[meteorite-list] Vesta's Potassium-to-Thorium Ratio Reveals Hot Origins

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Sun, 26 Jul 2015 21:16:47 -0700 (PDT)
Message-ID: <201507270416.t6R4GlQA022307_at_zagami.jpl.nasa.gov>

https://www.psi.edu/news/vestak-th

Vesta's Potassium-to-Thorium Ratio Reveals Hot Origins
Planetary Science Institute
July 22, 2015
 
Tucson, Ariz. -- Studies of materials on the surface of Vesta offer new
evidence that the giant asteroid is the source of howardite, eucrite and
diogenite (HED) basaltic meteorites, supporting current models of solar
system evolution and terrestrial planet formation, a new paper by Planetary
Science Institute researcher Tom Prettyman says.
 
Prettyman, a senior scientist at the Planetary Science Institute, and
co-authors determined the globally averaged concentrations of radioactive
elements potassium (K) and thorium (Th) on Vesta's surface using data
from the Gamma Ray and Neutron Detector (GRaND) instrument aboard NASA's
Dawn spacecraft.
 
PSI Postdoctoral Research Scientist Yuki Yamashita and Senior Scientist
Bob Reedy were coauthors on the paper "Concentrations of Potassium and
Thorium within Vesta's Regolith" that appears in the Icarus Special
Issue on Vesta's Composition.
 
"The K and Th content is important because together these elements provide
constraints on the composition of materials from which Vesta was made
and conditions in the early solar system," Prettyman said. The K/Th
ratio of Vesta is very similar to that of the HED meteorites and distinct
from other basaltic meteorites, which strongly supports connection between
Vesta and the HEDs.
 
The solar system originated from a molecular cloud that collapsed to form
the Sun and a rotating disk of gas and dust from which the planets grew.
Vesta is thought to be a planetary "embryo," a leftover planetary
building block that survived more or less intact to the present day. Because
it underwent magmatic processes, similar to the inner planets, Vesta is
also regarded as "the smallest terrestrial planet."
 
As the gas and dust cooled, elements condensed to form solid compounds.
 Each element has a representative condensation temperature. Volatile
elements evaporate/condense at lower temperatures, whereas refractory
elements condense at higher temperatures.
 
Potassium, a moderately volatile element, would have condensed at relatively
low temperatures - about 700C - to form potassium feldspar. However,
thorium condenses at much higher temperatures, 1300C. After accretion
from the protoplanetary disk, Vesta was heated by the decay of short-lived
radionuclides to the point of large-scale melting.
 
K and Th would likely have remained in constant proportions as Vesta cooled
from its initial melted state to form a layered interior consisting of
an iron-rich core, a mantle composed of iron- and magnesium-rich minerals,
and basaltic crust richer in calcium and aluminum. In this process, K
and Th were almost entirely concentrated in the crust. Thus, the K/Th
ratio of the primordial material that made Vesta is likely very similar
to that of Vesta's crust and regolith as viewed by GRaND.
 
All of the inner planets are depleted in moderately volatile elements,
such as K, and have low K/Th ratios in comparison to the solar photosphere,
which is thought to be representative of the composition of the solar
nebula. Measurements of Vesta's K/Th ratio by GRaND show that this inner
main belt asteroid is also depleted in K relative to Th. In fact, of the
inner solar system bodies for which K/Th has been measured, Vesta is second
only to the moon in K-depletion.
 
"Vesta was probably made early from material that condensed at high
temperature, which limited the accumulation of K," Prettyman said. "However,
the mechanisms for depletion of moderately volatile elements are still
not fully understood."
 
Alternatives for depletion of K on Vesta include degassing of more volatile
elements from high-temperature magmas and disruption and re-accretion
of Vesta following a giant impact, similar to the formation of the Earth-Moon
system. For various reasons, neither of these scenarios is favored.
 
The dearth of moderately volatile elements throughout the inner solar
system remains one of the long-standing, unresolved problems of cosmochemistry.
This paper provides another piece of the puzzle in this complex story
and further evidence that the HED meteorites hail from Vesta.
 
The project was funded by a contract from the NASA Jet Propulsion Laboratory,
which is operated by the California Institute of Technology in Pasadena,
California. The Dawn mission is led by the University of California, Los
Angeles under the auspices of the NASA Discovery Program. GRaND is managed
by the Planetary Science Institute.
Received on Mon 27 Jul 2015 12:16:47 AM PDT