How often do you see binary star systems like this?

There are several binary systems, and I've been in a lot of them.

But like that one, I've only saw one, was tempted to fly between both stars so much :D
 
Is that physically even possible? I'd expect two stars, so close to each other, would have to orbit each other at such a high speed that they're probably wildly deformed.
 
I've flown to many. Some are far enough you can fly between, it makes for interesting fuel scoop techniques.

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Found one so far :D

and yes my first thought was... wonder if i can fit between there without cooking myself... LoL

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(sorry for the bad screenie, before i knew about alt-f10, shift + alt + g and the like)
 
There's a system similar near LHS 3447, can't remember what it's called. I jumped into on my first or second day and found myself coming out hyperspace between the two stars... My first experience of escape vectors was interesting. But I survived to tell the tale.
 
I've flown to many. Some are far enough you can fly between, it makes for interesting fuel scoop techniques.

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I once tryed to scope between closeup binaryes. BAD IDEA! Scooping rate was unefected but the heat goes nuts - was right between them as i realized it, with full throttle i made it out with 180% heat and the heartrate of a kolibri...
 
Its not, those stars would indeed be deformed and twisted into each other

It is possible. There are stars that are that close that can take hundreds and even hundreds of thousands of years to orbit one another. Why do I know this? Because I found a similar system and thought the same thing. So I did some research and it turns out that most binaries like this do not orbit each other at incredibly high speeds like you'd think, instead most orbit each other in slow procession. The reason they can do it is because the mass of the stars is almost identical, therefore the gravitational forces almost cancel each other out and the stars orbit a mutual point in space. Which is really hard to comprehend that this is even possible, but according to astronomers, it's not only possible - but very common.
 
They would spiral in. Gravity doesn't cancel out the way you think it does. You'd need a third mass or more to do that, but then you have the three body problem and everything gets complicated.

There are stars that orbit really close, but fast (5 hours is the usual cut-off for sun-like stars, less for red dwarfs).
 
It is possible. There are stars that are that close that can take hundreds and even hundreds of thousands of years to orbit one another. Why do I know this? Because I found a similar system and thought the same thing. So I did some research and it turns out that most binaries like this do not orbit each other at incredibly high speeds like you'd think, instead most orbit each other in slow procession. The reason they can do it is because the mass of the stars is almost identical, therefore the gravitational forces almost cancel each other out and the stars orbit a mutual point in space. Which is really hard to comprehend that this is even possible, but according to astronomers, it's not only possible - but very common.
Yes and no. Most binaries are very far apart, just like you said. But there are binaries that are as close as those shown in this thread. They are called "contact binaries" and orbit each other quite rapidly, usually within in a few hours. And these would be deformed and sometimes even fused, just liked Mellom said.
 
Yes and no. Most binaries are very far apart, just like you said. But there are binaries that are as close as those shown in this thread. They are called "contact binaries" and orbit each other quite rapidly, usually within in a few hours. And these would be deformed and sometimes even fused, just liked Mellom said.

No, I am sorry, but you're wrong.

It is estimated that approximately 1/3 of the star systems in the Milky Way are binary or multiple, with the remaining 2/3 consisting of single stars.[62]

There is a direct correlation between the period of revolution of a binary star and the eccentricity of its orbit, with systems of short period having smaller eccentricity. Binary stars may be found with any conceivable separation, from pairs orbiting so closely that they are practically in contact with each other, to pairs so distantly separated that their connection is indicated only by their common proper motion through space. Among gravitationally bound binary star systems, there exists a so-called log normal distribution of periods, with the majority of these systems orbiting with a period of about 100 years. This is supporting evidence for the theory that binary systems are formed during star formation.[63]

In pairs where the two stars are of equal brightness, they are also of the same spectral type. In systems where the brightnesses are different, the fainter star is bluer if the brighter star is a giant star, and redder if the brighter star belongs to the main sequence.[64]
Artist's impression of the sight from a (hypothetical) moon of planet HD 188753 Ab (upper left), which orbits a triple star system. The brightest companion is just below the horizon.
Artist's impression of the sight from a (hypothetical) moon of planet HD 188753 Ab (upper left), which orbits a triple star system. The brightest companion is just below the horizon.

The mass of a star can be directly determined only from its gravitational attraction. Apart from the Sun and stars which act as gravitational lenses, this can be done only in binary and multiple star systems, making the binary stars an important class of stars. In the case of a visual binary star, after the orbit and the stellar parallax of the system has been determined, the combined mass of the two stars may be obtained by a direct application of the Keplerian harmonic law.[65]
 
No, I am sorry, but you're wrong.

Yeah those ones that orbit in the order of hundreds of years AREN'T the ones that are almost touching... Which would also be gravitationally distorted, not the perfect spheres we're seeing in the game.

IF they orbited slowly they'd just fall in together, like two magnetic balls that are close to each other, if they're moving fast enough they won't fall in together, but when their speed drops magnetism would take over and they'd move towards each other.
 
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