11 infant stars, 1 million years (unexplored) Beautiful!

Had to rep this. Those stars were freaky and cool. Was weird to see those stars spinning so quickly. You should really put up some screenshots (suggest you grab a sidewinder if you can and get some sunroof screens).
 
They spin so fast, I'm wondering if this isn't a bug. I mean, do you realize the speed at which those have to be turning? I don't think it could even maintain its integrity.
 
Love the blue / green stars, though the T Tauris look weird with the rapid rotation? Also, I wonder if we'll get to see accretion disks at some point?
 
Fast spinning stars are probably not a bug. There are pulsars spinning at sub second frequencies. Not sure this is possible with suns of bigger sizes, lets say size of our sun, without tearing them apart or making them look like a lense at least.
 
I think what makes the 'fast-spinning' look odd is the way the stars (and really most objects) are modeled in the game, in that they're solid objects, when real stars are fluid. Stars would start to flatten out towards a disc shape if they're rapidly spinning. And the flares on the surface would likely look very different as well, if they looked like that at all. (I think there'd be some very strange-looking phenomena with such stars, which I hope make it into the game someday.)
 
I think what makes the 'fast-spinning' look odd is the way the stars (and really most objects) are modeled in the game, in that they're solid objects, when real stars are fluid. Stars would start to flatten out towards a disc shape if they're rapidly spinning. And the flares on the surface would likely look very different as well, if they looked like that at all. (I think there'd be some very strange-looking phenomena with such stars, which I hope make it into the game someday.)

Once the game goes live I'm heading out to the below star:

http://en.wikipedia.org/wiki/Achernar

I'd love to see what shape it is in the game.
 
Love the T Tauri Stars.

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I think, this fast spinning stars should be pulsars.
The system is official known as Gliese NN 3705 and in the catalogue it is marked as a DA4 Star. (White Dwarf)
A system with white dwarfs and a couple of pulsars should be likely, at least in my understanding, because both are very old stars. (And not very young ones, like in ED for the moment :D)

Neutron stars and pulsars seems to be not implemented yet.
Same with VY Canis Majoris.
The second star should be a neutron star and in ED it is marked as a Y5V. (brown dwarf)

Hopefully, we will see this in gamma. But on the other hand, this would destroy this beautiful system.:eek:
 
They spin so fast, I'm wondering if this isn't a bug. I mean, do you realize the speed at which those have to be turning? I don't think it could even maintain its integrity.

It's not a bug.
Some stars, neutron stars i.e. pulsars, spin almost 1000 times per second. Google for milisecond pulsar.
Something that weights as much as the Sun, and is the size of Manhattan, spinning around 1000 times every second.
Insane stuff.

The star models don't yet seem capable of reproducing the actual distortions found in actual stars.
Something spinning as fast as one of them in the vid would be a little distorted but not much, Stars are incredibly massive and have a lot of gravity holding them together. It would be an oblate spheroid, similar to the Earth, though. As far as I can tell that's not currently being modelled.

In the real universe it would seem that most "solid" objects, stars, planets etc..., only get to be oblate or have reasonably small distortions. It may be that only really large objects that are loosely gravitationally bound and have some angular momentum, that actually form into discs. I don't think it's possible for a star. Possibly due to the proximity of the core and the effect it would have on the internal density. The star may stop shining if it were too oblate.
Most neutron stars are almost perfect spheres that are held rigid by their gravity. Some of the really fast spinning ones are slightly oblate but only by a very tiny percentage I think.

So the simulation is pretty accurate but for completeness the fast spinning objects do need to be shown as oblate spheres. whether we would be able to detect that they are oblate is another matter. They may already be so but we can't detect it without instrumentation. Our brains and eyes may be nowhere near good enough to detect it. Like in the sun. Looks perfectly round to us. But it's definitely an oblate spheroid. Same with the Earth.
 
Thanks eveeryone, I couldn't pass up the opportunity to film this system-especially if it's going to be changed in Gamma. Really cool place to visit if you get time.

I've updated my main post with the second version, includes a couple planetary bodies and some HUDless shots.
 
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A quick google and download of some papers on the rotation periods of T-Tauri stars seems to suggest rotation periods in the order of days, rather than seconds. Where's Dr Wookie for clarification when you need him? :)

Edit: Sample reference used: http://arxiv.org/pdf/1301.2493v2.pdf
 
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