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1.
Science ; 311(5766): 1453-5, 2006 Mar 10.
Article in English | MEDLINE | ID: mdl-16456037

ABSTRACT

We report the direct detection of solid water ice deposits exposed on the surface of comet 9P/Tempel 1, as observed by the Deep Impact mission. Three anomalously colored areas are shown to include water ice on the basis of their near-infrared spectra, which include diagnostic water ice absorptions at wavelengths of 1.5 and 2.0 micrometers. These absorptions are well modeled as a mixture of nearby non-ice regions and 3 to 6% water ice particles 10 to 50 micrometers in diameter. These particle sizes are larger than those ejected during the impact experiment, which suggests that the surface deposits are loose aggregates. The total area of exposed water ice is substantially less than that required to support the observed ambient outgassing from the comet, which likely has additional source regions below the surface.


Subject(s)
Ice/analysis , Meteoroids , Spectrophotometry, Infrared
2.
Science ; 310(5746): 258-64, 2005 Oct 14.
Article in English | MEDLINE | ID: mdl-16150978

ABSTRACT

Deep Impact collided with comet Tempel 1, excavating a crater controlled by gravity. The comet's outer layer is composed of 1- to 100-micrometer fine particles with negligible strength (<65 pascals). Local gravitational field and average nucleus density (600 kilograms per cubic meter) are estimated from ejecta fallback. Initial ejecta were hot (>1000 kelvins). A large increase in organic material occurred during and after the event, with smaller changes in carbon dioxide relative to water. On approach, the spacecraft observed frequent natural outbursts, a mean radius of 3.0 +/- 0.1 kilometers, smooth and rough terrain, scarps, and impact craters. A thermal map indicates a surface in equilibrium with sunlight.


Subject(s)
Meteoroids , Jupiter , Organic Chemicals/analysis , Spectrum Analysis
4.
Genetics ; 143(2): 627-35, 1996 Jun.
Article in English | MEDLINE | ID: mdl-8725214

ABSTRACT

A new mutation, bglJ4, has been characterized that results in the expression of the silent bgl operon. The bgl operon encodes proteins necessary for the transport and utilization of the aromatic beta-glucosides arbutin and salicin. A variety of mutations activate the operon and result in a Bgl+ phenotype. Activating mutations are located upstream of the bgl promoter and in genes located elsewhere on the chromosome. Mutations outside of the bgl operon occur in the genes encoding DNA gyrase and in the gene encoding the nucleoid associated protein H-NS. The mutation described here, bglJ4, has been mapped to a new locus at min 99 on the Escherichia coli K-12 genetic map. The putative protein encoded by the bglJ gene has homolgy to a family of transcriptional activators. Evidence is presented that increased expression of the bglJ product is needed for activation of the bgl operon.


Subject(s)
Escherichia coli Proteins , Escherichia coli/genetics , Genes, Bacterial , Trans-Activators/genetics , Amino Acid Sequence , Base Sequence , Chromosome Mapping , Molecular Sequence Data , Mutation , Operon
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