On this site :
http://www.celestiaproject.net/gallery/view_al ... epe&page=2
there is some nice Sirius B pictures, which I think is a real object not included in Celestia's database. Can someone give here a complete ssc definition (with colors and glow) for this white dwarf ?
Sirius B ?
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Topic authorCham
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Sirius B ?
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Topic authorCham
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Okay, I've found the info on this forum, on an old discussion :
http://www.celestiaproject.net/forum/viewtopic ... ght=sirius
The only problem is , temperature doesn't fit.
http://www.celestiaproject.net/forum/viewtopic ... ght=sirius
The only problem is , temperature doesn't fit.
"Well! I've often seen a cat without a grin", thought Alice; "but a grin without a cat! It's the most curious thing I ever saw in all my life!"
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Here's the definition with a correctly orientated orbit:
Grant
Code: Select all
"Sirius B" "Sirius"
{
Texture "bstar.jpg"
Radius 5800
Emissive true
EllipticalOrbit {
Period 50.09
SemiMajorAxis 19.8
Eccentricity 0.592
Inclination 97.51
AscendingNode 161.33
ArgOfPericenter 184.56
MeanAnomaly 40.89
}
RotationPeriod 0.5 # plausible guess
}
Grant
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OK,but what texture is more accurate for Sirius B :"whitedwarf2.jpg" borrowed for the activity "Life and Death of the Stars" or "bstar.jpg"?
granthutchison wrote:Just because Celestia displays Sirius B's temperature as something like 100K, instead of the real value of 27000K.danielj wrote:Why the temperature not fitting is a problem?
Grant
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I have no idea what the surface of a white dwarf looks like, and have never seen whitedwarf2.jpg, so that makes things a bit tricky ...danielj wrote:OK,but what texture is more accurate for Sirius B :"whitedwarf2.jpg" borrowed for the activity "Life and Death of the Stars" or "bstar.jpg"?
But at 27000K Sirius B should look distinctly blue, like an early B star, which is why I chose the texture I did. See here for an approximate rendering of some star colours versus temperature.
Grant
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Topic authorCham
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How much oblateness (I guessed 0.09) for a white dwarf that rotate with a period of about 0.002 hours (exagerate guess?), with a radius of about 5800 km (is that too small?) ?
Do you have an idea ?
Do you have an idea ?
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Seems an extraordinarily fast rotation - a number of transverse velocities of close to 30km/s have been measured, implying a rotation period of around 20 minutes. At that speed the equatorial "centrifugal" force is about 1/10000th of the surface gravity. Compare Earth, where the equatorial "centrifugal" force is a 300th of the surface gravity, and results in an oblateness of only 0.003. These white dwarfs should be almost indistinguishable from spherical.
Grant
Grant
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Topic authorCham
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I think you're right, but astronomers are discovering that many stars may have a "big" oblateness, more than expected.
And the Earth is a pasty liquid with a hard crust. A white dwarf is more gazeous-liquid (I'm not sure about this). So the rotation may have a stronger effect on them. And as I can tell (not sure), a white dwarf is not so far away of a neutron star state, which may be spinning very fast.
And the Earth is a pasty liquid with a hard crust. A white dwarf is more gazeous-liquid (I'm not sure about this). So the rotation may have a stronger effect on them. And as I can tell (not sure), a white dwarf is not so far away of a neutron star state, which may be spinning very fast.
"Well! I've often seen a cat without a grin", thought Alice; "but a grin without a cat! It's the most curious thing I ever saw in all my life!"