«Clear evidence of [former] 60Fe
in chondrites was first found in troilite (FeS) and magnetite (Fe3O4).»
This will permit the average terrestrial concentrations of uranium and thorium to be 2 to 4.7 times higher than that observed
in chondrites.
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.
Not exact matches
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.
Radioactive isotopes of elements such as uranium, potassium, and thorium are found
in a class of rocky meteorites known as
chondrites.
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.
Almost on a whim, Piatek paid $ 6000 for the stone — cheap
in the meteorite world — thinking it was nothing more than a regular
chondrite.
It didn't have the heft of a
chondrite, which are typically rich
in dense metals.
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
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.
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.
There is one other LL
chondrite whose orbit is known: the asteroid Itokawa, which the Japanese Hayabusa spacecraft visited
in 2005.
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.
One thing was odd about Chelyabinsk compared to other LL
chondrites: it was shot through with cracks that had filled
in with molten metal.
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?»
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.
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.
Krypton
in today's atmosphere is somewhat heavier than solar krypton, and the krypton embedded
in meteorites known as carbonaceous
chondrites is even heavier than that.
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 say
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 say
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.
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.
In gas with extra carbon or too little oxygen, carbon compounds like carbides and graphite condense out instead of silicates, possibly explaining the origin of carbonaceous
chondrites and suggesting the possibility of carbon planets.
«Carbon planets could form
in much the same way as do certain meteorites
in our solar system, the carbonaceous
chondrites,» said Dr. Marc J. Kuchner of Princeton University, making the report
in Aspen together with Dr. Sara Seager of the Carnegie Institute of Washington.
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 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.
The so - called «Galactic Cosmic Rays» probably come directly from the Sun's pulsar core, and were recorded as a gradient
in cosmic ray exposures of meteorites at the birth of the solar system: iron meteorites > stone meteorites > carbonaceous
chondrites