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Vera Rubin Sticker
Galaxy Rotation? She Saw the Dark Side. | Physics
The outer stars of galaxies move too fast for what we can see. Vera Rubin and Kent Ford’s 1970s galaxy rotation curves showed outer stars orbit too fast for the visible mass: key dark matter evidence. A pixel-art portrait on a 3" × 3" sticker; the physics panel below has the equation, every symbol and the sources.
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Details
Size3″ × 3″
3″ × 3″ kiss-cut sticker.
Shipping
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Returns & replacements21 days
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The physics
If most of a galaxy's mass were in its bright centre, stars far out would orbit more slowly. Vera Rubin found the speeds stay roughly constant far out, which means the enclosed mass keeps growing with radius: unseen matter.
Equations
| Symbol | Meaning | Unit |
|---|---|---|
| \(v(r)\) | circular orbital speed | \(\mathrm{m/s}\) |
| \(M(r)\) | enclosed mass | \(\mathrm{kg}\) |
| \(r\) | radius | \(\mathrm{m}\) |
| \(G\) | gravitational constant | \(\mathrm{m³·kg⁻¹·s⁻²}\) |
Sources
- Rubin & Ford (1970) Rotation of the Andromeda Nebula, ApJ 159, 379 (opens in a new tab)
- Zwicky (1937) On the Masses of Nebulae and of Clusters of Nebulae, ApJ 86, 217 (opens in a new tab)
- Encyclopaedia Britannica — Vera Rubin (opens in a new tab)
- Encyclopaedia Britannica — Dark matter (opens in a new tab)
- PDG 2024 review — Dark matter (opens in a new tab)
Source Rubin, V. C.; Ford, W. K., Jr. (1970). Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions. The Astrophysical Journal 159, 379.doi.org/10.1086/150317 (opens in a new tab)