Closed ajtribick closed 11 months ago
So I did a little peek into this issue and it looks like Luhman 16's issue is just the erroneous mean anomaly (and for the other parameters, I arrived at slightly different values due to using position in Table 7). I haven't checked the other systems yet at this point.
Is this one done now?
I think so for now. Thanks!
The following is a check on the various binary star systems in the first ~50% of nearstars.stc (down to 36 Oph).
Reversed orbits
These systems typically look correct from the perspective of the view of the sky-plane, but they are reversed in the radial direction.
Luhman 16
Reference: https://arxiv.org/pdf/1808.07835.pdf - table 6
In 2014, the radial velocity V_A - V_B is positive, implying that Luhman 16 A is receding faster than Luhman 16 B. In Celestia, this situation is reversed: Luhman 16 A is moving towards the Sun (-ve RV), Luhman 16 B is moving away
Sirius
Reference: https://arxiv.org/pdf/1809.01240.pdf - figure 9
At the current time, Sirius B should have a positive RV with respect to the system barycenter (i.e. receding). In Celestia, Sirius B is approaching the Sun.
Gliese 65
Reference: https://www.aanda.org/articles/aa/pdf/2016/09/aa28631-16.pdf - section 3.2
Measured V_B - V_A as positive on 2005-11-17, i.e. Gliese 65 B should be receding w.r.t. Gliese 65 A. In Celestia, Gliese 65 B is approaching the Sun, Gliese 65 A is receding.
Gliese 234
Reference: https://iopscience.iop.org/article/10.3847/1538-4365/ac7e57/pdf - figure 4
As shown on the RV diagram, the RV of Gliese 234 A at epoch 2456418 should be negative, i.e. approaching. Celestia shows this star as receding.
Gliese 229
Reference: https://iopscience.iop.org/article/10.3847/1538-3881/ac273e/pdf - figure 8
Radial velocity should be increasing from 2005 to 2020, in Celestia the radial velocity appears to be decreasing.
Correct orbits
As far as I can see, the following have the correct orbits in terms of radial velocities.
Undetermined
Could not check these, most cases due to insufficient RV data to distinguish between the two possible orientations that match the visual orbit.