It is possible to do a forensic study of the Solar System by going to the main asteroid belt. You can find rocks from the Solar System there. asteroids are mostly unaffected by space weathering out in the cold vacuum of space. Space scientists refer to asteroids and meteorites as time capsule because of the evidence they have.

NASA is sending a team to investigate the asteroid Psyche. A team of researchers combined observations of Psyche from telescopes and created a map of the asteroid.

The asteroids are divided into three groups. The most common type of asteroid is carbonaceous. About 75% of known asteroids are made up of them. They are dark because of the carbon. The second most common type is s-type asteroid. Most of the asteroids are made of iron and magnesium silicates.

About 8% of known asteroids are metal or M type. They are thought to be the source of iron meteorites that fall to Earth. One of the earliest sources of iron was the M-type meteorite.

King Tut's iron dagger was concealed in the wrappings surrounding the boy-king's mummy. Image: Daniela Comelli/Polytechnic University of Milan
King Tut was buried with an iron dagger made from an M-type meteorite. Image: Daniela Comelli/Polytechnic University of Milan

Psyche is an M type asteroid. It is a dwarf planet, with a diameter of about 140 miles. The 16th minor planet was called 16 Psyche. Minor planets, like Psyche, are larger asteroids. Psyche has a lot of iron and nickel, which makes it a gold-mine asteroid. Nobody believes it is rich in gold.

Light images of Psyche don't give us a lot. Some pictures of the asteroid were captured by the VLT, but they didn't reveal much.

The Very Large Telescope captured this image of 16 Psyche in August 2019. Image Credit: By ESO/Vernazza et al./MISTRAL algorithm (ONERA/CNRS) - Cropped from: Kalliope and Psyche, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=111158926
The Very Large Telescope captured this image of 16 Psyche in August 2019. Image Credit: By ESO/Vernazza et al./MISTRAL algorithm (ONERA/CNRS) – Cropped from Kalliope and Psyche, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=111158926

The history of Psyche is uncertain. Astronomers thought it was the iron core of a larger body. The body was stripped away by a powerful collision. The bigger body would have been 500 km in diameter. The iron-rich core was the only thing left.

As time went on, the idea fell out of favor with the astronomer. It wasn't dense enough to be a solid iron.

Psyche was disrupted and then re-accreted as a mixture of metals and silicates, according to other researchers. Psyche is more of a rubble pile, according to one study. There was a layer of carbon and other materials on Psyche's surface.

The ferro-volcanic idea is the most exotic of Psyche's beginnings. According to the study, Psyche was once molten. The molten core erupted as iron volcanoes when the outer layers cooled.

This graphic of 16 Psyche is from a 2021 study. It's a smoothed and contour-filled optical albedo map with purported topographical and albedo features labelled. It shows some of the asteroid's surface features like the depressions Eros, Foxtrot, and Panthia. Names with question marks are indeterminate features. The three blurred white spots are optical bright spots and the white circles are radar echo centers. Image Credit: By Michael K. Shepard et al., Asteroid 16 Psyche: Shape, Features, and Global Map (2021), figure 10. https://iopscience.iop.org/article/10.3847/PSJ/abfdba#psjabfdbaf9, CC BY-SA 4.0, https://commons.wikimedia.org/w/index.php?curid=113172869
This graphic of 16 Psyche is from a 2021 study. It’s a smoothed, contour-filled optical albedo map with labelled topographical and albedo features. It shows some of the asteroid’s surface features like the depressions Eros, Foxtrot, and Panthia. Names with question marks are indeterminate features. The three blurred white spots are optical bright spots, and the white circles are radar echo centers. Image Credit: Michael K. Shepard et al., Asteroid 16 Psyche: Shape, Features, and Global Map (2021), figure 10. https://iopscience.iop.org/article/10.3847/PSJ/abfdba#psjabfdbaf9, CC BY-SA 4.0, https://commons.wikimedia.org/w/index.php?curid=113172869

If you want to know what Psyche is, you have to look at it. That is what NASA is doing

The mission is called Psyche and will be launched in the fall of 2022, A gravity-assisted maneuver with Mars will allow the craft to arrive at Psyche. It will take 21 months to study the asteroid and follow four different paths. It will focus on different objectives as it approaches the asteroid.

A new map of Psyche's surface was created by researchers. There is a map in a paper. Saverio Cambioni is from the Department of Earth, Atmospheric and Planetary Sciences at MIT.

The surface of Psyche is heterogeneous. These maps show that metal-rich asteroids are intriguing. The Psyche mission will go to the asteroid.

The authors looked at 16 Psyche using the ALMA. ALMA is a radio telescope. The interferometer operates with a high resolution. ALMA operates at a wavelength that is sensitive to Psyche's surface.

A synthetic signal that is equivalent to a telescope with a diameter of 10 miles can be created by combining the signals of the ALMA antenna. The bigger the telescope, the better.

The map is based on two different things. Thermal inertia is how long a material takes to get to the temperature of its environment. It takes more time because of higher thermal inertia.

The second is the same as the first. A material conducts heat, electricity, or sound with the help of the dielectric constant. A material with a low constant is a bad conductor and a good one.

The researchers ran hundreds of simulations to see which combinations of materials would explain thermal inertia. The simulations were run so that differences in surface properties could be seen.

Iron has a constant. The researchers were able to map the surface and find areas rich in iron. It has high thermal inertia because it is so dense. A good idea of which surface regions are rich in iron and other metals is given by combining thermal inertia and dielectric constant measurement.

This figure from the study shows the thermal inertia (L) and dielectric constant (R) of 16 Psyche's surface as measured by ALMA. Image Credit: Cambioni et al. 2022.
This figure from the study shows the thermal inertia (L) and dielectric constant (R) of 16 Psyche’s surface as measured by ALMA. Image Credit: Cambioni et al. 2022.

A feature on Psyche is called a curious feature. The region has a lower thermal inertia than the highlands. There is a depression just to the right of the asteroid in the image below.

This figure from the paper combines thermal inertia with elevation. The low-elevation Bravo-Golf region is clearly visible. Image Credit: Cambioni et al. 2022.
This figure from the paper combines thermal inertia with elevation. The low-elevation Bravo-Golf region is visible. Image Credit: Cambioni et al. 2022.

The low elevation area has lower thermal inertia. The region is also bright on the radar. What is that? The researchers came up with a few options.

The lowlands could be metal rich but covered with porous regolith that lowers their thermal inertia compared to the highlands. There is an increase in thermal insturment with particle size. Regolith would have pooled in the lowlands.

There are fine-grained materials on small asteroids because of their low gravity. Psyche is a large body, so if fine-grained materials accumulate on the bottom of the depression, this is intriguing.

The surface material is more porous in the lowlands. There is a decrease in thermal inertia as rock becomes more porous. The lowlands could be more porous due to impact Fractures.

The third hypothesis is that the lowlands have more silicate-rich materials than the highlands. The depression may have been formed by an impact with a silicate-rich impactor.

This figure from the study illustrates the three scenarios that might explain the low-thermal-inertia detected in the Bravo-Golf region. Image Credit: Cambioni et al. 2022.
This figure from the study illustrates the three scenarios that might explain the low-thermal-inertia detected in the Bravo-Golf region. Image Credit: Cambioni et al. 2022.

The study shows that 16 Psyche has a lot of different materials on its surface. It adds to the evidence that the asteroid is rich in metal and silicates. It is possible that the asteroid is a remnant of a differentiated body that has lost its mantle and crust. The authors conclude that Psyche is a metal-rich asteroid with both metal and silicate materials.

Simone Marchi is a co- investigator on the NASA Psyche mission. Marchi commented on the importance of the study in a press release. The data shows that Psyche's surface is heterogeneous. One of the main goals of the Psyche mission is to study the composition of the asteroid's surface using a variety of scientific instruments. The Psyche Science Team is eager to learn more about the presence of compositional Heterogeneities.

This animation from the paper shows thermal inertia on 16 Psyche’s surface. The low-elevation Bravo-Golf region is of particular interest. Credit: Cambioni et al. 2022.

It will be up to NASA to confirm these findings more thoroughly.

Sending a craft all the way to Psyche is more than just Psyche.

Psyche is the remnant core of a rocky, differentiated planet. Some of the light elements that we expect are in Earth's core will be contained in it. Earth's core isn't dense enough to hold iron and nickel. Scientists think it has lighter elements.

The Psyche mission will determine if the asteroid formed under more oxidizing or less reducing conditions. That will give us more information about the planets.

Psyche is often referred to as the Gold Mine Asteroid because it is rich in metal. It is unlikely that the iron value of an object of its size will be realized or accessible in the near future.

16 Psyche is a gold mine if knowledge is as valuable as iron.

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