By precisely
measuring the changes in the brightness and color of these sources as they rotate, we can explore their surface brightness distributions, thus creating rough maps of their cloud cover and temperature distributions.
Not exact matches
They are
measured by the variation
in brightness to the time allowed between each
change, This
measures the distance to objects 10s of millions of light years across.
«Depending on the camera's configuration, we can
measure either the
brightness or color of the emitted light across the bandage or the
change in brightness over time,» Li said.
One method involves
measuring the
changes in a star's
brightness that result from the gravitational effects of a primordial black hole passing between Earth and that star.