A new study led by Western University's all - star cosmochemist Audrey Bouvier proves that the Earth and other
planetary objects formed in the early years of the Solar System share similar chemical origins — a finding at odds with accepted wisdom held by scientists for decades.
Not exact matches
That's at least 100 times larger than the nanodiamonds that
form when
planetary objects collide, and it's far larger than diamonds that
form by condensing from carbon vapor inside clouds of interplanetary gas and dust.
The Earth
formed from an accumulation of gas, dust, and small
planetary objects.
«We show that Imbrium was likely
formed by an absolutely enormous
object, large enough to be classified as a protoplanet,» said Pete Schultz, professor of earth, environmental and
planetary sciences at Brown University.
A layer of iron and other elements deep underground is the evidence scientists have long been seeking to support the hypothesis that the moon was
formed by a
planetary object hitting the infant Earth some 4.5 billion years ago, a new study led by Johns Hopkins University scientists argues.
Now,
planetary scientists have conducted the first computer simulations that bolster a controversial alternative idea: The satellites
formed as our own moon did, after a big
object smashed into the planet and kicked up debris.
The final stages of life for a star like our Sun result in the star blowing its outer layers out into the surrounding space,
forming objects known as
planetary nebulae in a wide range of beautiful and striking shapes.
«The results confirm one of the basic ideas of
planetary formation theory, that most of the Earth
formed by collisions of smaller
objects like carbonaceous chondrites,» says Scott Kenyon at the Harvard - Smithsonian Center for Astrophysics in Cambridge, Massachusetts.
The belt contains essential information about the
planetary formation processes, including both the «cold disk» that harbors the
objects that are thought to
formed in situ with the whole
planetary system, and the «hot / scattered disk» that is the refuge of
objects that are dynamically scattered into it during the dynamical evolution of the inner solar system.
I apply numerical models to investigate the physical and chemical evolution of
planetary materials, ranging from the small dust grains suspended in protoplanetary disks to the many kilometer - scale
objects which accrete together to
form planets.
Well, almost encloses: Enceladus sprays geysers of water ice out into space, some of which settles back down to the moon's surface in the
form of snow, making it the most reflective
planetary object in the solar system.
Oddly enough, Oort Cloud
objects were probably
formed in a region of the proto -
planetary disk that was located closer to the Sun than the Edgeworth - Kuiper Belt
objects that persist in the orbital plane of the planets (ecliptic) to this day.
Using the known decay rates of various radioactive isotopes, he investigates the chronology of early processes on small
planetary objects and studies the chemical and physical aspects of old and young crust -
forming processes on Earth.
Both
objects formed among the rocky and icy protoplanets beyond the Solar System's «ice line» now located around 2.7 AUs, but the early development of Jupiter apparently prevented such large protoplanets between the gas giant and planet Mars from agglomerating into even bigger
planetary bodies, by sweeping many into pulverizing collisions as well as slinging them into the Sun or Oort Cloud, or even beyond Sol's gravitational reach altogether.