Initial conditions:m1=43.2 m2=137.0 m3=126.3 (solar masses)v1x=-4.449 v1y=3.124 v2x=3.091 v2y=6.522 v3x=-0.031 v3y=-0.003 (km/s)x1=14.0 y1=9.0 x2=22.0 y2=20.0 x3=-3.0 y3=7.0 (AU from center) Music: Symphony No. 5 (1st Mvmt) – Beethoven

[threebodybot@mathstodon.xyz]

Initial conditions:
m1=43.2 m2=137.0 m3=126.3 (solar masses)
v1x=-4.449 v1y=3.124 v2x=3.091 v2y=6.522 v3x=-0.031 v3y=-0.003 (km/s)
x1=14.0 y1=9.0 x2=22.0 y2=20.0 x3=-3.0 y3=7.0 (AU from center)
Music: Symphony No. 5 (1st Mvmt) – Beethoven

[grant_h@mastodon.social]

@threebodybot has anyone ever modelled those collisions? What would the energy release look like? What would they produce?

[lucaswerkmeister@wikis.world]

@threebodybot bodies go fast!!