[meteorite-list] Angrites hot under the colar
From: Pete Pete <rsvp321_at_meteoritecentral.com>
Date: Fri, 31 Oct 2008 10:15:27 -0400 Message-ID: <BAY141-W44C90151EF16E8F932FE3F8200_at_phx.gbl> Hi, Darren and List, You would think then, that there would be more angrite meteorites found, and chondrules in meteorites would be more rare...? Cheers, Pete > From: cynapse at charter.net > To: meteorite-list at meteoritecentral.com > Date: Fri, 31 Oct 2008 09:30:39 -0500 > Subject: [meteorite-list] Angrites hot under the colar > > http://www.space.com/scienceastronomy/081030-planet-formation.html > > Ancient Meteorites Give Clues to Planet Formation > By SPACE.com staff > > posted: 30 October 2008 > 02:04 pm ET > > Meteorites that are among the oldest rocks ever found have provided new clues > about the conditions that existed at the beginning of the solar system, solving > a longstanding mystery and overturning some accepted ideas about the way planets > form. > > The ancient meteorites, called angrites, still contain magnetic records about > the very early history of planets, like disk drives salvaged from an ancient > computer, new research by MIT planetary scientist Benjamin P. Weiss indicates. > > The results of the study, which was by a grant from the National Science > Foundation's Instrumentation and Facilities Program, are detailed in the Oct. 31 > issue of the journal Science. > > The analysis showed that surprisingly, during the formation of the solar system, > when dust and rubble in a disk around the sun collided and stuck together to > form ever-larger rocks and eventually the planets we know today, even objects > much smaller than planets ? just 100 miles (160 kilometers) across or so ? were > large enough to melt almost completely. > > This total melting of the planet-forming chunks of rock, called planetesimals, > caused their constituents to separate out, with lighter materials including > silicates floating to the surface and eventually forming a crust, while heavier > iron-rich material sank down to the core, where it began swirling around to > produce a magnetic dynamo. The researchers were able to study traces of the > magnetic fields produced by that dynamo, now recorded in the meteorites that > fell to Earth. > > "The magnetism in meteorites has been a longstanding mystery," Weiss said, and > the realization that such small bodies could have melted and formed magnetic > dynamos is a major step toward solving that riddle. > > Until relatively recently, it was commonly thought that the planetesimals ? > similar to the asteroids seen in the solar system today ? that came together to > build planets were "just homogenous, unmelted rocky material, with no > large-scale structure," Weiss said. "Now we're realizing that many of the things > that were forming planets were mini-planets themselves, with crusts and mantles > and cores." > > That could change theorists' picture of how the planets themselves took shape. > > If the smaller bodies were already molten as they slammed together to build up > larger planet-sized bodies, that could "significantly change our understanding" > of the processes that took place in the early years of the nascent planets, as > their internal structures were forming, Weiss said. This could have implications > for how different minerals are distributed in the Earth's crust, mantle and core > today, for example. > > "Events happened surprisingly fast at the beginning of the solar system," Weiss > said. Some of the angrite meteorites in this study formed just 3 million years > after the birth of the solar system itself, 4,568 million years ago, and show > signs that their parent body had a magnetic field that was 20 to 40 percent as > strong as Earth's today. > > "We are used to thinking of dynamo magnetic fields in rocky bodies as uncommon > phenomena today," Weiss said. "But it may be that short-lived planetesimal > dynamos were widespread in the early solar system." > > > > http://sciencenow.sciencemag.org/cgi/content/full/2008/1030/2 > > First Planets Lived Fast and Died Young > > By Phil Berardelli > ScienceNOW Daily News > 30 October 2008 > Surprising findings from some of the oldest known meteorites suggest that our > solar system was once chock-full of miniature planets, complete with metallic > cores and rocky crusts. The findings could force a rethinking of how the solar > system and its constituent bodies evolved. > > Some 4.568 billion years ago, our sun and solar system condensed out of a > primordial cloud of dust and gas. Within about 3 million years, small, rocky > objects called planetesimals were circulating in the nascent solar system. > Fragments of these planetesimals remain today as meteorites called achondrites, > which scientists have pored over for clues to how planets formed. Oddly, the > meteorites are magnetic, which is strange because the planetesimals were > supposed to be just large agglomerations of rubble. > > A U.S.-Canadian team took a new approach to the problem, testing samples of > three well-preserved achondrite meteorites with an extremely sensitive > magnetometer. What they discovered stunned them: The meteorites showed evidence > of ancient magnetic fields similar to those of rocks formed on Earth within the > planet's magnetic field. In other words, the team reports this week in Science, > the 4.565-billion-year-old meteorites once were part of bodies that were either > big enough or hot enough to produce central, molten, metallic cores. > > "The meteorites, therefore, are essentially magnetic recording tapes," says > planetary scientist and lead author Benjamin Weiss of the Massachusetts > Institute of Technology in Cambridge. The magnetic fields that they recorded > were probably generated by molten metal swirling around inside the planet's core > like a giant, rotating dynamo, as happens on Earth. Although most asteroids now > are rocky through and through, the new findings suggest that back at the > beginning of the solar system even planetesimals could melt at their cores and > retain a rocky crust. These bodies could be as small as 160 kilometers in > diameter, the research suggests. The planetesimals, which eventually merged to > form the rocky planets, were more planetlike than previously thought, with cores > that must have formed and melted within just a few million years of the > formation of the solar system, Weiss says. > > The paper "makes a good case," says planetary scientist David Stevenson of the > California Institute of Technology in Pasadena. Although dynamos are thought to > require large planetary cores, it's possible that the > > > > for those with access to _Science_ full text: > > http://www.sciencemag.org/cgi/content/abstract/322/5902/713 > > > and here's a related PDF: > > http://www.lpi.usra.edu/meetings/lpsc2008/pdf/2143.pdf > ______________________________________________ > http://www.meteoritecentral.com > Meteorite-list mailing list > Meteorite-list at meteoritecentral.com > http://six.pairlist.net/mailman/listinfo/meteorite-list _________________________________________________________________ Received on Fri 31 Oct 2008 10:15:27 AM PDT |
StumbleUpon del.icio.us Yahoo MyWeb |