«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.
``... every metamorphosed ordinary
chondrite has been shocked and subsequently heated, some of them multiple times.»
u «An H3 — 6
chondrite called Zag fell in the Moroccan Sahara desert five months [after the Monahans meteorite] that also had halite crystals with water inclusions.»
The Chelyabinsk meteorite is a low iron, low metals
chondrite (stony meteorite).
This period was apparently associated with increased meteoric impacts (around 100 times more frequent than today) associated with the break - up in the Main Asteroid Belt of the L -
chondrite parent body — the largest documented asteroid breakup event over the past few billion years.
Due to its rarity, Cooke reckons 30 grams of CM
chondrite is worth about $ 6000.
The Murchison meteorite, a large CM
chondrite that made landfall in Australia in 1969, is now one of the most studied rocks in the world.
Some chondrite classes have up to a few percent of carbon in the dark rock matrix, but not in the chrondules, in which it got lost because of flash - heating events.
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.
They also determined, based on this rapid cooling rate and the composition of lava deposits on Mercury's surface, that the planet likely has the composition of an enstatite
chondrite — a type of meteorite that is extremely rare here on Earth.
«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.
They found the closest match to be an enstatite
chondrite, an extremely rare form of meteorite that is thought to make up only about 2 percent of the meteorites that fall to Earth.
Physicist John Remo holds a slice of the Leoville
chondrite, a meteorite billions of years old.
Based on data obtained with the Gamma Ray and Neutron Detector aboard the Dawn spacecraft, Prettyman et al. (p. 242, published online 20 September) show that Vesta's reputed volatile - poor regolith contains substantial amounts of hydrogen delivered by carbonaceous
chondrite impactors.
The 1,100 - pound (500 kilogram) meteorite is an ordinary H5
chondrite, a type of stony meteorite responsible for 31 percent of Earth's impacts.
Deimos is composed of rock rich in carbonaceous material, much like C - type asteroids and carbonaceous
chondrite meteorites.
But
the chondrite signatures are too heavy to explain the deep Earth samples, Hallis says.
There is one other LL
chondrite whose orbit is known: the asteroid Itokawa, which the Japanese Hayabusa spacecraft visited in 2005.
They moreover show that the light signature emitted by Phobos and Deimos is incompatible with that of the primordial matter that formed Mars (meteorites such as ordinary
chondrite, enstatite
chondrite and / or angrite).
The meteorite's composition matches that of an LL
chondrite, — the LL stands for Low iron, Low metals.
Edwin Thompson holds a large slice of enstatite
chondrite meteorite that fell in Alberta, Canada, in 1952.
Early accretion of water in the inner solar system from a carbonaceous
chondrite - like source.
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 abundance is lower than model estimates of ultraviolet (UV) degradation of accreted interplanetary dust particles (IDP's) or carbonaceous
chondrite material.
It didn't have the heft of
a chondrite, which are typically rich in dense metals.
Almost on a whim, Piatek paid $ 6000 for the stone — cheap in the meteorite world — thinking it was nothing more than a regular
chondrite.
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.
The characterization of Annama indicates that this is an ordinary H5
chondrite, a group of meteorites with high strength that constitutes 31 % of meteorite falls.
The cores of the worlds studied by Bouquet and his co-authors are thought to have
chondrite - like compositions.
Using a new analytical technique, the team looked at different kinds of
chondrite meteorites, a type of primitive meteorite approximately 4.6 billion years old.
A recent analysis of
chondrites by Carnegie's Myriam Telus was concerned with iron - 60, a short - lived radioactive isotope that decays into nickel - 60.
Measuring the amount of these daughter isotopes can tell scientists when, and possibly how,
the chondrites formed.
But carbonaceous
chondrites are known to have formed later than other meteorites — so it was possible that their peculiar isotopic chemistry reflected changes over time in the disk, rather than a distinct place of origin.
Like a chemical fingerprint, the isotopic ratio between Earth's samples and the carbonaceous
chondrites» samples matched.
Some of that water was contained as ice in primitive meteorites called carbonaceous
chondrites.
Radioactive isotopes of elements such as uranium, potassium, and thorium are found in a class of rocky meteorites known as
chondrites.
These results show also that Mercury likely formed with enstatite
chondrites.
The vast majority are
chondrites, pieces of asteroids filled with little glassy beads called chondrules.
The stone's noble gas content supports an extraterrestrial origin, while the presence of tiny diamonds — larger than nanodiamonds found in a common kind of meteorite called
chondrites, but similar in size to diamond aggregates known to be formed by impacts — supports a cometary origin.
Water and other volatile elements arrived on Earth via meteorites called carbonaceous
chondrites.
Though the cometary region is now ruled out, the exact birthplace of the carbonaceous
chondrites is far from certain, says Fred Ciesla, a researcher at the University of Chicago.
Microscopic analyses of
chondrites, the oldest rocks in the solar system, are filling in details of what our neighborhood in space was like shortly before the planets formed
Or, the proto - moon and proto - Earth were showered by the same family of carbonaceous
chondrites soon after they separated, said James Van Orman, professor of earth, environmental and planetary sciences at Case Western Reserve, and a co-author.
The investigators found that the deuterium / hydrogen ratio in the melt inclusions was relatively low and matched the ratio found in carbonaceous
chondrites.
In total, the effects proved to be small for the melt inclusions, and the ratios remained consistent with the those of
the chondrites.
Stony meteorites, or
chondrites — such as this fragment of the Axtell meteorite, found in Texas in 1943 — are among the most common larger pieces.
Most knowledge about the first solid bodies in the solar system comes from meteorites called carbonaceous
chondrites, thought to be chunks of the first asteroids.
«The carbonaceous
chondrites don't really work.»
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.
For one, the new data throw a wrench in the conventional story that carbonaceous
chondrites — a water - rich variety of asteroid — delivered water to an initially dry Earth after its formation.