D-printed model of Psyche. This is one imagining of how the asteroid looks, but we have no idea what its surface is like

Studies of iron meteorites have shown that a sulphur-rich fluid sometimes forms inside the parent body. "We think that could get squeezed out through the cracks and form a kind of sulphur-iron volcanism on the cooling Psyche," said the mission's principal investigator.

She said the team was "super-excited about this", but explained that it was "completely hypothetical".

"Our very best and favourite model for Psyche is that it froze from the outside in, recording its [magnetic] field and that it would be covered in the now billions-of-years-old remnants of sulphur volcanoes," she explained.

The mission will be discussed this week at the 50th Lunar and Planetary Science Conference (LPSC), here in The Woodlands, outside Houston.

The Psyche spacecraft will also test several important technological innovations. The engine uses inert gases - energised by electric power from the solar arrays - to provide gentle, non-stop thrust.

This solar-electric propulsion (SEP) system saves on fuel mass compared with conventional chemical propulsion, allowing the spacecraft to enter orbit around 16 Psyche and freeing up space for science instruments.

During flight, controllers will also test a communications system that uses laser light, rather than conventional radio waves.

The mission was formally chosen by Nasa in March 2018, along with a separate asteroid mission called Lucy. The Lucy mission will launch in 2021 to explore the Trojans, a group of asteroids that share Jupiter's orbit around the Sun.

Quelle: BBC


Update: 9.04.2019


Iron volcanoes may have erupted on metal asteroids

NASA's upcoming mission to the asteroid Psyche could look for signs of past eruptions, and evidence of 'ferrovolcanism' may also turn up in iron meteorites

Metallic asteroids are thought to have started out as blobs of molten iron floating in space. As if that's not strange enough, scientists now think that as the metal cooled and solidified, volcanoes spewing liquid iron could have erupted through a solid iron crust onto the surface of the asteroid.

This scenario emerged from an analysis by planetary scientists at UC Santa Cruz whose investigation was prompted in part by NASA's plans to launch a probe to Psyche, the largest metallic asteroid in the solar system. Francis Nimmo, professor of Earth and planetary sciences, said he was interested in the composition of metallic asteroids indicated by analyses of iron meteorites, so he had graduate student Jacob Abrahams work on some simple models of how the asteroids cooled and solidified.

"One day he turned to me and said, 'I think these things are going to erupt,'" Nimmo said. "I'd never thought about it before, but it makes sense because you have a buoyant liquid beneath a dense crust, so the liquid wants to come up to the top."

The researchers described their findings in a paper that has been accepted for publication in Geophysical Research Letters and is available online.

Metallic asteroids originated early in the history of the solar system when planets were beginning to form. A protoplanet or "planetesimal" involved in a catastrophic collision could be stripped of its rocky outer layers, exposing a molten, iron-rich core. In the cold of space, this blob of liquid metal would quickly begin to cool and solidify.

"In some cases it would crystallize from the center out and wouldn't have volcanism, but some would crystallize from the top down, so you'd get a solid sheet of metal on the surface with liquid metal underneath," Nimmo said.

As for what the iron volcanoes would look like, Abrahams said it depends on the composition of the melt. "If it's mostly pure iron, then you would have eruptions of low-viscosity surface flows spreading out in thin sheets, so nothing like the thick, viscous lava flows you see on Hawaii," he said. "At the other extreme, if there are light elements mixed in and gases that expand rapidly, you could have explosive volcanism that might leave pits in the surface."

NASA's Psyche mission is scheduled to launch in 2022 and reach the asteroid in 2026. Signs of past volcanism that researchers could look for include variations in the color or composition of material on the surface, and possibly features that look like volcanic vents. Large volcanic cones are probably unlikely, Abrahams said.

Unfortunately, because metallic asteroids would have solidified fairly quickly after their formation, there has been plenty of time (billions of years) for any surface features of volcanism to be degraded. "It's not clear what they might look like now," Abrahams said.

The best opportunity to find evidence of ferrovolcanism on metallic asteroids might actually come from studying iron meteorites already in collections on Earth, the researchers said.

"There are lots of these metallic meteorites, and now that we know what we're looking for, we might find evidence of volcanism in them," Nimmo said. "If material got erupted onto the surface, it would cool very fast, which would be reflected in the composition of the meteorite. And it might have holes in it left by escaping gas."

When they presented their findings at a recent Lunar and Planetary Science Conference, Abrahams and Nimmo discovered that another research team had independently arrived at similar conclusions about the possibility of ferrovolcanism.

"It's not a shocking idea, but we'd just never thought about iron volcanism before, so it's something new and interesting to investigate," Abrahams said.

This research was supported in part by NASA.