Is parallax a “technique to measure the star distances” or a “tiny shift in star's position”?












13












$begingroup$


I am not completely sure whether the Parallax is a "technique to measure the star distances" or a "tiny shift in star's position"?



The a book says two points about Parallax:




  • Astronomers have developed a variety of clever techniques for measuring the vast distances to stars, one is called Parallax.


  • Astronomers can measure a star's position once and then again 6 months later and calculate the apparent change in position. This tiny shift in stars position is called its parallax.



Apart from the book source, whatis.techtarget.com defines Parallax as the way an object’s position or direction seems to change depending on viewing angle.










share|improve this question











$endgroup$








  • 6




    $begingroup$
    You are presenting this as if it's one or the other, but not both. The answer is that both are true. Annual parallax is a tiny shift that varies inversely with distance. This means that the observed shift can be used as a way to measure distance.
    $endgroup$
    – David Hammen
    Nov 29 '18 at 8:11






  • 1




    $begingroup$
    Parallax is something you can see on earth. Eg, if you're traveling by vehicle and look out the window, the nearby trees appear to pass very quickly, the houses further away appear to pass slowly, and the distant mountains more slowly still. Parallax scrolling is used in video games to give the illusion of distance: en.wikipedia.org/wiki/Parallax_scrolling#/media/… I think the idea in astronomy is that as the earth moves, the things that appear most stationary must be farthest away, like the distant mountains on Earth.
    $endgroup$
    – Nathan Long
    Nov 29 '18 at 19:14












  • $begingroup$
    BTW, welcome to Astronomy.SE!
    $endgroup$
    – David Hammen
    Nov 30 '18 at 5:56










  • $begingroup$
    @David, thanks a bunch! :-)
    $endgroup$
    – Ahmed
    Nov 30 '18 at 9:19
















13












$begingroup$


I am not completely sure whether the Parallax is a "technique to measure the star distances" or a "tiny shift in star's position"?



The a book says two points about Parallax:




  • Astronomers have developed a variety of clever techniques for measuring the vast distances to stars, one is called Parallax.


  • Astronomers can measure a star's position once and then again 6 months later and calculate the apparent change in position. This tiny shift in stars position is called its parallax.



Apart from the book source, whatis.techtarget.com defines Parallax as the way an object’s position or direction seems to change depending on viewing angle.










share|improve this question











$endgroup$








  • 6




    $begingroup$
    You are presenting this as if it's one or the other, but not both. The answer is that both are true. Annual parallax is a tiny shift that varies inversely with distance. This means that the observed shift can be used as a way to measure distance.
    $endgroup$
    – David Hammen
    Nov 29 '18 at 8:11






  • 1




    $begingroup$
    Parallax is something you can see on earth. Eg, if you're traveling by vehicle and look out the window, the nearby trees appear to pass very quickly, the houses further away appear to pass slowly, and the distant mountains more slowly still. Parallax scrolling is used in video games to give the illusion of distance: en.wikipedia.org/wiki/Parallax_scrolling#/media/… I think the idea in astronomy is that as the earth moves, the things that appear most stationary must be farthest away, like the distant mountains on Earth.
    $endgroup$
    – Nathan Long
    Nov 29 '18 at 19:14












  • $begingroup$
    BTW, welcome to Astronomy.SE!
    $endgroup$
    – David Hammen
    Nov 30 '18 at 5:56










  • $begingroup$
    @David, thanks a bunch! :-)
    $endgroup$
    – Ahmed
    Nov 30 '18 at 9:19














13












13








13





$begingroup$


I am not completely sure whether the Parallax is a "technique to measure the star distances" or a "tiny shift in star's position"?



The a book says two points about Parallax:




  • Astronomers have developed a variety of clever techniques for measuring the vast distances to stars, one is called Parallax.


  • Astronomers can measure a star's position once and then again 6 months later and calculate the apparent change in position. This tiny shift in stars position is called its parallax.



Apart from the book source, whatis.techtarget.com defines Parallax as the way an object’s position or direction seems to change depending on viewing angle.










share|improve this question











$endgroup$




I am not completely sure whether the Parallax is a "technique to measure the star distances" or a "tiny shift in star's position"?



The a book says two points about Parallax:




  • Astronomers have developed a variety of clever techniques for measuring the vast distances to stars, one is called Parallax.


  • Astronomers can measure a star's position once and then again 6 months later and calculate the apparent change in position. This tiny shift in stars position is called its parallax.



Apart from the book source, whatis.techtarget.com defines Parallax as the way an object’s position or direction seems to change depending on viewing angle.







star distances






share|improve this question















share|improve this question













share|improve this question




share|improve this question








edited Nov 29 '18 at 21:16









Glorfindel

1,9331924




1,9331924










asked Nov 29 '18 at 7:27









AhmedAhmed

16816




16816








  • 6




    $begingroup$
    You are presenting this as if it's one or the other, but not both. The answer is that both are true. Annual parallax is a tiny shift that varies inversely with distance. This means that the observed shift can be used as a way to measure distance.
    $endgroup$
    – David Hammen
    Nov 29 '18 at 8:11






  • 1




    $begingroup$
    Parallax is something you can see on earth. Eg, if you're traveling by vehicle and look out the window, the nearby trees appear to pass very quickly, the houses further away appear to pass slowly, and the distant mountains more slowly still. Parallax scrolling is used in video games to give the illusion of distance: en.wikipedia.org/wiki/Parallax_scrolling#/media/… I think the idea in astronomy is that as the earth moves, the things that appear most stationary must be farthest away, like the distant mountains on Earth.
    $endgroup$
    – Nathan Long
    Nov 29 '18 at 19:14












  • $begingroup$
    BTW, welcome to Astronomy.SE!
    $endgroup$
    – David Hammen
    Nov 30 '18 at 5:56










  • $begingroup$
    @David, thanks a bunch! :-)
    $endgroup$
    – Ahmed
    Nov 30 '18 at 9:19














  • 6




    $begingroup$
    You are presenting this as if it's one or the other, but not both. The answer is that both are true. Annual parallax is a tiny shift that varies inversely with distance. This means that the observed shift can be used as a way to measure distance.
    $endgroup$
    – David Hammen
    Nov 29 '18 at 8:11






  • 1




    $begingroup$
    Parallax is something you can see on earth. Eg, if you're traveling by vehicle and look out the window, the nearby trees appear to pass very quickly, the houses further away appear to pass slowly, and the distant mountains more slowly still. Parallax scrolling is used in video games to give the illusion of distance: en.wikipedia.org/wiki/Parallax_scrolling#/media/… I think the idea in astronomy is that as the earth moves, the things that appear most stationary must be farthest away, like the distant mountains on Earth.
    $endgroup$
    – Nathan Long
    Nov 29 '18 at 19:14












  • $begingroup$
    BTW, welcome to Astronomy.SE!
    $endgroup$
    – David Hammen
    Nov 30 '18 at 5:56










  • $begingroup$
    @David, thanks a bunch! :-)
    $endgroup$
    – Ahmed
    Nov 30 '18 at 9:19








6




6




$begingroup$
You are presenting this as if it's one or the other, but not both. The answer is that both are true. Annual parallax is a tiny shift that varies inversely with distance. This means that the observed shift can be used as a way to measure distance.
$endgroup$
– David Hammen
Nov 29 '18 at 8:11




$begingroup$
You are presenting this as if it's one or the other, but not both. The answer is that both are true. Annual parallax is a tiny shift that varies inversely with distance. This means that the observed shift can be used as a way to measure distance.
$endgroup$
– David Hammen
Nov 29 '18 at 8:11




1




1




$begingroup$
Parallax is something you can see on earth. Eg, if you're traveling by vehicle and look out the window, the nearby trees appear to pass very quickly, the houses further away appear to pass slowly, and the distant mountains more slowly still. Parallax scrolling is used in video games to give the illusion of distance: en.wikipedia.org/wiki/Parallax_scrolling#/media/… I think the idea in astronomy is that as the earth moves, the things that appear most stationary must be farthest away, like the distant mountains on Earth.
$endgroup$
– Nathan Long
Nov 29 '18 at 19:14






$begingroup$
Parallax is something you can see on earth. Eg, if you're traveling by vehicle and look out the window, the nearby trees appear to pass very quickly, the houses further away appear to pass slowly, and the distant mountains more slowly still. Parallax scrolling is used in video games to give the illusion of distance: en.wikipedia.org/wiki/Parallax_scrolling#/media/… I think the idea in astronomy is that as the earth moves, the things that appear most stationary must be farthest away, like the distant mountains on Earth.
$endgroup$
– Nathan Long
Nov 29 '18 at 19:14














$begingroup$
BTW, welcome to Astronomy.SE!
$endgroup$
– David Hammen
Nov 30 '18 at 5:56




$begingroup$
BTW, welcome to Astronomy.SE!
$endgroup$
– David Hammen
Nov 30 '18 at 5:56












$begingroup$
@David, thanks a bunch! :-)
$endgroup$
– Ahmed
Nov 30 '18 at 9:19




$begingroup$
@David, thanks a bunch! :-)
$endgroup$
– Ahmed
Nov 30 '18 at 9:19










4 Answers
4






active

oldest

votes


















19












$begingroup$

It is both - a small shift of the position of a star on the sky as we see it, and a means of estimating the distance to the star.



The apparent position (with respect to very distant objects like quasars) changes because our viewing point changes as the Earth moves around the Sun in its orbit. The amount by which the position changes is inversely proportional to is distance.






share|improve this answer









$endgroup$





















    8












    $begingroup$

    It's all of that! If you look at an object with just your left, and then with just your right eye, you'll see its position slightly differently. The angle that your lines of sight form (from one eye to the object, and from the other), divided by two, is called "parallax angle". With trigonometry, one can calculate the distance to the object by knowing this angle and the distance between your eyes. Instead of the eyes, astronomers typically use the distance from the Earth to the Sun, by observing when the Earth is at diametrically opposite points during its orbit (approximately).
    See: https://en.m.wikipedia.org/wiki/Parallax under "distance measurement" for more details.






    share|improve this answer









    $endgroup$





















      4












      $begingroup$

      It is both



      But, specifically, the small motion is what we observe of the star at opposing points of Earth's orbit around the Sun. Then, because we know the radius of that orbit (1 AU) we can use the parallax, the observed small angular change in the location of a star against a distant background between opposite sides of the Earth's orbit, to make a parallax estimate of the star's distance, which is the inverse of small angular change (in radians) in units of parsecs.



      enter image description here






      share|improve this answer









      $endgroup$





















        3












        $begingroup$

        It is really just imprecise language in the first example.



        Parallax is the change in apparent position. To be formally correct, you measure or observe parallax and use it, with trigonometry, to determine the distance.



        You can call this the parallax method of distance measurement. What you have found is that people often omit the word "method".



        More precise language would be either:




        Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. One uses an effect called parallax.



        Astronomers have developed a variety of clever techniques for measuring the vast distances to stars, one is by measuring parallax.



        Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. The parallax method is one of them.




        A similar issue comes up with "Doppler".






        share|improve this answer









        $endgroup$













          Your Answer





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          4 Answers
          4






          active

          oldest

          votes








          4 Answers
          4






          active

          oldest

          votes









          active

          oldest

          votes






          active

          oldest

          votes









          19












          $begingroup$

          It is both - a small shift of the position of a star on the sky as we see it, and a means of estimating the distance to the star.



          The apparent position (with respect to very distant objects like quasars) changes because our viewing point changes as the Earth moves around the Sun in its orbit. The amount by which the position changes is inversely proportional to is distance.






          share|improve this answer









          $endgroup$


















            19












            $begingroup$

            It is both - a small shift of the position of a star on the sky as we see it, and a means of estimating the distance to the star.



            The apparent position (with respect to very distant objects like quasars) changes because our viewing point changes as the Earth moves around the Sun in its orbit. The amount by which the position changes is inversely proportional to is distance.






            share|improve this answer









            $endgroup$
















              19












              19








              19





              $begingroup$

              It is both - a small shift of the position of a star on the sky as we see it, and a means of estimating the distance to the star.



              The apparent position (with respect to very distant objects like quasars) changes because our viewing point changes as the Earth moves around the Sun in its orbit. The amount by which the position changes is inversely proportional to is distance.






              share|improve this answer









              $endgroup$



              It is both - a small shift of the position of a star on the sky as we see it, and a means of estimating the distance to the star.



              The apparent position (with respect to very distant objects like quasars) changes because our viewing point changes as the Earth moves around the Sun in its orbit. The amount by which the position changes is inversely proportional to is distance.







              share|improve this answer












              share|improve this answer



              share|improve this answer










              answered Nov 29 '18 at 7:48









              Rob JeffriesRob Jeffries

              52k4103160




              52k4103160























                  8












                  $begingroup$

                  It's all of that! If you look at an object with just your left, and then with just your right eye, you'll see its position slightly differently. The angle that your lines of sight form (from one eye to the object, and from the other), divided by two, is called "parallax angle". With trigonometry, one can calculate the distance to the object by knowing this angle and the distance between your eyes. Instead of the eyes, astronomers typically use the distance from the Earth to the Sun, by observing when the Earth is at diametrically opposite points during its orbit (approximately).
                  See: https://en.m.wikipedia.org/wiki/Parallax under "distance measurement" for more details.






                  share|improve this answer









                  $endgroup$


















                    8












                    $begingroup$

                    It's all of that! If you look at an object with just your left, and then with just your right eye, you'll see its position slightly differently. The angle that your lines of sight form (from one eye to the object, and from the other), divided by two, is called "parallax angle". With trigonometry, one can calculate the distance to the object by knowing this angle and the distance between your eyes. Instead of the eyes, astronomers typically use the distance from the Earth to the Sun, by observing when the Earth is at diametrically opposite points during its orbit (approximately).
                    See: https://en.m.wikipedia.org/wiki/Parallax under "distance measurement" for more details.






                    share|improve this answer









                    $endgroup$
















                      8












                      8








                      8





                      $begingroup$

                      It's all of that! If you look at an object with just your left, and then with just your right eye, you'll see its position slightly differently. The angle that your lines of sight form (from one eye to the object, and from the other), divided by two, is called "parallax angle". With trigonometry, one can calculate the distance to the object by knowing this angle and the distance between your eyes. Instead of the eyes, astronomers typically use the distance from the Earth to the Sun, by observing when the Earth is at diametrically opposite points during its orbit (approximately).
                      See: https://en.m.wikipedia.org/wiki/Parallax under "distance measurement" for more details.






                      share|improve this answer









                      $endgroup$



                      It's all of that! If you look at an object with just your left, and then with just your right eye, you'll see its position slightly differently. The angle that your lines of sight form (from one eye to the object, and from the other), divided by two, is called "parallax angle". With trigonometry, one can calculate the distance to the object by knowing this angle and the distance between your eyes. Instead of the eyes, astronomers typically use the distance from the Earth to the Sun, by observing when the Earth is at diametrically opposite points during its orbit (approximately).
                      See: https://en.m.wikipedia.org/wiki/Parallax under "distance measurement" for more details.







                      share|improve this answer












                      share|improve this answer



                      share|improve this answer










                      answered Nov 29 '18 at 7:53









                      TosicTosic

                      36019




                      36019























                          4












                          $begingroup$

                          It is both



                          But, specifically, the small motion is what we observe of the star at opposing points of Earth's orbit around the Sun. Then, because we know the radius of that orbit (1 AU) we can use the parallax, the observed small angular change in the location of a star against a distant background between opposite sides of the Earth's orbit, to make a parallax estimate of the star's distance, which is the inverse of small angular change (in radians) in units of parsecs.



                          enter image description here






                          share|improve this answer









                          $endgroup$


















                            4












                            $begingroup$

                            It is both



                            But, specifically, the small motion is what we observe of the star at opposing points of Earth's orbit around the Sun. Then, because we know the radius of that orbit (1 AU) we can use the parallax, the observed small angular change in the location of a star against a distant background between opposite sides of the Earth's orbit, to make a parallax estimate of the star's distance, which is the inverse of small angular change (in radians) in units of parsecs.



                            enter image description here






                            share|improve this answer









                            $endgroup$
















                              4












                              4








                              4





                              $begingroup$

                              It is both



                              But, specifically, the small motion is what we observe of the star at opposing points of Earth's orbit around the Sun. Then, because we know the radius of that orbit (1 AU) we can use the parallax, the observed small angular change in the location of a star against a distant background between opposite sides of the Earth's orbit, to make a parallax estimate of the star's distance, which is the inverse of small angular change (in radians) in units of parsecs.



                              enter image description here






                              share|improve this answer









                              $endgroup$



                              It is both



                              But, specifically, the small motion is what we observe of the star at opposing points of Earth's orbit around the Sun. Then, because we know the radius of that orbit (1 AU) we can use the parallax, the observed small angular change in the location of a star against a distant background between opposite sides of the Earth's orbit, to make a parallax estimate of the star's distance, which is the inverse of small angular change (in radians) in units of parsecs.



                              enter image description here







                              share|improve this answer












                              share|improve this answer



                              share|improve this answer










                              answered Nov 29 '18 at 19:12









                              kingledionkingledion

                              22316




                              22316























                                  3












                                  $begingroup$

                                  It is really just imprecise language in the first example.



                                  Parallax is the change in apparent position. To be formally correct, you measure or observe parallax and use it, with trigonometry, to determine the distance.



                                  You can call this the parallax method of distance measurement. What you have found is that people often omit the word "method".



                                  More precise language would be either:




                                  Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. One uses an effect called parallax.



                                  Astronomers have developed a variety of clever techniques for measuring the vast distances to stars, one is by measuring parallax.



                                  Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. The parallax method is one of them.




                                  A similar issue comes up with "Doppler".






                                  share|improve this answer









                                  $endgroup$


















                                    3












                                    $begingroup$

                                    It is really just imprecise language in the first example.



                                    Parallax is the change in apparent position. To be formally correct, you measure or observe parallax and use it, with trigonometry, to determine the distance.



                                    You can call this the parallax method of distance measurement. What you have found is that people often omit the word "method".



                                    More precise language would be either:




                                    Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. One uses an effect called parallax.



                                    Astronomers have developed a variety of clever techniques for measuring the vast distances to stars, one is by measuring parallax.



                                    Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. The parallax method is one of them.




                                    A similar issue comes up with "Doppler".






                                    share|improve this answer









                                    $endgroup$
















                                      3












                                      3








                                      3





                                      $begingroup$

                                      It is really just imprecise language in the first example.



                                      Parallax is the change in apparent position. To be formally correct, you measure or observe parallax and use it, with trigonometry, to determine the distance.



                                      You can call this the parallax method of distance measurement. What you have found is that people often omit the word "method".



                                      More precise language would be either:




                                      Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. One uses an effect called parallax.



                                      Astronomers have developed a variety of clever techniques for measuring the vast distances to stars, one is by measuring parallax.



                                      Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. The parallax method is one of them.




                                      A similar issue comes up with "Doppler".






                                      share|improve this answer









                                      $endgroup$



                                      It is really just imprecise language in the first example.



                                      Parallax is the change in apparent position. To be formally correct, you measure or observe parallax and use it, with trigonometry, to determine the distance.



                                      You can call this the parallax method of distance measurement. What you have found is that people often omit the word "method".



                                      More precise language would be either:




                                      Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. One uses an effect called parallax.



                                      Astronomers have developed a variety of clever techniques for measuring the vast distances to stars, one is by measuring parallax.



                                      Astronomers have developed a variety of clever techniques for measuring the vast distances to stars. The parallax method is one of them.




                                      A similar issue comes up with "Doppler".







                                      share|improve this answer












                                      share|improve this answer



                                      share|improve this answer










                                      answered Nov 29 '18 at 20:46









                                      user71659user71659

                                      1312




                                      1312






























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