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Mars’ Interior: Deep Planetary Scan Confirms Martian Core

An illustration of the Martian interior. Credit: Dr Sheng Wang and Professor Hrvoje Tkalcic/ANU

A new method to scan the deep interior of planets in our solar system to confirm whether they have a core at the heart of their existence has been developed by seismologists from the Australian National UniversityFounded in 1946, the Australian National University (ANU) is a national research university located in Canberra, the capital of Australia. Its main campus in Acton encompasses seven teaching and research colleges, in addition to several national academies and institutes.” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]”>Australian National University (ANU).  

Functioning in a similar way to an ultrasound scan using sound waves to generate images of a patient’s body, the scanning method requires only a single seismometer on a planet’s surface in order to work. It can also be used to confirm the size of a planet’s core. The research was published on October 27 in the journal Nature Astronomy.  

Using the ANU model to scan the entirety of MarsMars is the second smallest planet in our solar system and the fourth planet from the sun. It is a dusty, cold, desert world with a very thin atmosphere. Iron oxide is prevalent in Mars' surface resulting in its reddish color and its nickname "The Red Planet." Mars' name comes from the Roman god of war.” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]”>Mars’ interior, the researchers confirmed the Red Planet has a large core at its center – a theory first confirmed by a team of scientists in 2021.

Study co-author Professor Hrvoje Tkalcic, from ANU, said that based on data collected using the ANU technique, the researchers determined that the Martian core, which is smaller than Earth’s, is about 3,620 kilometers (2,250 miles) in diameter. 

“Our research presents an innovative method using a single instrument to scan the interior of any planet in a way that’s never been done before,” he said.   

Confirming the existence of a planetary core, which the researchers refer to as the “engine room” of all planets, can help scientists learn more about a planet’s past and evolution. It can also help scientists determine at what point in a planet’s history a magnetic field formed and ceased to exist.

The core plays an active role in sustaining a planet’s magnetic field. In the case of Mars, it could help explain why, unlike Earth, the Red Planet no longer has a magnetic field – something that is critical to sustaining all life forms.   

“Modelling suggests that the Martian core is liquid and while it is made up of mostly iron and nickel, it could also contain traces of lighter elements such as hydrogen and sulfur. These elements can alter the ability of the core to transport heat,” lead author Dr. Sheng Wang, who is also from ANU, said. 

“A magnetic field is important because it shields us from cosmic radiation, which is why life on Earth is possible.”

Using a single seismometer on Mars’ surface, the ANU team measured specific types of seismic waves. The seismic waves, which were triggered by marsquakes, give off a spectrum of signals, or “echoes”, that change over time as they reverberate throughout the Martian interior.  

These seismic waves pierce through and bounce off the Martian core. 

Professor Tkalcic said researchers are interested in the “late” and “weaker” signals that can survive hours after they are emitted from quakes, meteoroid impacts, and other sources.  

“Although these late signals appear to be noisy and not useful, the similarity between these weak signals recorded at various locations on Mars manifests itself as a new signal that reveals the presence of a large core in the Red Planet’s heart,” Professor Tkalcic said. 

“We can determine how far these seismic waves travel to reach the Martian core but also the speed at which they travel through Mars’ interior. This data helps us make estimations about the size of Mars’ core.” 

According to the researchers, their method of using a single seismometer to confirm the presence of a planetary core is also a “cost-effective solution.”

“There is a single seismic station on Mars. There were four of them on the Moon in 1970s. The situation of having a limited number of instruments is unlikely to change in the coming decades or even this century due to high cost,” Dr. Wang said.

“We need an approach right now to use only a single seismometer to study planetary interiors.”

The researchers hope this new ANU-developed technique involving a single seismometer could be used to help scientists learn more about our other planetary neighbors, including the moon. 

“The US and China plan to send seismometers to the moon, and Australia also has ambitions to participate in future missions, so there’s potential for further studies using new and more sophisticated instruments,” Professor Tkalcic said.  

Dr. Wang said: “Although there are many studies on planetary cores, the images we have of planetary interiors are still very blurry. But with new instruments and methods like ours, we’ll be able to get sharper images which will help us answer questions such as how big the cores are and whether they take a solid or liquid form. 

“Our method could even be used to analyze the JupiterJupiter is the largest planet in the solar system and the fifth planet from the sun. It is a gas giant with a mass greater then all of the other planets combined. Its name comes from the Roman god Jupiter.” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]”>Jupiter moons and the outer solar system planets that are solid.” 

To carry out their research, ANU scientists used data collected from a seismometer attached to NASA’s InSight lander, which has been collecting information about marsquakes, Martian weather, and the planet’s interior since touching down on Mars in 2018.

Reference: “Scanning for planetary cores with single-receiver intersource correlations” by Sheng Wang and Hrvoje Tkalcic, 27 October 2022, Nature Astronomy.
DOI: 10.1038/s41550-022-01796-8

Source: SciTechDaily