Two possible ways that the inner solar system received water are: water molecules sticking to dust grains inside the «snow line» (as shown in the inset) and carbonaceous
chondrite material flung into the inner solar system by the effect of gravity from protoJupiter.
This abundance is lower than model estimates of ultraviolet (UV) degradation of accreted interplanetary dust particles (IDP's) or carbonaceous
chondrite material.
Not exact matches
McCord's grad students set to work on the data and came up with some preliminary findings: Ceres was a carbonaceous
chondrite (a type of asteroid composed of water locked in minerals and carbon - based
materials), and it had not been thermally altered.
On his desk at ASU are some polished slices of NWA 6991, a speckled, black stone known as a carbonaceous
chondrite: the most primitive type of meteorite containing some of the first
material from the solar system's youth.
This suggests that the value of K / U ≈ 1 X 104 is characteristic of terrestrial
materials and is distinct from the value of 8 X 104 found in
chondrites.
Deimos is composed of rock rich in carbonaceous
material, much like C - type asteroids and carbonaceous
chondrite meteorites.
Scientists have speculated that a rain of carbonaceous
chondrites may have seeded early Earth with the raw
material for biology here.
«We now know something like an enstatite
chondrite was the starting
material for Mercury, which is surprising, because they are about 10 standard deviations away from all other
chondrites,» Grove says.
Fred Ciesla, an associate professor of planetary science at the University of Chicago, says the findings may reclassify
chondrites, a class of meteorites that are thought to be examples of the original
material from which planets formed.
«The most primitive meteorites, the carbonaceous
chondrites, are primarily mixtures of many distinct
materials that reflect a variety of solar nebular environments as well as planetary processing.»
«The complex suite of organic
materials in carbonaceous
chondrite meteorites probably originally formed in the interstellar medium and / or the solar protoplanetary disk, but were subsequently modified in the meteorites» asteroidal parent bodies.
One type, called carbonaceous
chondrites, contain some of the most - primitive known samples of Solar System
material, including a lot more xenon than is found in our own planet's atmosphere.