Because Proxima Centauri is the closest star to our sun (distance, 4.2 light - years), its angular motion across the sky is relatively fast compared to much more
distant background stars.
Microlensing occurs when a foreground star passes close to our line of sight to a more
distant background star.
Scientists can take advantage of the warping effect by measuring the light of distant stars, looking for a brightening that might be caused by a massive object, such as a planet, that passes between a telescope and
a distant background star.
Not exact matches
Along with the familiar cosmic microwave
background — the afterglow of the big bang — the
distant universe is suffused with an infrared
background, thought to come from galaxies and
stars too faint and far away to see.
So a number of observational projects have taken a different tack, trying to identify small KBOs by monitoring
background stars for sudden dips in brightness that might result from a
distant object crossing the line of sight between the
star and Earth.
Background Astronomers can figure out what
distant stars are made of (in other words, their atomic composition) by seeing what type of light the
star produces.
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.
The only accurate approach to measure the tangential speed of M31 is to observe proper motion of M31's
stars against a
background of
distant galaxies.
The thin, glowing streak slicing across this image cuts a lonely figure, with only a few foreground
stars and galaxies in the
distant background for company.
The image, which shows gas, dust and
stars spread across the sky in a disorderly and irregular jumble, also reveals several other, far more
distant galaxies that appear as fuzzy shapes in the
background.