The answer is: yes, just about, maybe.
Astronomers had catalogued over 2 million stars with parallax values.
However many of the values are estimates and some of the angles are very small.
The parallax refers to the apparent change in the star's position, due to Earth's movement around the Sun. This parallax can be used to measure the distance to nearby stars (the closer the star, the larger will its parallax be).
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.
Earth's atmosphere does not limit a telescope's resolving power.
If you mean, using the parallax method, that might be Hipparcos, or Gaia. From Wikipedia, article "Parallax":In 1989, the satellite Hipparcos was launched primarily for obtaining parallaxes and proper motions of nearby stars, increasing the reach of the [parallax] method tenfold. Even so, Hipparcos is only able to measure parallax angles for stars up to about 1,600 light-years away, ... The European Space Agency's Gaia mission, due to launch in 2012 and come online in 2013, will be able to measure parallax angles to an accuracy of 10 microarcseconds, thus mapping nearby stars (and potentially planets) up to a distance of tens of thousands of light-years from earth.
To measure the distance from the earth to the sun, or to any star for that matter astronomers use a form of trigonometry called Parallax (see related Link). Simply put, think of measuring a known distance (the larger the better) and measure the angles to the sun at the same time at each end of that baseline. Using the Angle-Side-Angle formula, (See related link #2) the lengths of the other two sides can be calculated
The stars with the largest parallax angles are typically the closest to Earth. For instance, Proxima Centauri, the closest known star to our solar system, has a parallax angle of about 0.7686 arcseconds. Other nearby stars, like Barnard's Star and Sirius A, also exhibit relatively large parallax angles, allowing astronomers to measure their distances with greater precision. These measurements are crucial for understanding stellar distances and the structure of our galaxy.
Pressumably, they didn't have the high-precision devices required to measure those angles. You must consider that we are talking about extremely small angles - even the closest star has a parallax of less than one arc-second (1/3600 of a degree).
Yes, objects that are farther away than others will exhibit less parallax. Parallax is the apparent change in position of an object when viewed from different perspectives. The closer an object is, the greater its parallax when viewed from different angles.
the stars nearest Earth
The farther the object, the smaller its parallax. In this case, the parallax is about 1/300,000 of an arc-second (and an arc-second is 1/3600 of a degree) - way too small to measure. Perhaps you will eventually find a way to measure smaller parallax angles.
The parallax refers to the apparent change in the star's position, due to Earth's movement around the Sun. This parallax can be used to measure the distance to nearby stars (the closer the star, the larger will its parallax be).
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.
Earth's atmosphere does not limit a telescope's resolving power.
they couldn't measure small angles
If you mean, using the parallax method, that might be Hipparcos, or Gaia. From Wikipedia, article "Parallax":In 1989, the satellite Hipparcos was launched primarily for obtaining parallaxes and proper motions of nearby stars, increasing the reach of the [parallax] method tenfold. Even so, Hipparcos is only able to measure parallax angles for stars up to about 1,600 light-years away, ... The European Space Agency's Gaia mission, due to launch in 2012 and come online in 2013, will be able to measure parallax angles to an accuracy of 10 microarcseconds, thus mapping nearby stars (and potentially planets) up to a distance of tens of thousands of light-years from earth.
To measure the distance from the earth to the sun, or to any star for that matter astronomers use a form of trigonometry called Parallax (see related Link). Simply put, think of measuring a known distance (the larger the better) and measure the angles to the sun at the same time at each end of that baseline. Using the Angle-Side-Angle formula, (See related link #2) the lengths of the other two sides can be calculated
Parallax is the apparent shift in the position of an object when viewed from different angles. In astronomy, parallax is used to measure the distance to stars by observing how their positions change as the Earth orbits the Sun. By measuring the angle of the shift, scientists can calculate the distance to the star using trigonometry.