<p>No, the telescope doesn't measure the parallax. A sextant or any other angle measuring device fit on the telescope does.</p>

<p>And, we don't(can't) directly measure the parallax angle. Instead, we just track the position of the star/object throughout the year. A little bit of spherical astronomy math shows us that the path of a star in the celestial sphere defined by a fixed reference through the year is an ellipse around it's mean postion, called the <em>parallactic ellipse</em></p>

<p><img src="https://i.sstatic.net/vlESX.jpg" alt="parallactic ellipse"></p>

<p><a href="http://star-www.st-and.ac.uk/~fv/webnotes/chapt14.htm" rel="noreferrer">Here</a> is a link which does the rough math involved.</p>

<p>The semi-major axis of this ellipse is equal to the parllax angle P, while the semi-minor axis is equal to P*sin(b), where b is the stars ecliptic latitude.</p>

<p><strong>EXTRA NOTE:</strong> These parallactic ellipses are often rotated and parameters modified as the abberational ellipse is superposed on it. In practice, things get nigh complicated.</p>

CC BY-SA 3.0
2014-01-06T17:42:32.497Z
Perhaps it's worth adding that the mean position is usually not fixed, but (for single stars) moves (nearly) on a line. This motion is called *proper motion* and measured from the same type of data (stellar positions over several epochs) as the parallax.
Walter
CC BY-SA 3.0
2014-01-06T00:03:56.600Z
2014-01-06T00:03:56.600Z
Cheeku
<p>In addition: It's often better to measure the angular distance to reference stars, instead of absolute angles, because those angles can be measured with much higher accuracy.</p>

CC BY-SA 3.0
2014-01-06T15:10:10.847Z
Very true. That is what I meant by "celestial sphere" fixed with some reference(as in the reference stars) :)
Cheeku
CC BY-SA 3.0
2014-01-06T20:18:20.190Z
@Cheeku As you already indicated in your answer, things get hugely more complex, when improving accuracy or looking to more distant stars in the order of 10s of thousands of lightyears. Everything is in motion to each other, including gravitational aberration, even by bodies within our solar system. The Gaia people are struggling with (and are defining) a reference system taking all those effects into account.
Gerald
CC BY-SA 3.0
2014-01-06T06:20:12.200Z
2014-01-06T06:20:12.200Z
Gerald
<p>I know how stars' distances are measured by using parallax, but I want to know how the actual telescope measures the parallax angle. Any helpful links/ explanations are needed.</p>

<telescope><parallax><angular-resolution>
How does a telescope measure parallax angle?
anna 1234
# How does a telescope measure parallax angle?

(Asked by: username_0 on 2014-01-05)

I know how stars' distances are measured by using parallax, but I want to know how the actual telescope measures the parallax angle. Any helpful links/ explanations are needed.

**Tags:** telescope, parallax, angular-resolution


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## 2 answers

### Answer by username_1 on 2014-01-06. Score: 8

No, the telescope doesn't measure the parallax. A sextant or any other angle measuring device fit on the telescope does.

And, we don't(can't) directly measure the parallax angle. Instead, we just track the position of the star/object throughout the year. A little bit of spherical astronomy math shows us that the path of a star in the celestial sphere defined by a fixed reference through the year is an ellipse around it's mean postion, called the *parallactic ellipse*

![parallactic ellipse](https://i.sstatic.net/vlESX.jpg)

[Here](http://star-www.st-and.ac.uk/~fv/webnotes/chapt14.htm) is a link which does the rough math involved.

The semi-major axis of this ellipse is equal to the parllax angle P, while the semi-minor axis is equal to P\*sin(b), where b is the stars ecliptic latitude.

**EXTRA NOTE:** These parallactic ellipses are often rotated and parameters modified as the abberational ellipse is superposed on it. In practice, things get nigh complicated.

> **Comments:**
> **username_2**: Perhaps it's worth adding that the mean position is usually not fixed, but (for single stars) moves (nearly) on a line. This motion is called *proper motion* and measured from the same type of data (stellar positions over several epochs) as the parallax.  

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### Answer by username_3 on 2014-01-06. Score: 3

In addition: It's often better to measure the angular distance to reference stars, instead of absolute angles, because those angles can be measured with much higher accuracy.

> **Comments:**
> **username_1**: Very true. That is what I meant by "celestial sphere" fixed with some reference(as in the reference stars) :)  
> **username_3**: @username_1 As you already indicated in your answer, things get hugely more complex, when improving accuracy or looking to more distant stars in the order of 10s of thousands of lightyears. Everything is in motion to each other, including gravitational aberration, even by bodies within our solar system. The Gaia people are struggling with (and are defining) a reference system taking all those effects into account.  

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