The percentages denote the amount of
nebular light passing through the disk.
The right - hand image is the same, but with contours denoting levels of increasing attenuation of the background
nebular light toward the central star.
Not exact matches
Based on measurements of Jupiter and the solar wind, which are thought to preserve the hydrogen isotopic ratio of the protosolar nebula, scientists think
nebular water had an extremely
light hydrogen isotopic signature — much closer to what the Baffin Island lavas suggest about the deep mantle's water.
These star - formation rate estimators include the ultraviolet
light that is emitted from young stars, the infrared
light that shows how much of the ultraviolet
light was absorbed by dust, and the
nebular emission lines that are caused by young stars making the clouds of gas around them glow and radiate.
This study makes the first direct comparison between the optical emission line and the ultraviolet and infrared tracers of star formation and indicates that, despite the underlying uncertainties, astronomers can trust the
nebular emission lines as robust indicators of the star - formation rate and the amount of
light that is obscured by dust in distant galaxies.
Nguyen sets a panorama of
nebular expanse, slippery time, and infinite spectral
light that could be perceived only in the immeasurable depths of a dream void or through interstellar outer space.