Astronomy · Our view of the Milky Way
Stellar and gas motion as evidence about mass
Project an original circular velocity field to expose a near–far ambiguity, then use a separate spherical force model to identify what a circular-speed estimate actually constrains.
Continue in the approved chapter order. Necessary vocabulary, quantities and assumptions are explained in the lesson.
Back to the chapterAfter reading, you can
- Distinguish a measured line-of-sight component from a three-dimensional orbit or circular speed.
- Calculate two distances with the same direction and observer-relative radial velocity.
- Apply an enclosed-mass relation only within its stated Newtonian spherical domain.
Motion becomes dynamical evidence through a model
A calibrated stellar or gas spectral shift constrains a line-of-sight velocity component under the appropriate spectral interpretation. Proper motion measures angular change on the sky and needs distance to yield a transverse speed. The observer’s motion must also be accounted for before combining those components in a Galactic frame.
A circular-speed curve describes the speed required for a circular orbit in an adopted potential. It is not the instantaneous total speed of every halo star or gas parcel. Random motions, pressure, bars, spiral structure and departures from equilibrium can matter when observed motions are related to that curve.
A longitude–velocity diagram displays viewing direction and line-of-sight velocity. It can reveal organized patterns without directly supplying a three-dimensional map. Bovy’s treatment of Galactic gas kinematics makes the observer-relative projection explicit; a rotation model is an added ingredient in a distance interpretation.
The following experiment isolates that geometry. All lengths and speeds are invented dimensionless ratios, and neither the observer’s radius nor the velocity scale is a fitted Solar or Galactic value.
State the geometry before projecting velocities
Use arbitrary positive units L0 and V0, with V0 small compared with the vacuum light speed. In a right-handed planar Cartesian drawing, put the centre C at (0,0) and observer O at (8,0)L0. The +x direction runs from the centre toward the observer; the observer moves along +y. All stipulated circular rotation is counterclockwise in this drawing.
Choose a sightline at l = 30° measured from the inward −x ray toward +y. Its outward-from-observer unit vector is n = (−√3/2, 1/2). A point at distance d has position P = O + dn. Thus a viewing direction and one positive distance specify a point, while a viewing direction alone specifies a ray.
On radii 1 ≤ R/L0 ≤ 8, give every circular tracer speed V0, with velocity v = (−y/R, x/R)V0 and R = √(x² + y²). The observer has v_O = (0,1)V0. There are no radial or vertical motions, turbulence, instrumental offsets or peculiar observer motion in this model.
Define v_los = (v − v_O)·n, positive for recession. Substitution gives v_los/V0 = [8/(R/L0) − 1] sin(l). The subtraction of observer velocity is essential. The formula concerns this declared orientation and frame; it must not be mixed with an unlabelled coordinate drawing having a different handedness.
The same interior ring crosses the ray twice
Intersect the l = 30° ray with the ring R = 5L0. Writing u = d/L0 gives R²/L0² = 64 + u² − 8√3 u. Setting this equal to 25 yields u² − 8√3 u + 39 = 0. Its positive roots are u = 4√3 − 3 and u = 4√3 + 3.
The near and far distances are therefore approximately 3.928203230L0 and 9.928203230L0. Both lie on the same R = 5L0 ring and both have v_los/V0 = (8/5 − 1)/2 = 0.3. Their full velocity vectors differ, but these particular line-of-sight components agree.
The closest point on the ray to the centre is the tangent point at d = 4√3L0 ≈ 6.928203230L0, with R = 4L0. Here the same speed field gives v_los/V0 = (8/4 − 1)/2 = 0.5. A tangent point is geometrically different from the two intersections with the larger ring.
Even perfect direction and line-of-sight velocity measurements thus need not select one distance. Real terminal-velocity methods additionally require gas to sample the tangent region and require treatment of line widths and noncircular motion. No observed terminal envelope or actual cloud distance is supplied by this experiment.
| Location | Observer distance d/L0 | Centre-based radius R/L0 | v_los/V0 |
|---|---|---|---|
| Near intersection | 3.928203230 | 5 | 0.3 |
| Tangent point | 6.928203230 | 4 | 0.5 |
| Far intersection | 9.928203230 | 5 | 0.3 |
One sightline, two distances, one radial velocity
Scroll sideways to see the full diagram. Its explanation is below.
A separate spherical model gives a restricted mass relation
For a circular test orbit in a Newtonian spherical mass distribution, radial acceleration balance gives v_c²/r = GM(<r)/r². Hence M(<r) = rv_c²/G, where M(<r) is mass enclosed by the orbit’s radius. This is not automatically total mass, and it is not an exact inversion for a flattened Galactic disk.
For an original finite-interval comparison, define M0 = V0²L0/G. A spherical model with flat v_c = V0 on 1 ≤ r/L0 ≤ 8 has M(<r)/M0 = r/L0 on that interval. At radii L0, 2L0 and 4L0 it therefore encloses M0, 2M0 and 4M0.
This finite spherical toy is consistent with a nonnegative inner mass distribution containing M0 within L0 and density V0²/(4πGr²) on the stated annulus. Its continuation inside and outside the interval is not specified. Extending a flat speed to infinity, or to a singular centre, is not part of the construction.
A separate fixed central point mass M0 gives v_c/V0 = (r/L0)⁻¹ᐟ². It is a comparison model, not simultaneously the source of the flat-speed field. The point-mass and distributed-mass predictions show why a centre does not imply that one central object controls every Galactic orbit.
| r/L0 | Flat-model v_c/V0 | Flat-model M(<r)/M0 | Fixed-point-mass v_c/V0 |
|---|---|---|---|
| 1 | 1 | 1 | 1 |
| 2 | 1 | 2 | 0.707106781 |
| 4 | 1 | 4 | 0.5 |
A dynamical discrepancy does not identify a microscopic component
In a Galactic mass model, stars, stellar remnants, gas and any additional gravitating component contribute to the potential. Estimating stellar mass from light requires a population and mass-to-light prescription. The spatial geometry matters because a disk and a sphere with similar enclosed luminosity do not generally give the same radial force.
For components contributing to the same radial force, their contributions add in v_c² through the potential gradient, rather than as a simple sum of circular speeds. A decomposition that looks plausible in a light image must still predict the measured motions within its assumptions.
Substantial outer speeds can challenge a model containing only centrally concentrated luminous mass. That is evidence about the gravitating distribution under the adopted gravity law and dynamical assumptions. It does not by itself determine a unique dark-matter density profile, identify a particle or establish every aspect of a gravity theory.
Combining distance, spectral motion, proper motion and independent population constraints can reduce ambiguity. The lesson’s two demonstrations retain their separate roles: the first exposes a projection ambiguity, and the second illustrates a conditional motion-to-mass relation. Neither is a fitted model of our Galaxy.
Worked examples
Solve the same-ring intersections
What distances along the supplied ray intersect R = 5L0, and what radial velocity does each have?
- The geometry gives u² − 8√3 u + 39 = 0 for u = d/L0.
- The roots are 4√3 − 3 and 4√3 + 3, approximately 3.928203230 and 9.928203230.
- Both have R/L0 = 5, so v_los/V0 = (8/5 − 1) sin(30°) = 0.3.
There are two distances with the same receding radial component 0.3V0. Additional information is needed to distinguish them.
Hold speed or enclosed mass fixed, with different consequences
At r = 4L0, how do the declared flat-speed spherical model and separate fixed point mass differ?
- For flat v_c = V0, the spherical relation gives M(<r) = 4M0.
- For a fixed point mass M0, the circular speed is V0/√4 = V0/2.
- The difference concerns the stipulated radial distribution of gravitating mass, not a new measured Galactic parameter.
The flat-speed model encloses 4M0 and has speed V0; the point-mass alternative encloses M0 and has speed V0/2.
Try the reasoning
Does one calibrated Doppler velocity determine a star’s full three-dimensional orbit?
Show the answer and reasoning
No.
It constrains one motion component; distances, transverse motion and a dynamical model supply further information.
In the supplied model, does l = 30° and v_los = 0.3V0 select only the near intersection?
Show the answer and reasoning
No.
The far R = 5L0 intersection has the same observer-relative radial component.
Is M(<r) = rv_c²/G an exact mass inversion for any flattened disk?
Show the answer and reasoning
No.
Its elementary enclosed-mass form assumes Newtonian gravity, spherical symmetry and circular motion.
Does a dynamical excess over a specified luminous-mass prediction identify the microscopic nature of an unseen component?
Show the answer and reasoning
No.
It constrains the gravitating model and does not uniquely identify a particle.
What to carry forward
- Velocity components require a declared observer and reference frame.
- One direction and radial velocity can admit two distances even in a perfect circular model.
- Circular motion constrains mass through physical assumptions; enclosed mass, total mass and particle identity are different inferences.
References
Teaching resources and research supporting this lesson’s explanations and examples.
- Astronomy 2e 25.3: The Mass of the GalaxyFraknoi, Morrison and Wolff / OpenStax, Rice University, USATextbook chapter
Jo Bovy / University of Toronto, Canada; Princeton University Press3 sources
- Dynamics and Astrophysics of Galaxies, Chapter 8 openingJo Bovy / University of Toronto, Canada; Princeton University PressTextbook chapter
- Dynamics and Astrophysics of Galaxies, 8.3: The kinematics of the Milky Way’s interstellar mediumJo Bovy / University of Toronto, Canada; Princeton University PressTextbook chapter
- Dynamics and Astrophysics of Galaxies, 8.2: Rotation curves of external galaxiesJo Bovy / University of Toronto, Canada; Princeton University PressTextbook chapter
- Dynamics and Astrophysics of Galaxies, A.2: Positions in the Milky WayJo Bovy / University of Toronto, Canada; Princeton University Press, 2026 online textbookTextbook chapter