Colliding at speeds up to 22,000 miles per hour (36,000 kilometers per hour), such a collision may have stripped most
of the rocky mantle from the protoplanet that became Mercury with its iron - rich core, while a Mars - size protoplanet struck the early Earth off - center and created a spray of mostly mantle material that later accreted to form the Moon.
Not exact matches
Brent spent several years as a post-doctoral scholar at MIT and the National Museum
of Natural History in Washington D.C. researching the Earth's
rocky mantle.
Although its surface is an airless landscape
of cracked ice, all the evidence says that beneath that bleak shell is a liquid water ocean stretching hundreds
of kilometres down to the
rocky mantle below.
The arrays are due to open for real in November to power a two - year mission to probe the guts
of Mars and reveal how
rocky planets» core,
mantle and crust form
Earth's outermost shell is a fragmented jigsaw puzzle
of rocky plates sliding over the
mantle below.
For instance, a catastrophic impact could have stripped away most
of Mercury's
rocky mantle, leaving the planet with its relatively huge iron core.
The presence
of this rock at a site indicates either that material has pushed up through Earth's crust from the
mantle (a silicate
rocky shell between the crust and the core with an average thickness
of 2,886 km and depths ranging from 30 km to almost 3,000 km below the crust) or that a celestial body (a comet, meteor or meteorite) fell there.
Where researchers expected to find a large
mantle plume, the map
of the geologic structure beneath Yellowstone instead seems to show a ghostly fragment
of an old tectonic plate — a former chunk
of Earth's
rocky shell — lodged under the western United States, right near the Yellowstone hot spot.
Published in the current issue
of the journal Nature Geoscience, the paper uses laboratory simulations
of an Earth impact as evidence that a stratified layer beneath the
rocky mantle — which appears in seismic data — was created when Earth was struck by a smaller object.
Scientists have long wondered if the moon's vast subsurface ocean, sandwiched between a
rocky mantle and a global sheet
of ice, could prove as habitable as Earth's early oceans.
At the moment, the team's favored idea is akin to the second solution above: that large bodies
of solid metal slowly dropped from the
rocky mantle and into the core to lower the nucleation barrier.
Previous research showed Eureka is rich the mineral olivine, which forms in the
mantles of large
rocky bodies but is rare in asteroids.
That heat led to the separation
of the primordial body into a
rocky crust, an underlying
rocky mantle, and a central metallic core, hallmarks
of planet Earth and the other
rocky planets.
If Pluto's core was
rocky and its
mantle icy, most
of the material blasted into space by the collision would have been ice, accounting for Pluto's high rock - to - ice ratio today.
The interior
of Vesta, unlike that
of most asteroids, separated into layers resembling a planet's, with a
rocky crust covering a
mantle composed
of the mineral olivine.
Analysis
of data also shows that Ceres has a water - ice
mantle surrounding a
rocky core, and that there may still be at least pockets
of liquid water beneath the surface, raising the prospect
of potential habitability for microorganisms, as seemingly unlikely as that may sound for a world so far from the Sun.
As significant uncertainties about the thickness
of the surface ice still exist, some planetary scientists have identified two possible mechanisms for how possible volcanic heat can escape to the surface from Europa's
rocky mantle and be carried upward by buoyant oceanic currents.
«When our hero travels into Arabia Terra it is described as much
rockier than Acidalia, but the opposite is generally true: much
of Arabia is dust
mantled and smooth at the scale
of a rover,» NASA helpfully explained in the run - up to the release
of the book's movie adaptation.
The interior
of Venus is probably very similar to that
of Earth, with an iron core about 6,000 km (3,700 miles) in diameter radius and a molten
rocky mantle comprising most
of the planet.
As a result, Vesta «differentiated» into a relatively dense metallic core (
of approximately 136 miles or 220 kilometers across), lighter
mantle, and crust, like the
rocky inner planets, many large planetary satellite's like the Earth's Moon, and probably most, if not all,
of the newly named «dwarf planets» like Ceres.
Assuming an iron - rich planet with an internal structure like Earth, modelling results for the first discovered super-Earth (GJ 876 d) indicate the existence
of a threshold in planetary diameter above which a super-Earth «most certainly» has a high water content (an «ocean planet» or «water world,» where thick layers
of water and pressurized ice surround a
rocky mantle and core); this threshold was found to be around 24,000 kilometers (or nearly 15,000 miles) in the particular case
of GJ 876 d (Valencia et al, 2007).
It really all depends
of course on the
rocky types
of mantle and their makeup at depth and the amount
of glacial melt being returned to the oceans, the amount
of rainfall vs snowfall, the amount
of water no longer being tied up in the icy environment as well as that melted from prior eras.
The author tells us that on timescales
of 35 million years and more the Earth actually «breathes,» exhaling carbon dioxide from volcanoes and hot springs (many
of the latter undersea), and inhaling it from the atmosphere into the oceans and forests — and eventually into the
rocky crust, or even the fiery
mantle beneath.