The 'parsec' (3.26 light years) is the distance at which an object exhibits an annual
parallax of 1 arcsecond. Although the whole idea is based in the trigonometric tangent
of angles, we can assume a perfectly linear relationship for such small angles.
-- 0.1 arcsecond ==> 3.26/0.1 = 32.6 light years
-- 0.02 arcsecond ==> 3.26/0.02 = 163 light years
Their magnitude has nothing to do with the question you asked. It may be
relevant to the second part of the question from which you copied only the
first part. Thanks for including all of the given data, though.
stellar parallax
Parallax helps because the bigger the parallax is the closer the star is. Knowing the distance helps to determine the "absolute magnitude" of a star, not just how bright it appears.
Distance (to an object).
I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.
Parallax
Stellar Parallax Astronomers estimate the distance of nearby objects in space by using a method called stellar parallax, or trigonometric parallax. Simply put, they measure a star's apparent movement against the background of more distant stars as Earth revolves around the sun.
The Parallax Method. See the link for more info.
The closer the star, the greater the parallax angle, which is why you can't measure the distance to very distant stars using the parallax method.
stellar parallax
The parallax should get smaller and harder to notice although in astronomy there are techniques used to find the parallax of stars by using the Earth's position around the sun to find the distance of the stars.
Parallax helps because the bigger the parallax is the closer the star is. Knowing the distance helps to determine the "absolute magnitude" of a star, not just how bright it appears.
Distance.
Distance (to an object).
He was on to a brilliant idea about how parallax can be used to estimate some astronomical distances.
for determining distance
I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.
If a certain star displayed a large parallax, i would say its distance is not wide.