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Dont do it, you're gonna blow your ship upBut like that one, I've only saw one, was tempted to fly between both stars so much![]()
Its not, those stars would indeed be deformed and twisted into each otherIs that physically even possible?
I even had a drop from SC were I was literally flying through a brown dwarf (in the short 1 second decelerating phase when dropping out of SC).
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...I've flown to many. Some are far enough you can fly between, it makes for interesting fuel scoop techniques.
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Its not, those stars would indeed be deformed and twisted into each other
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.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.
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.
No, you are wrong. Here's one example where the stars orbit very close to each other (but not as close as in this thread), and there's accretion disks and all sorts of fun stuff.No, I am sorry, but you're wrong.
No, you are wrong. Here's one example where the stars orbit very close to each other (but not as close as in this thread), and there's accretion disks and all sorts of fun stuff.
http://en.wikipedia.org/wiki/Beta_Lyrae
and here is a non-simulated animation of those stars, do they look like in normal shape?
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