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The compositions of the first solar system solids were shaped by nonequilibrium condensation and evaporation., Equilibrium condensation of solar gas is often invoked to explain the abundance of refractory elements in planets and meteorites. This is partly motivated, by the observation that the depletions in both the least and most refractory rare earth elements (REEs) in meteoritic group II calcium-aluminum–rich inclusions (CAIs) can be reproduced by thermodynamic models of solar nebula condensation. We measured the isotopic compositions of Ce, Nd, Sm, Eu, Gd, Dy, Er, and Yb in eight CAIs to test this scenario. Contrary to expectation for equilibrium condensation, we find light isotope enrichment for the most refractory REEs and more subdued isotopic variations for the least refractory REEs. This suggests that group II CAIs formed by a two-stage process involving fast evaporation of preexisting materials, followed by near-equilibrium recondensation. The calculated time scales are consistent with heating in events akin to FU Orionis– or EX Lupi–type outbursts of eruptive pre–main-sequence stars.

著者人数: 75名, 資料番号: SA1003700000

We have previously used single nucleotide polymorphisms to detect an association of basal cell carcinoma (BCC) in Caucasian Americans and Danes with the genome region 19q13.2-3, which contains several genes involved in the nucleotide excision repair of DNA. In this exploratory paper we have extended the data and used them in a chromosomal scan. The results indicate the presence of a gene variation modulating the risk of developing BSS in a submegabase region including and surrounding the gene RAI. Specifically, persons that are homozygous for the haplotype RAI intron 1(A) RAI exon 6(A) appear at increased risk for BCC. In addition, we have looked for possible synergisms between all pairs of markers. We find that a marker in GLTSCR1, presumably separated from RAI by several million bases, supplements the most significant marker in RAI in separating cases from controls, which may suggest the presence of an independent, risk-modulating variation in this second gene region.

One form of nucleotide excision repair (NER) is known to be functionally coupled to transcription, but the nature of this functional link in Escherichia coli is still unclear. Here we have employed the isolated membrane-associated nucleoids from E.coli to examine this issue. We show that the isolated nucleoid fraction is capable of excision of UV-induced pyrimidine dimers when reconstituted with a cytoplasmic fraction resolved by sucrose gradient fractionation. This excision activity by UvrABC is sensitive to rifampicin and is dependent on transcription. By using crosslinking and immunoprecipitation, the damage recognition protein, UvrA, was found to be specifically associated with the RNA polymerase beta subunit on the chromosomal DNA independent of DNA damage. It suggests that at least in one of the NER pathways the search for damage may be directly linked to RNA polymerase. In addition, the role of transcription in the unfolding of the nucleoid structure to allow repair enzymes to gain access to the damaged DNA is described. This study provides insight into the understanding of the transcription-repair coupling in vivo.

Oxygen isotopic variations across the outer margins and Wark–Lovering (WL) rims of a diverse suite of six coarse-grained Types A and B refractory inclusions from both oxidized and reduced CV3 chondrites suggest that CAIs originated from a 16 O-rich protosolar gas reservoir and were later exposed to both relatively 17,18 O-rich and 16 O-rich reservoirs. The O-isotope profiles of CAIs can be explained by changes in the composition of gas near the protoSun or the migration of CAIs through a heterogeneous nebula. Variability within the inclusion interiors appears to have been set prior to WL rim growth. Modeling the isotopic zoning profiles as diffusion gradients between inclusion interiors and edges establishes a range of permissible time–temperature combinations for their exposure in the nebula. At mean temperatures of 1400 K, models that match the isotope gradients in the inclusions yield timescales ranging from 5 × 10 3 to 3 × 10 5 years. Assuming CAIs originated with a relatively 16 O-rich (protosolar) isotopic composition, differences among the melilite interiors and the isotopic gradients in their margins imply the existence of a number of isotopically distinct reservoirs. Evidence at the edges of some CAIs for subsequent isotopic exchange may relate to the beginning of rim formation. In the WL rim layers surrounding the interiors, spinel is relatively 16 O-rich but subtly distinct among different CAIs. Melilite is often relatively 16 O-poor, but rare relatively 16 O-rich grains also exist. Pyroxene generally exhibits intermediate O-isotope compositions and isotopic zoning. Olivine in both WL and accretionary rims, when present, is isotopically heterogeneous. The extreme isotopic heterogeneity among and within individual WL rim layers and in particular, the observed trends of outward 16 O-enrichments, suggest that rims surrounding CAIs contained in CV3 chondrites, like the inclusions themselves, formed from a number of isotopically distinct gas reservoirs. Collectively, these results support numerical protoplanetary disk models in which CAIs were transported between several distinct nebular reservoirs multiple times prior to accretion onto a parent body.

At least two endonucleolytic activities that preferentially incise ultraviolet (UV)-irradiated DNA exist in extracts of E. coli . These two activities can be separated by phosphocellulose chromatographic fractionation. The subject of this paper is one of these activities, which elutes from phosphocellulose with 0.25 M potassium phosphate, pH 7.5. This endonucleolytic activity specific for UV-irradiated DNA is absent from partially purified extracts of uvrA and uvrB mutants, which are defective in excision of pyrimidine dimers, but is present in normal amounts in the uvrC excision-defective mutant. The enzyme binds very tightly and specifically to UV-irradiated DNA. Binding can be prevented by prior treatment of the irradiated DNA with photoreactivating enzyme. This binding activity is absent in uvrA and uvrB mutants, but present in uvrC and uvrD mutants.

The incorporation of U-C14-L-phenylalanine prepared from poiy-L- phenylaianine from Escherichia coli into acidinsoluble material and poly-L- phenylaianine following ultraviolet irradiation of poiyuridylic acid was examined. Irradiation of the polyuridylic acid with doses of ultraviolet light from 24 to 72 x 104 ergs/mm2 resulted in a marked depression in C14- phenyiaianine incorporation and was accompanied by an increase in C14- serine uptake into both acid-soluble material as well as polyphenylaianine.