# How did they measure the distance to the center of our galaxy to 0.3% accuracy?

The abstract of A geometric distance measurement to the Galactic center black hole with 0.3% uncertainty (Open Access) says:

We present a 0.16% precise and 0.27% accurate determination of R₀, the distance to the Galactic center. Our measurement uses the star S2 on its 16-year orbit around the massive black hole Sgr A* that we followed astrometrically and spectroscopically for 27 years. Since 2017, we added near-infrared interferometry with the VLTI beam combiner GRAVITY, yielding a direct measurement of the separation vector between S2 and Sgr A* with an accuracy as good as 20 μas in the best cases. S2 passed the pericenter of its highly eccentric orbit in May 2018, and we followed the passage with dense sampling throughout the year. Together with our spectroscopy, in the best cases with an error of 7 km s−1, this yields a geometric distance estimate of R₀ = 8178 ± 13stat. ± 22sys. pc. This work updates our previous publication, in which we reported the first detection of the gravitational redshift in the S2 data. The redshift term is now detected with a significance level of 20σ with fredshift = 1.04 ± 0.05.

and figure 2 shown below provides an example of the error analysis post fitting.

1. If you have the angular size of an orbit and a set of radial velocity measurements, even if it was viewed edge-on and the inclination was known, wouldn't this give only a parametric relationship between R₀ and the mass of the central object?

I don't understand how they were able to state a specific value for R₀, I'm probably missing something obvious but I can't figure it out. According to this answer:

We have reasonably good measurements of the mass of Sagittarius A*, thanks to measurements of the movements of stars like S0-2 over several decades. It's been well-established that the mass of the central object is $$M\approx4\times10^6M_{\odot}$$;

so to me the whole situation appears on the surface to be circular referencing. I'm sure it isn't of course, I'm just missing something.

2. Is the measurement really to the "Galactic center" as the first sentence of the abstract states, or really the distance to Sgr A* around which S2 orbits?

3. "bonus points" Why is every instance of "Galactic" in this published paper (not a preprint) capitalized?

Selected posterior densities as obtained from the MCMC sampler with N = 200 000, here for the noise model data set. The contour lines mark the 1, 2, and 3σ levels. We only show the diagrams with the strongest correlations. All parameters are well determined (see Appendix D). Source

• Things referring to our Galaxy or the Galaxy, should be capitalised. It is a proper noun, like the Sun. I guess this is just extended to Galactic to indicate it refers to the Galaxy. – Rob Jeffries Jul 26 at 3:38
• @RobJeffries Thanks for that! I wonder if it extends to the Galaxy on Orion's Belt as well? – uhoh Jul 26 at 3:46

The orbit of star S2 is completely determined by the astrometric observations. i.e. One has the orbital period, the angular scale of the orbit and the inclination of the orbital plane. With this information alone, the distance and central mass are degenerate. If you know the distance you get the mass and vice versa.

However, here the mass is not needed. Full knowledge of the orbit means that you can predict the radial (line of sight) velocity of the star at any point in its orbit. The conversion from the angular scale of the observations to an absolute velocity, depends (linearly) on the distance to the source.

Hence they fold a set of radial velocity measurements into their analysis and get an estimate of the distance.

The distance is that to Sgr A*. The paper discusses that this is compatible with other measurements of where the dynamical centre of the Galaxy is.

The Galaxy is a proper noun (like the Sun), referring to our Milky Way, and hence is capitalised. When referring to the Galaxy it is conventional (though not strictly necessary I think) to use the word Galactic to indicate a property of the Galaxy (as opposed to some other galaxy).

• Aha, so it's my very small "gedankenexperiment" in the question, setting inclination to zero (edge-on) that confused me. This technique doesn't work in that case, and for trivial reasons wouldn't work at 90 degrees either (no radial velocity). It's the in-between-ness of the inclination of S2 (~134 degrees) that makes this possible? – uhoh Jul 26 at 4:16
• The inclination is obtained from the requirement that Sgr A* be at a focus of the deprojected elliptical orbit. – Rob Jeffries Jul 26 at 4:19
• yep. I should have remembered my answer to my own question from last year Why does Earth not appear to be at the focus of TESS' elliptical orbit in this video? – uhoh Jul 26 at 4:35