The telescopes look for the slight
dimming of distant stars that occurs as Kuiper belt objects momentarily pass in front of them.
Not exact matches
The cyclic
dimming of more
distant stars would be too faint for Kepler to measure.
A device called a coronagraph can be built into a telescope to block most
of the photons from a
distant star's glow, allowing the
dim light from a planet to pass into the telescope's sensors and create a glare - free image.
Microlensing works on a much smaller scale: Individual
stars or planets focus the light
of more
distant stars, making the background
star appear to grow brighter and then
dim again.
In the 1990s, observations
of exploding
stars showed that more
distant explosions were
dimmer than existing theories predicted.
The specifics to how Haumea
dimmed the light
of that
distant star would be perfectly explained by a semi-transparent ring with a width
of 70 kilometers (around 43 miles) and a radius
of 2,287 kilometers (1,421 miles).