Catálogo de publicaciones - revistas

<jats:p>A new text confronts how bias tainted efforts to preserve native cultures of the Americas</jats:p>

<jats:p> Highlights from the <jats:italic>Science</jats:italic> family of journals </jats:p>

<jats:p>Editors’ selections from the current scientific literature</jats:p>

<jats:title>A tricky mimicry</jats:title> <jats:p> RNA viruses use dynamic, multifunctional folded elements to hijack host cellular machinery. Bonilla <jats:italic>et al</jats:italic> . used cryo–electron microscopy (cryo-EM) to explore an RNA element from Brome mosaic virus that tricks host cell tyrosine transfer RNA synthetase (TyrRS) into adding a tyrosine to the viral genome’s 3′ end. Visualizing this RNA both in isolation and bound to a cellular TyrRS revealed a bound structure unlike the canonical transfer RNA L-like shape and conformational rearrangements in the RNA upon binding to the TyrRS, which suggests a multistep process of enzyme recognition. This study highlights the power of cryo-EM to illustrate dynamic processes involving small structured RNAs and RNA-protein complexes. —DJ </jats:p>

<jats:title>Measuring the depth of Jupiter’s storms</jats:title> <jats:p> The atmosphere of Jupiter consists of bands of winds rotating at different rates, punctuated by giant storms. The largest storm is the Great Red Spot (GRS), which has persisted for more than a century. It has been unclear whether the storms are confined to a thin layer near the top of the atmosphere or if they extend deep into the planet. Bolton <jats:italic>et al</jats:italic> . used microwave observations from the Juno spacecraft to observe several storms and vortices. They found that the storms extended below the depths at which water and ammonia are expected to condense, implying a connection with the deep atmosphere. Parisi <jats:italic>et al</jats:italic> . analyzed gravity measurements taken while Juno flew over the GRS. They detected a perturbation in the planet’s gravitational field caused by the storm, finding that it was no more than 500 kilometers deep. In combination, these results constrain how Jupiter’s meteorology links to its deep interior. —KTS </jats:p>

<jats:title>Measuring the depth of Jupiter’s storms</jats:title> <jats:p> The atmosphere of Jupiter consists of bands of winds rotating at different rates, punctuated by giant storms. The largest storm is the Great Red Spot (GRS), which has persisted for more than a century. It has been unclear whether the storms are confined to a thin layer near the top of the atmosphere or if they extend deep into the planet. Bolton <jats:italic>et al</jats:italic> . used microwave observations from the Juno spacecraft to observe several storms and vortices. They found that the storms extended below the depths at which water and ammonia are expected to condense, implying a connection with the deep atmosphere. Parisi <jats:italic>et al</jats:italic> . analyzed gravity measurements taken while Juno flew over the GRS. They detected a perturbation in the planet’s gravitational field caused by the storm, finding that it was no more than 500 kilometers deep. In combination, these results constrain how Jupiter’s meteorology links to its deep interior. —KTS </jats:p>