About 4.6 billion years ago, the solar system coalesced from an enormous cloud of gas and dust. The sun formed first, and the planets then accreted from the leftover material spinning. Contact online >>
About 4.6 billion years ago, the solar system coalesced from an enormous cloud of gas and dust. The sun formed first, and the planets then accreted from the leftover material spinning...
Our Solar System formed 4.6 billion years ago. 3.8 billion years ago, it was relatively young. All the planets possibly had acquired stable orbits by that time. However, they appeared...
(PhysOrg ) -- Differences in the number and speed of cometary impacts onto Jupiter''s large moons Ganymede and Callisto some 3.8 billion years ago can explain their vastly different...
"Jupiter is the oldest planet of the solar system, and its solid core formed well before the solar nebula gas dissipated, consistent with the core-accretion model for giant planet formation," lead author Thomas Kruijer, of the University of Munster in Germany and Lawrence Livermore National Laboratory in California, said in a statement. [Photos: Jupiter, the Solar System''s Largest Planet]
Theoretical work strongly suggests that Jupiter took shape quite early in the solar system''s history, but the planet''s precise age had remained a mystery, Kruijer and his colleagues said.
The researchers dated Jupiter''s formation and growth by analyzing the ages of certain iron meteorites — shards of the metallic cores of ancient planetary building blocks — that have fallen to Earth. These ages were determined by measuring the abundances of molybdenum and tungsten isotopes. (Isotopes are versions of elements with different numbers of neutrons in their atomic nuclei.)
This work indicated that the meteorites came from two distinct "reservoirs" that were spatially separate for 2 million to 3 million years, beginning about 1 million years after the solar system formed, the researchers said.
"The most plausible mechanism for this efficient separation is the formation of Jupiter, opening a gap in the disk and preventing the exchange of material between the two reservoirs," the researchers wrote in the new study, which was published online today (June 12) in the journal Proceedings of the National Academy of Sciences.
Jupiter''s core would have to be about 20 times more massive than Earth to keep the two reservoirs from mixing, Kruijer and his team calculated. So, the results suggest the nascent gas giant was already that big within the first 1 million years of solar system history, the researchers said.
Jupiter''s growth rate slowed thereafter, they said. The gas giant didn''t reach 50 Earth masses until a minimum of 3 million to 4 million years after the sun''s formation, the researchers determined. (Jupiter is currently about 318 times more massive than Earth.)
"Our measurements show that the growth of Jupiter can be dated using the distinct genetic heritage and formation times of meteorites," Kruijer said in the same statement.
The new study could also help explain why the solar system lacks worlds intermediate in mass between Earth and "ice giants" such as Uranus and Neptune. Such "super-Earths" are relatively common in other star systems.
"One important implication of this result is that, because Jupiter acted as a barrier against inward transport of solids across the disk, the inner solar system remained relatively mass deficient, possibly explaining its lack of any ''super-Earths,''" the researchers wrote in the new study.
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