Meteorites from Mars suffer a velocity boost due to the material pileup
(11 December 2017 - Chiba Institute of Technology; Tokyo Institute of Technology) Researchers have performed numerical simulations to explore the launch mechanism of Martian meteorites.
According to the knowledge of shock physics, a strong shock compression higher than 50 GPa is required to accelerate Martian materials up to the escape velocity of Mars (5 km/s). In contrast, detailed analysis of Martian meteorites shows that they suffer only 30-50 GPa during the ejection. The researchers found that a material pileup in an excavation flow causes a significant velocity boost of materials near the surface without strong compression. This newly discovered "late-stage acceleration" could play an important role not only in the launch of Martian meteorites, but also in the context of the (Litho-) Panspermia.
An infographic on the generation of Martian meteorites. The inset shows the figure shows the hydrodynamic behavior during a projectile penetration. The color bar indicates the temporal pressures of the data point. Selected six tracers with velocity vectors are indicated as filled circles. The tracer overlays at the same depth of the tracers are also shown. A material pileup is obvious, showing that the materials initially located at a deeper position (ex. Purple circle) extrude the surface materials (ex. Red circle). The temporal pressure at the root of the ejecta curtain, where the late-stage acceleration occurs, reaches 10 GPa despite the height of the materials having already excessed ground level. The new finding suggests that the material transportation due to hypervelocity impacts, as illustrated here, occurs more easily than what was previously thought. (courtesy: Chiba Institute of Technology; Tokyo Institute of Technology)
One hundred and ninety-eight meteorites from Mars have been discovered on Earth as of Sep. 2017. Hypervelocity impacts on Mars have been a widely accepted mechanism that launches Martian rocks into the space. Petrographic analyses of the Martian meteorites have shown that they suffer relatively low peak pressure ranging from 30 to 50 GPa during impact ejection events. In contrast, shock physics tells us that a stronger shock compression higher than 50 GPa is required to accelerate materials up to the escape velocity of Mars (5 km/s). This contradiction between petrology and shock physics was the outstanding problem regarding the Martian meteorites' launch.
The researchers numerically modeled a vertical impact onto the Martian surface using two independent hydrocodes (iSALE code and SPH code) to explore the launch mechanism of the Martian meteorites. The impact-driven pressure field and material movements near the impact point has been investigated in detail. The maximum spatial resolution in the computation employed in this study is one order of magnitude higher than that used in the previous studies.
Overview of Research Achievement
The research team found that a velocity boost of surface materials occurs due to a material pileup in an impact-driven excavation flow without strong shock compression (See Figure 1). The newly discovered velocity boost mechanism has been named "late-stage acceleration". The parts of the ejecta mass that experienced 30-50 GPa and were ejected higher than 5 km/s were investigated. Although the mass is limited to 0.1-1% of the projectile mass, this is sufficient for hypervelocity impacts to have been a plausible mechanism for the ejection of Martian meteorites.
The new discovery of late-stage acceleration has a wide range of implications not only for the Martian meteorites' launch, but also for material exchange amongst planetary bodies (See Figure 1). Since microbes may survive the relatively weak shock compression, the late-stage acceleration could provide us with new insight into (Litho-) Panspermia. The researchers are planning to do a series of hypervelocity impact experiments to validate the numerically discovered new mechanism using a two-stage light gas gun installed at the Planetary Exploration Research Center, Chiba Institute of Technology, Japan.
Kosuke Kurosawa, Takaya Okamoto, Hidenori Genda, Hydrocode modeling of the spallation process during hypervelocity impacts: Implications for the ejection of Martian meteorites, Icarus, 301, 219-234, DOI: 10.1016/j.icarus.2017.09.015
About Chiba Institute of Technology
Chiba Institute of Technology was established in 1942, as Koa Institute of Technology, in Tokyo, in response to growing social demand for technology education. In 1946, the university was relocated to Chiba, and was renamed the Chiba Institute of Technology. In 2016, 3 faculties were reorganized into 5 faculties (the Faculties of Engineering, Creative Engineering, Advanced Engineering, Information and Computer Science, and Social Systems Science) with 17 departments; and 3 graduate schools (the Graduate Schools of Engineering, Information and Computer Science, and Social Systems Science) with 9 programs. With approximately 10,000 students studying in the programs, the university are one of the largest technological universities in Japan.
The Planetary Exploration Research Center (PERC) was established in 2009 under Chiba Institute of Technology to explore the field of astrobiology, which involves studying the origin, evolution, distribution and future of life in the universe. PERC conducts research and development in collaboration with other organizations in Japan and overseas, including JAXA (Japan), NASA (US), and ESA (Europe).
About Tokyo Institute of Technology
Tokyo Institute of Technology stands at the forefront of research and higher education as the leading university for science and technology in Japan. Tokyo Tech researchers excel in a variety of fields, such as material science, biology, computer science and physics. Founded in 1881, Tokyo Tech has grown to host 10,000 undergraduate and graduate students who become principled leaders of their fields and some of the most sought-after scientists and engineers at top companies. Embodying the Japanese philosophy of "monotsukuri," meaning technical ingenuity and innovation, the Tokyo Tech community strives to make significant contributions to society through high-impact research.
Launched in 2012, ELSI is one of Japan's ambitious World Premiere International research centers, whose aim is to achieve progress in broadly inter-disciplinary scientific areas by inspiring the world's greatest minds to come to Japan and work on the most challenging issues as a collaborative effort. ELSI's primary aim is to address the co-origin and co-evolution of the Earth and life.
The World Premier International Research Center Initiative (WPI) was launched in 2007 by the Ministry of Education, Culture, Sports, Science and Technology (MEXT) in a drive to build "globally visible" research centers in Japan. These institutes aim to boast a very high research standard and outstanding research environment that attracts frontline researchers from around the world to come and work in them. These centers are given a high degree of autonomy, allowing them to revolutionize conventional modes of research operation and administration in Japan.