To understand where the measured flux from the planet is coming from we need to capture both reflected and thermal components of the light from the planet. This requires broad

Venus as seen by Himawari satellites. A photo with magnified sections to show just how small Venus is in the field of view of the observation satellites. Despite this limitation,

CT models of internal or external growth structures, as well as shell thickness, of individual foraminifera Credit University of Southampton Scientists at the University of Southampton have developed a new

Time series of relative FWHM measurements for all NETS stars with multiple nights of data collected prior to August 2021. We observe a sharp decrease in FWHM in August 2021

β-curves for amorphous carbon (‘C’, green lines, Kimura & Mann 1999), astronomical silicates (“SiO”, solid gold line, Gustafson 1994; and blue lines, Kimura & Mann 1999), and adapted astronomical silicates