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Scientists believe early cosmic impacts may have influenced the evolution of Mars, and this suggests that the Red Planet formed much slower than previously thought.
The early solar system was a violent, chaotic place, where planetesimals — small protoplanets measuring up to 1,200 miles (1,900 kilometers) in diameter — asteroids and other debris collided, shaping the planets and celestial bodies we know today.
A new study from the Southwest Research Institute (SwRI) in San Antonio shows that Mars was likely struck by planetesimals early in its history. These large, long-ago collisions introduced “iron-loving” elements to the Red Planet, and those elements, in turn, influenced how quickly the planet formed, according to a statement from SwRI.
Using Martian meteorite samples found on Earth, the researchers were able to model the mixture of materials that formed the early Martian mantle. The study revealed that Mars received a variety of elements — such as tungsten, platinum and gold — that are attracted to iron as a result of these collisions.
“To investigate this process, we performed smoothed-particle hydrodynamics impact simulation,” Simone Marchi, lead author of the study from SwRI, said in the statement. “Based on our model, early collisions produce a heterogeneous, marble-cake-like Martian mantle.”
This illustration shows how early Mars may have looked, with signs of liquid water, large-scale volcanic activity and heavy bombardment from planetary projectiles. (Image credit: SwRI/Marchi)
The meteorite samples suggest that planetesimals bombarded the Red Planet sometime after the planet’s primary core formed. That’s because “iron-loving” elements like tungsten, platinum and gold generally migrate from a planet’s mantle to its central iron core during formation, according to the statement. “Evidence of these elements in the Martian mantle as sampled by meteorites are important because they indicate that Mars was bombarded by planetesimals sometime after its primary core formation ended,” SwRI said in the statement.
Earlier studies of the ratio of tungsten isotopes in the Martian meteorite samples suggested that Mars grew rapidly, within 2 million to 4 million years after the solar system began forming, about 4.6 billion years ago. Because tungsten isotopes are produced via radioactive decay processes over time, the ratio of these isotopes in the mantle of Mars provides a clue about the timeline of the planet’s formation.
However, the new models show that early, large collisions could have altered the ratio of elements in the Martian mantle, meaning the planet may have formed over a period of up to 20 million years.
Researchers at the Southwest Research Institute in San Antonio performed high-resolution simulations of a large projectile hitting early Mars after the planet’s core and mantle formed. The projectile’s core and mantle particles are indicated by brown and green spheres, respectively, showing how the projectile’s materials assimilated into the Martian mantle. (Image credit: SwRI/Marchi)
“Collisions by projectiles large enough to have their own cores and mantles could result in a heterogeneous mixture of those materials in the early Martian mantle,” Robin Canup, co-author and assistant vice president of SwRI’s Space Science and Engineering Division, said in the statement. “This can lead to different interpretations on the timing of Mars’ formation than those that assume that all projectiles are small and homogenous.”
The findings, published Wednesday (Feb. 12) in the journal Science Advances, provide insight on how Mars evolved and how early collisions affected the planet’s formation. The Martian meteorites found on Earth are believed to be the result of more recent collisions with the Red Planet. These meteorite samples offer a unique view into Mars’ past, as they contain a record of the planet’s history, the researchers said.
“To fully understand Mars, we need to understand the role the earliest and most energetic collisions played in its evolution and composition,” Marchi said in the statement.
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