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Can a system of three stars exist?


How many stars can stay close to each other without collapsing?Ramifications of black hole stellar systemWhat happens if two or three stars collide with each other?Could this three moons system be stable?Hip2.dat and Solo, Binary and Multiple Star SystemsA “tidally locked” double planet?Can Two Stars of One Same Type Orbit Each Other?Doing Correct Calculations with Binary Star SystemsIn System KIC 9246715, How Far Does One Star Orbit the Other?






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2












$begingroup$


Just like binary stars can a system of three stars mutually equidistant from each other?
What I mean is three stars at the vertices of a equilateral
If yes than what will be the orbit of a planet out there
If no what will be the problem for it's nonexistence?










share|improve this question







New contributor



Heth Ghetiya is a new contributor to this site. Take care in asking for clarification, commenting, and answering.
Check out our Code of Conduct.






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    2












    $begingroup$


    Just like binary stars can a system of three stars mutually equidistant from each other?
    What I mean is three stars at the vertices of a equilateral
    If yes than what will be the orbit of a planet out there
    If no what will be the problem for it's nonexistence?










    share|improve this question







    New contributor



    Heth Ghetiya is a new contributor to this site. Take care in asking for clarification, commenting, and answering.
    Check out our Code of Conduct.






    $endgroup$
















      2












      2








      2





      $begingroup$


      Just like binary stars can a system of three stars mutually equidistant from each other?
      What I mean is three stars at the vertices of a equilateral
      If yes than what will be the orbit of a planet out there
      If no what will be the problem for it's nonexistence?










      share|improve this question







      New contributor



      Heth Ghetiya is a new contributor to this site. Take care in asking for clarification, commenting, and answering.
      Check out our Code of Conduct.






      $endgroup$




      Just like binary stars can a system of three stars mutually equidistant from each other?
      What I mean is three stars at the vertices of a equilateral
      If yes than what will be the orbit of a planet out there
      If no what will be the problem for it's nonexistence?







      star orbit






      share|improve this question







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      Heth Ghetiya is a new contributor to this site. Take care in asking for clarification, commenting, and answering.
      Check out our Code of Conduct.










      share|improve this question







      New contributor



      Heth Ghetiya is a new contributor to this site. Take care in asking for clarification, commenting, and answering.
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      share|improve this question






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      asked 8 hours ago









      Heth GhetiyaHeth Ghetiya

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      New contributor



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          2 Answers
          2






          active

          oldest

          votes


















          3













          $begingroup$

          Systems of three stars can exist, but a system of three stars in a triangle is unstable and won't exist in reality. There are configurations of three stars that are stable, for example, two stars in a close orbit about their common centre of gravity, and a third star in a distant orbit.



          Planets can exist in such a system, they could orbit around the distant third star (like a moon orbits a planet), or they could be circumbinary, around the two close stars. Such complex systems are more likely to be unstable on the scale of billions of years. The key to stability is having each body in approximately an inverse-square gravitational field, so its orbit can be approximated by a Keplerian ellipse. That is not the case if three equal mass bodies are in an equilateral triangle.






          share|improve this answer









          $endgroup$














          • $begingroup$
            Why? If there is a huge star, then two other stars could orbit it. They would be each others' Trojans.
            $endgroup$
            – peterh
            6 hours ago










          • $begingroup$
            There are stable equilateral systems, but not with equal masses. There's some info here & anims here. For some interesting stable n-body systems of equal mass see Cris Moore's gallery. Eg, the figure-8 orbit
            $endgroup$
            – PM 2Ring
            6 hours ago


















          2













          $begingroup$

          It is possible in a Trojan configuration:



          enter image description here



          In the place of the "Planet" on the image, also a small star could exist. The third star would be at $L_4$ or at $L_5$. This configuration could be made stable.



          However, as this link shows,




          In unnormalized units, this criterion becomes



          $$fracm_2m_1+ m_2 < 0.0385$$



          We thus conclude that the $L_4$ and $L_5$ Lagrange points are stable
          equilibrium points, in the co-rotating frame, provided that mass $m_2$
          is less than about $4%$ of mass $m_1$.




          Thus, the mass of the second star should be at most 3.85% of the central star.



          As far I know, no such known star system exists, but if it would, it would be stable.






          share|improve this answer











          $endgroup$

















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            2 Answers
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            active

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            2 Answers
            2






            active

            oldest

            votes









            active

            oldest

            votes






            active

            oldest

            votes









            3













            $begingroup$

            Systems of three stars can exist, but a system of three stars in a triangle is unstable and won't exist in reality. There are configurations of three stars that are stable, for example, two stars in a close orbit about their common centre of gravity, and a third star in a distant orbit.



            Planets can exist in such a system, they could orbit around the distant third star (like a moon orbits a planet), or they could be circumbinary, around the two close stars. Such complex systems are more likely to be unstable on the scale of billions of years. The key to stability is having each body in approximately an inverse-square gravitational field, so its orbit can be approximated by a Keplerian ellipse. That is not the case if three equal mass bodies are in an equilateral triangle.






            share|improve this answer









            $endgroup$














            • $begingroup$
              Why? If there is a huge star, then two other stars could orbit it. They would be each others' Trojans.
              $endgroup$
              – peterh
              6 hours ago










            • $begingroup$
              There are stable equilateral systems, but not with equal masses. There's some info here & anims here. For some interesting stable n-body systems of equal mass see Cris Moore's gallery. Eg, the figure-8 orbit
              $endgroup$
              – PM 2Ring
              6 hours ago















            3













            $begingroup$

            Systems of three stars can exist, but a system of three stars in a triangle is unstable and won't exist in reality. There are configurations of three stars that are stable, for example, two stars in a close orbit about their common centre of gravity, and a third star in a distant orbit.



            Planets can exist in such a system, they could orbit around the distant third star (like a moon orbits a planet), or they could be circumbinary, around the two close stars. Such complex systems are more likely to be unstable on the scale of billions of years. The key to stability is having each body in approximately an inverse-square gravitational field, so its orbit can be approximated by a Keplerian ellipse. That is not the case if three equal mass bodies are in an equilateral triangle.






            share|improve this answer









            $endgroup$














            • $begingroup$
              Why? If there is a huge star, then two other stars could orbit it. They would be each others' Trojans.
              $endgroup$
              – peterh
              6 hours ago










            • $begingroup$
              There are stable equilateral systems, but not with equal masses. There's some info here & anims here. For some interesting stable n-body systems of equal mass see Cris Moore's gallery. Eg, the figure-8 orbit
              $endgroup$
              – PM 2Ring
              6 hours ago













            3














            3










            3







            $begingroup$

            Systems of three stars can exist, but a system of three stars in a triangle is unstable and won't exist in reality. There are configurations of three stars that are stable, for example, two stars in a close orbit about their common centre of gravity, and a third star in a distant orbit.



            Planets can exist in such a system, they could orbit around the distant third star (like a moon orbits a planet), or they could be circumbinary, around the two close stars. Such complex systems are more likely to be unstable on the scale of billions of years. The key to stability is having each body in approximately an inverse-square gravitational field, so its orbit can be approximated by a Keplerian ellipse. That is not the case if three equal mass bodies are in an equilateral triangle.






            share|improve this answer









            $endgroup$



            Systems of three stars can exist, but a system of three stars in a triangle is unstable and won't exist in reality. There are configurations of three stars that are stable, for example, two stars in a close orbit about their common centre of gravity, and a third star in a distant orbit.



            Planets can exist in such a system, they could orbit around the distant third star (like a moon orbits a planet), or they could be circumbinary, around the two close stars. Such complex systems are more likely to be unstable on the scale of billions of years. The key to stability is having each body in approximately an inverse-square gravitational field, so its orbit can be approximated by a Keplerian ellipse. That is not the case if three equal mass bodies are in an equilateral triangle.







            share|improve this answer












            share|improve this answer



            share|improve this answer










            answered 7 hours ago









            James KJames K

            38k2 gold badges66 silver badges128 bronze badges




            38k2 gold badges66 silver badges128 bronze badges














            • $begingroup$
              Why? If there is a huge star, then two other stars could orbit it. They would be each others' Trojans.
              $endgroup$
              – peterh
              6 hours ago










            • $begingroup$
              There are stable equilateral systems, but not with equal masses. There's some info here & anims here. For some interesting stable n-body systems of equal mass see Cris Moore's gallery. Eg, the figure-8 orbit
              $endgroup$
              – PM 2Ring
              6 hours ago
















            • $begingroup$
              Why? If there is a huge star, then two other stars could orbit it. They would be each others' Trojans.
              $endgroup$
              – peterh
              6 hours ago










            • $begingroup$
              There are stable equilateral systems, but not with equal masses. There's some info here & anims here. For some interesting stable n-body systems of equal mass see Cris Moore's gallery. Eg, the figure-8 orbit
              $endgroup$
              – PM 2Ring
              6 hours ago















            $begingroup$
            Why? If there is a huge star, then two other stars could orbit it. They would be each others' Trojans.
            $endgroup$
            – peterh
            6 hours ago




            $begingroup$
            Why? If there is a huge star, then two other stars could orbit it. They would be each others' Trojans.
            $endgroup$
            – peterh
            6 hours ago












            $begingroup$
            There are stable equilateral systems, but not with equal masses. There's some info here & anims here. For some interesting stable n-body systems of equal mass see Cris Moore's gallery. Eg, the figure-8 orbit
            $endgroup$
            – PM 2Ring
            6 hours ago




            $begingroup$
            There are stable equilateral systems, but not with equal masses. There's some info here & anims here. For some interesting stable n-body systems of equal mass see Cris Moore's gallery. Eg, the figure-8 orbit
            $endgroup$
            – PM 2Ring
            6 hours ago













            2













            $begingroup$

            It is possible in a Trojan configuration:



            enter image description here



            In the place of the "Planet" on the image, also a small star could exist. The third star would be at $L_4$ or at $L_5$. This configuration could be made stable.



            However, as this link shows,




            In unnormalized units, this criterion becomes



            $$fracm_2m_1+ m_2 < 0.0385$$



            We thus conclude that the $L_4$ and $L_5$ Lagrange points are stable
            equilibrium points, in the co-rotating frame, provided that mass $m_2$
            is less than about $4%$ of mass $m_1$.




            Thus, the mass of the second star should be at most 3.85% of the central star.



            As far I know, no such known star system exists, but if it would, it would be stable.






            share|improve this answer











            $endgroup$



















              2













              $begingroup$

              It is possible in a Trojan configuration:



              enter image description here



              In the place of the "Planet" on the image, also a small star could exist. The third star would be at $L_4$ or at $L_5$. This configuration could be made stable.



              However, as this link shows,




              In unnormalized units, this criterion becomes



              $$fracm_2m_1+ m_2 < 0.0385$$



              We thus conclude that the $L_4$ and $L_5$ Lagrange points are stable
              equilibrium points, in the co-rotating frame, provided that mass $m_2$
              is less than about $4%$ of mass $m_1$.




              Thus, the mass of the second star should be at most 3.85% of the central star.



              As far I know, no such known star system exists, but if it would, it would be stable.






              share|improve this answer











              $endgroup$

















                2














                2










                2







                $begingroup$

                It is possible in a Trojan configuration:



                enter image description here



                In the place of the "Planet" on the image, also a small star could exist. The third star would be at $L_4$ or at $L_5$. This configuration could be made stable.



                However, as this link shows,




                In unnormalized units, this criterion becomes



                $$fracm_2m_1+ m_2 < 0.0385$$



                We thus conclude that the $L_4$ and $L_5$ Lagrange points are stable
                equilibrium points, in the co-rotating frame, provided that mass $m_2$
                is less than about $4%$ of mass $m_1$.




                Thus, the mass of the second star should be at most 3.85% of the central star.



                As far I know, no such known star system exists, but if it would, it would be stable.






                share|improve this answer











                $endgroup$



                It is possible in a Trojan configuration:



                enter image description here



                In the place of the "Planet" on the image, also a small star could exist. The third star would be at $L_4$ or at $L_5$. This configuration could be made stable.



                However, as this link shows,




                In unnormalized units, this criterion becomes



                $$fracm_2m_1+ m_2 < 0.0385$$



                We thus conclude that the $L_4$ and $L_5$ Lagrange points are stable
                equilibrium points, in the co-rotating frame, provided that mass $m_2$
                is less than about $4%$ of mass $m_1$.




                Thus, the mass of the second star should be at most 3.85% of the central star.



                As far I know, no such known star system exists, but if it would, it would be stable.







                share|improve this answer














                share|improve this answer



                share|improve this answer








                edited 3 hours ago

























                answered 6 hours ago









                peterhpeterh

                1,8483 gold badges13 silver badges32 bronze badges




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