I am out exploring and made a tour to see the system VV CEPHEI. From our observations this a binary star system with a red supergiant star and a smaller companion star. Furthermore VV CEPHEI A is one of the biggest known stars in the milky way.
I give you wikipedia as source, because the information are packed nicely together there. http://en.wikipedia.org/wiki/VV_Cephei
Yesterday I reached my destination and I was disappointed to say the least. In the game VV CEPHEI is one single supergiant, that has only a fraction of the size it should have.
This is what I found:
The two big problems I have with this are the two obvious ones:
A) It is way to small. It is widely belived this star has a solar radius of at the very least(!) 1,050. Ingame this was reduced to 318? From everything I've heard and discovered so far, the systems in ED are modeled after what we know of them NOW. I know, that in fact our knowledge is centuries old the further we are from a star, but I was under the impression this is not part of the star calculation. And this wouldn't explain:
B) Where is VV CEPHEI B? Not much to say here. It is by fact a binary system.
I accepted, that the distances in ED are inacurate to what is believed to be known today. I was also not expecting to see the mass transfer, that should be visible between star A and B. But I was not prepared to find a whole different system at my destination. Maybe someone can shine a light at some facts I am missing. Otherwise I'm not sure if exploring can be "I'm going to a certain POI I know exists" other than "well, I just fly in one direction, hoping to find something".
:S:S:S
I give you wikipedia as source, because the information are packed nicely together there. http://en.wikipedia.org/wiki/VV_Cephei
Yesterday I reached my destination and I was disappointed to say the least. In the game VV CEPHEI is one single supergiant, that has only a fraction of the size it should have.
This is what I found:
The two big problems I have with this are the two obvious ones:
A) It is way to small. It is widely belived this star has a solar radius of at the very least(!) 1,050. Ingame this was reduced to 318? From everything I've heard and discovered so far, the systems in ED are modeled after what we know of them NOW. I know, that in fact our knowledge is centuries old the further we are from a star, but I was under the impression this is not part of the star calculation. And this wouldn't explain:
B) Where is VV CEPHEI B? Not much to say here. It is by fact a binary system.
I accepted, that the distances in ED are inacurate to what is believed to be known today. I was also not expecting to see the mass transfer, that should be visible between star A and B. But I was not prepared to find a whole different system at my destination. Maybe someone can shine a light at some facts I am missing. Otherwise I'm not sure if exploring can be "I'm going to a certain POI I know exists" other than "well, I just fly in one direction, hoping to find something".
:S:S:S