Deuterium-enriched water ties planet-forming disks to comets and protostars.

Water is a fundamental molecule in the star and planet formation process, essential for catalysing the growth of solid material and the formation of planetesimals within disks. However, the water snowline and the HDO:HO ratio within proto-planetary disks have not been well characterized because water only sublimates at roughly 160 K (ref. ), meaning that most water is frozen out onto dust grains and that the water snowline radii are less than 10 AU (astronomical units).

Robust nuclear lamina-based cell classification of aging and senescent cells.

Changes in the shape of the nuclear lamina are exhibited in senescent cells, as well as in cells expressing mutations in lamina genes. To identify cells with defects in the nuclear lamina we developed an imaging method that quantifies the intensity and curvature of the nuclear lamina. We show that this method accurately describes changes in the nuclear lamina.