A research group from Kobe University has demonstrated that the heat generated by the impact of a small astronomical body could enable aqueous alteration and organic solid formation to occur on the surface of an asteroid. They achieved this by first conducting high-velocity impact cratering experiments using an asteroid-like target material and measuring the post-impact heat distribution around the resulting crater. From these results, they then established a rule-of-thumb for maximum temperature and the duration of the heating, and developed a heat conduction model from this.
The research group consisted of the following members from Kobe University’s Graduate School of Science; Lecturer YASUI Minami, TAZAWA Taku (a 2nd year masters student at the time of research), HASHIMOTO Ryohei (then a 4th year undergraduate in the Faculty of Science) and Professor ARAKAWA Masahiko, in addition to JAXA Space Exploration Center’s Associate Senior Researcher OGAWA Kazunori (who was a technical specialist at Kobe University at the time of the study).
These results have expanded the spatial and temporal range over which the necessary conditions for aqueous alteration and organic solid formation could occur. This is expected to significantly increase the number of prospective astronomical bodies that could have brought water and the origins of life to Earth.
It is believed that the water and organic substances necessary for life to begin on Earth were the result of a comet or asteroid impacting the planet. Minerals and organic substances that have experienced aqueous alteration have been discovered in meteorites (from which asteroids originate), providing proof that they once contained water. However, a heat source is necessary for the chemical reactions that cause aqueous alteration and organic solid formation inside asteroids.
One sufficiently strong heat source is the radioactive decay heating of 26Al (aluminum, *5), a short-lived radioactive nuclide found inside rocks. However, it is said that the radioactive heating that caused aqueous alteration and solid formation on asteroid parent bodies (*4) could have only occurred at the beginning of the solar system’s history due to the short half-life of 26Al (720,000 years).
In recent years, the theory that the impact heat generated when a small astronomical body hits an asteroid could also be a viable heat source has started to gain attention. However, it is not known how much heat is generated depending on the astronomical body’s characteristics (size, density, impact speed) and how far within the asteroid this generated heat is transmitted. Up until now, there have been no studies that have experimentally investigated this heat generation and propagation process to determine whether aqueous alteration and organic substance formation would be possible.
This research group conducted laboratory experiments to investigate the relationship between the impact heat generated on an asteroid (as a result of a small astronomical body’s impact) and the impact’s characteristics. For the target, they used gypsum (a porous mineral composed of calcium sulfate dihydrate) to imitate an asteroid. They accelerated projectiles at the target at high impact velocities of between 1km/s to 5km/s using Kobe University’s two-stage horizontal gas gun.
Multiple thermocouples were set in the gypsum target in order to measure the temperature changes post-impact. In this series of experiments, the researchers changed the size, density, impact speed of the projectiles and the thermocouples’ positions in order to investigate the differences in heat duration depending on the characteristics of the impact.
From the heat duration graph, the research group investigated the maximum temperature and its duration, and looked at how this related to the impact characteristics. By using the dimensionless distance obtained by normalizing the distance from the impact point (where the projectile hit the target) by the crater radius, they successfully determined how maximum temperature and its duration are altered by impact characteristics and came up with a rule-of-thumb for this.
Subsequently constructing a heat conduction model incorporating this rule of thumb, enabled them to calculate the heat distribution around the crater formed on the asteroid surface. The research group checked the numerical results from the heat conduction model against data on the required heat and duration for aqueous alteration and organic solid formation obtained from past analyses of meteorites.
These results showed that aqueous alteration could occur if a crater with a radius of over 20km was formed within 2au from the Sun. In addition, they estimated that even a small crater with a 100m radius on an asteroid within 4au could heat up to 100C, meaning that it could support organic solid formation. Most asteroids are located within 4au. The researchers also found that if a crater with a radius of over 1km is formed within 2au, the circumference of the crater can heat up to 0C (the temperature at which ice becomes water), thus enabling organic solids to be formed.
It is thought that radioactive decay heating of 26Al triggers the chemical reactions for aqueous alteration and organic solid formation on asteroids. However, this heating can only occur near the core of comparatively large asteroids that are tens of kilometers in diameter.
Furthermore, it is said that this could have only occurred within a million years after the Sun’s formation due to the short half-life of 26Al. On the other hand, collisions between asteroids still occur today, and it is possible that such collisions heat up the surface of even small asteroids, providing that the impact does not destroy the asteroid itself.
In other words, these research results show that the potential for asteroids to support aqueous alteration and organic solid formation is temporarily and spatially far greater than previously thought. This will contribute towards an increased number of astrological bodies being considered as candidates that brought the water and organic substances for the beginning of life on Earth.
Next the research group hopes to examine samples returned from asteroid exploration missions conducted not only by Japan but other countries as well. If aqueously altered minerals or organic substances were to be discovered in the collected samples, this could provide evidence of impact heating’s effects.