Thinking small has enabled an international team of scientists to gain new insight into the evolution
of planetary building blocks in the early solar system.
«Chondrules were long viewed
as planetary building blocks,» states Maria Zuber, Professor of Geophysics and MIT's vice president for research.
In a fascinating set of projects we will look at the smallest scales and back in time, probing the mineralogy and composition of micron - sized grains in ancient meteorites using the most sophisticated microscopic techniques, to explore the history of volatiles and organics in
planetary building blocks at the time when the Solar System was young.
Then, the team used a computer program to test different compositions of
basic planetary building blocks to determine which makeups would yield planets with those densities.
One ERS program will stare into the hearts of neighboring nascent star systems to watch ices, organic molecules and
other planetary building blocks dance around coalescing suns.
We will carry out a series of numerical investigations to understand how organics and volatiles are incorporated
into planetary building blocks and then trace the dynamical evolution of these building blocks throughout the period of planetary assembly.
«Here we have a rare opportunity to study a phenomenon that plays out over many decades and provides a window into the types of environments around stars that could
represent planetary building blocks at the very end of a star system's life.»
Computer models have shown that the early solar system was a tumultuous billiards table, with dozens or even hundreds
of planetary building blocks the size of Earth bouncing around.
However,
another planetary building block does appear to linger: the gaseous parts of the disks, perhaps fostering additional growth of gas - giant planets like Jupiter for millions of years.
Comets, like asteroids, are
planetary building blocks that were never incorporated into planets.
In research published this week in Astrophysical Journal Letters, Dr Zoe Leinhardt and colleagues from Bristol's School of Physics have completed computer simulations of the early stages of planet formation around the binary stars using a sophisticated model that calculates the effect of gravity and physical collisions on and between one million
planetary building blocks.