Publications by authors named "J F Isa"

Silica polymorphs occur under various pressures and temperature conditions, and their characteristics can be used to better understand the complex metamorphic history of planetary materials. Here, we conducted isothermal heating experiments of silica polymorphs in basaltic eucrites to assess their formation and stability. We revealed that each silica polymorph exhibits different metamorphic responses: (1) Quartz recrystallizes into cristobalite when heated at ≥ 1040 °C.

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Article Synopsis
  • Polycyclic aromatic hydrocarbons (PAHs) make up about 20% of carbon in the interstellar medium and can form under various conditions, including in hot circumstellar environments and cold interstellar clouds.
  • Isotopic analysis of PAHs from asteroid Ryugu and meteorite Murchison shows that some PAHs, like naphthalene, fluoranthene, and pyrene, have higher carbon isotopic values than expected, indicating they likely formed in the interstellar medium rather than in hot environments.
  • In contrast, the PAHs phenanthrene and anthracene from Ryugu display isotopic values that suggest they were formed through higher-temperature reactions.
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Amino acids in carbonaceous chondrites may have seeded the origin of life on Earth and possibly elsewhere. Recently, the return samples from a C-type asteroid Ryugu were found to contain amino acids with a similar distribution to Ivuna-type CI chondrites, suggesting the potential of amino acid abundances as molecular descriptors of parent body geochemistry. However, the chemical mechanisms responsible for the amino acid distributions remain to be elucidated particularly at low temperatures (<50°C).

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Objective: Pregnancy-associated breast cancer (PABC) is a rare cancer. This study aimed to determine the survival probabilities and prognostic factors in patients with PABC.

Methods: A retrospective cohort study was conducted in two tertiary care hospitals in Kota Bharu.

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The Hayabusa2 spacecraft collected samples from the surface of the carbonaceous near-Earth asteroid (162173) Ryugu and brought them to Earth. The samples were expected to contain organic molecules, which record processes that occurred in the early Solar System. We analyzed organic molecules extracted from the Ryugu surface samples.

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