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0 answers
68 views

Impact Parameter as function of orbital parameters

In the case of a binary system (pulsar+companion), the impact parameter $\textbf{b}$ is the projection of the binary separation $\textbf{r}$ on the sky plane: \begin{equation}\tag{1} \textbf{b} = \...
gravitone123's user avatar
4 votes
0 answers
161 views

Confusion about Post-Newtonian orbital motion (Damour-Deruelle)

In their famous paper in 1985 (link), Damour&Deruelle describe the orbital motion for a binary system taking into account first-order post-Newtonian corrections (1PN). The solution is given in ...
gravitone123's user avatar
0 votes
1 answer
32 views

Inquiry Regarding Hypothetical Celestial Mechanics Scenario

How would the addition of a second sun, located at the other focus of the planet's elliptical orbit, impact the motion and orbit of the planet? Specifically, how would the gravitational forces from ...
user avatar
0 votes
1 answer
119 views

Does the Centre of Mass of a binary star system accelerate?

At the COM of a binary star system (where both stars has a different mass), the net force at the centre of mass is non-zero. Does this mean that the COM will be accelerating? And if so, wouldn't the ...
john's user avatar
  • 568
1 vote
1 answer
49 views

Pair of binary stars orbiting each other

Suppose we have a pair of binary stars orbiting around each other in their mutual gravitational field. My question is, is the trajectory of the combined system would be an ellipse? And, if it is an ...
Sambhav Antriksh's user avatar
2 votes
0 answers
304 views

Find semi-minor axis of elliptical binary orbit given semi-major axis and mass ratio

I'm working on a simulation of binary stars. I'm using Kepler's Laws to solve for the angular velocity given the semi-major axis $a$ and the masses $m_1$ and $m_2$ of the two objects in an elliptical ...
Sofia Splawska's user avatar
2 votes
3 answers
241 views

Could two planets trapped between two stars orbit each other?

Say there are two stars, each exerting and equal force on a point in the midde of them. For simplicity, we'll say the two stars have the same mass and are equidistant from the point. Now suppose that ...
TheDragonOfFlame's user avatar
0 votes
1 answer
77 views

Binary stars orbiting around each other are equidistant [closed]

This is a problem that was given to me in my Classical Mechanics course: J.S.Plaskett's star is one of the most massive stars known at present. It is a binary star, that is, it consists of two stars ...
Lt. Commander. Data's user avatar
1 vote
1 answer
133 views

Keplerian orbital elements of a binary system: computing the eccentricity vector and angular momentum vector

I have been given a binary system and know a few of the keplerian orbital elements such as ...
Warrenmovic 's user avatar
0 votes
1 answer
36 views

Position vector of an eccentric binary

For a circular, equatorial ($z=0$) Newtonian binary, the position can be clearly written as, $$ x_i = r(\cos \Omega t, \sin \Omega t, 0)$$ for orbital frequency $\Omega$. My question is how would ...
user1887919's user avatar
  • 1,751
1 vote
1 answer
415 views

Barycenter of a binary star system

It is said that the barycenter of 11 Draconis (Thuban) and 10 Draconis which compose a binary star system is a central point. Is this central point a material or immaterial object? Does the size of ...
starstruck's user avatar
4 votes
3 answers
3k views

Kepler's 3rd law applied to binary systems: How can the two orbits have different semi-major axes?

I suddenly came to the realization that I don't understand something about Kepler's law when applied to binary systems, because I encountered an apparent paradox. There must be an error somewhere in ...
Inzinity's user avatar
  • 830
6 votes
1 answer
2k views

Conservation of spin angular momentum in a close binary system

Consider a simple model of a close stellar binary, of mass $m_1$ and $m_2 < m_1$, moving on circular orbits around the system's barycenter (no eccentricity, to simplify things). Both star's ...
Cham's user avatar
  • 7,592
0 votes
0 answers
174 views

Double star system; relative orbit in the case of elliptical orbits

In my physics book they say that the relative distance between two stars (that both have elliptical orbits) in a double-star system equals $4.0 AU$ in the pericenter, and $16.0AU$ in the apocenter. ...
Sha Vuklia's user avatar
0 votes
2 answers
761 views

Will two planets in a binary star system rotate in the same circle around the mass center every period?

I am modeling a two binary star system, and I am wondering if this is the case. The way I have it right now is that I first figure out the mass center, and then the radius from each of the planet to ...
David Lund's user avatar

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