It didn't have the heft
of a chondrite, which are typically rich in dense metals.
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.
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
In total, the effects proved to be small for the melt inclusions, and the ratios remained consistent with
the those of the chondrites.
Not exact matches
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.
Some
of that water was contained as ice in primitive meteorites called carbonaceous
chondrites.
The cores
of the worlds studied by Bouquet and his co-authors are thought to have
chondrite - like compositions.
Radioactive isotopes
of elements such as uranium, potassium, and thorium are found in a class
of rocky meteorites known as
chondrites.
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 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.
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.
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.
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.
This abundance is lower than model estimates
of ultraviolet (UV) degradation
of accreted interplanetary dust particles (IDP's) or carbonaceous
chondrite material.
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.
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.
Early accretion
of water in the inner solar system from a carbonaceous
chondrite - like source.
Edwin Thompson holds a large slice
of enstatite
chondrite meteorite that fell in Alberta, Canada, in 1952.
The meteorite's composition matches that
of an LL
chondrite, — the LL stands for Low iron, Low metals.
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.
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).
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.
This will permit the average terrestrial concentrations
of uranium and thorium to be 2 to 4.7 times higher than that observed in
chondrites.
Deimos is composed
of rock rich in carbonaceous material, much like C - type asteroids and carbonaceous
chondrite meteorites.
He might ask, «What's the range
of iron content in the ordinary
chondrites?»
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.
It appears similar to a group
of asteroids known as carbonaceous
chondrites.
Scientists have speculated that a rain
of carbonaceous
chondrites may have seeded early Earth with the raw material for biology here.
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.
Physicist John Remo holds a slice
of the Leoville
chondrite, a meteorite billions
of years old.
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.
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.
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.
That, combined with nitrogen isotope data, points to carbonaceous
chondrites as the most likely common source
of water.
The measurements show that 4 - Vesta contains the same hydrogen isotopic composition as carbonaceous
chondrites, which is also that
of Earth.
The most primitive known meteorites, carbonaceous
chondrites, were formed in the same swirl
of dust, grit, ice and gasses that gave rise to the sun some 4.6 billion years ago, well before the planets were formed.
The study's authors turned to another potential source
of Earth's water — carbonaceous
chondrites.
In the samples
of mantle gas taken by Holland and his colleagues, the krypton measurements were heavy, producing «something that looks rather like gases that are trapped in primitive
chondrites today,» Pepin says.
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.
«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 Murchison meteorite, a large CM
chondrite that made landfall in Australia in 1969, is now one
of the most studied rocks in the world.
Due to its rarity, Cooke reckons 30 grams
of CM
chondrite is worth about $ 6000.
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.
«If this finding is correct, then it would suggest that
chondrites are not good analogs for the building blocks
of the Earth and other planets.
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 composition
of the matter from which the solar system formed is deduced from that
of stony meteorites called
chondrites and from the composition
of the Sun's atmosphere, supplemented by data acquired from spectral observations
of hot stars and gaseous nebulas.