STUDY OF METEORITES THAT FORMED THE EARTH IN THE OUTER SOLAR SYSTEM
Tokyo:
According to a study, the materials that formed the Earth may have originated
quite far out in the early solar system and then been brought in during the
solar system's turbulent early history.
Carbonaceous
meteorites, which are assumed to have come from outer main-belt asteroids, are
supposed to have contributed to Earth's formation.
According
to a new study led by Tokyo Institute of Technology experts, these asteroidal
materials may have formed far out in the early solar system and then been
brought into the inner solar system by chaotic mixing processes.
The
findings, which were published in the journal AGU Advances, suggest that the
surface minerals found on outer main-belt asteroids, particularly ammonia
(NH3)-bearing clays, are formed from starting materials containing NH3 and CO2
ice that are only stable at very low temperatures and in water-rich
environments.
The
study suggests that outer main-belt asteroids formed in distant orbits and
differentiated to generate various materials in water-rich mantles and
rock-dominated cores based on these findings.
Using
computer simulations, the researchers studied the chemical evolution of
numerous possible primordial mixes meant to imitate primitive asteroidal
materials to explain the source of inconsistencies in the recorded spectra of
carbonaceous meteorites and asteroids. They then used these computer models to
construct simulated reflectance spectra for comparison to the telescopically
obtained ones.
According
to their models, the starting material had to contain a significant amount of
water and ammonia, a low abundance of carbon dioxide (CO2), and react at
temperatures below 70 degrees Celsius in order to match the asteroid spectra,
implying that asteroids formed much further out than their current locations in
the early solar system.
If
this theory is correct, Earth's formation and distinctive traits are the
outcome of odd aspects of the solar system's formation.
"Whether
our solar system's birth is a typical consequence remains to be
determined," said lead author Hiroyuki Kurokawa of the Institute's
Earth-Life Science Institute, "but several measurements suggest we may be
able to set our cosmic history in perspective shortly" (ELSI).
There
will be multiple opportunities to put this concept to the test; for example,
this study predicts what will be discovered when Hayabusa 2 returning samples
are analysed. Hayabusa is the asteroid sample-return mission of Japan's
national space agency, JAXA.
If
this theory about asteroids' distant origins is right, ammoniated salts and
minerals will be found in Hayabusa 2's samples. Analyses of recovered samples
from NASA's OSIRIS-Rex mission will give an additional check on this model.
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