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1.
Med J Armed Forces India ; 78(Suppl 1): S319-S322, 2022 Sep.
Artigo em Inglês | MEDLINE | ID: mdl-36147420

RESUMO

An infant presented with recurrent episodes of encephalopathy, responding to nonspecific management of sepsis. High index of suspicion helped uncover underlying error of metabolism.

3.
5.
Science ; 326(5952): 568-72, 2009 Oct 23.
Artigo em Inglês | MEDLINE | ID: mdl-19779151

RESUMO

The search for water on the surface of the anhydrous Moon had remained an unfulfilled quest for 40 years. However, the Moon Mineralogy Mapper (M3) on Chandrayaan-1 has recently detected absorption features near 2.8 to 3.0 micrometers on the surface of the Moon. For silicate bodies, such features are typically attributed to hydroxyl- and/or water-bearing materials. On the Moon, the feature is seen as a widely distributed absorption that appears strongest at cooler high latitudes and at several fresh feldspathic craters. The general lack of correlation of this feature in sunlit M3 data with neutron spectrometer hydrogen abundance data suggests that the formation and retention of hydroxyl and water are ongoing surficial processes. Hydroxyl/water production processes may feed polar cold traps and make the lunar regolith a candidate source of volatiles for human exploration.


Assuntos
Radical Hidroxila , Lua , Água , Meio Ambiente Extraterreno , Minerais , Astronave , Análise Espectral , Luz Solar , Temperatura
6.
Science ; 298(5601): 2182-5, 2002 Dec 13.
Artigo em Inglês | MEDLINE | ID: mdl-12481135

RESUMO

Records of now-extinct short-lived nuclides in meteorites provide information about the formation and evolution of the solar system. We have found excess 10B that we attribute to the decay of short-lived 10Be (half-life 1.5 million years) in hibonite grains from the Murchison meteorite. The grains show no evidence of decay of two other short-lived nuclides-26Al (half-life 700,000 years) and 41Ca (half-life 100,000 years)-that may be present in early solar system solids. One plausible source of the observed 10Be is energetic particle irradiation of material in the solar nebula. An effective irradiation dose of approximately 2 x 10(18) protons per square centimeter with a kinetic energy of >/=10 megaelectronvolts per atomic mass unit can explain our measurements. The presence of 10Be, coupled with the absence of 41Ca and 26Al, may rule out energetic particle irradiation as the primary source of 41Ca and 26Al present in some early solar system solids and strengthens the case of a stellar source for 41Ca and 26Al.

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