Vera RubinGalaxy Rotation? She Saw the Dark Side.
Vera Rubin Sticker – Galaxy Rotation? She Saw the Dark Side. | Physics Sticker
- Size
- 3" × 3"
- Surface
- White
- Made
- To order · shipping times
Couldn't load pickup availability
Details
Size3″ × 3″
3″ × 3″ kiss-cut sticker.
Mix & match pricing
- Pick any 3: $5.25 each (3 for $15.75)
- Pick any 5: $4.20 each (5 for $21.00)
Any stickers count. Discounts apply automatically at checkout.
Shipping
Free US shipping. Free international shipping with 4+ stickers, a sheet, or any tee.
Outside the US, orders of only 1–3 single stickers ship for $10.99.
∂ The physics
The sticker says She Saw the Dark Side. What she saw first was a flat line where a falling curve should have been.
Nearly all the solar system's mass sits in the Sun, so the farther out a planet is, the slower it moves: speed falls as one over the square root of distance. Neptune, thirty times farther out than Earth, travels at less than a fifth of Earth's speed. The first formula on this page turns that rule around: measure how fast something orbits at radius r, and you can work out how much mass lies inside r.
In 1965 Vera Rubin began work at the Carnegie Institution's Department of Terrestrial Magnetism in Washington, with the astronomer W. Kent Ford and his sensitive new spectrograph. They measured the Doppler shifts of glowing gas clouds across the Andromeda galaxy and published in 1970, and through the following decade Rubin and colleagues measured many more spiral galaxies. Far out, past most of the visible starlight, the speeds did not fall. They stayed flat. By the second formula, a flat speed means the enclosed mass keeps growing in proportion to radius, long after the light has thinned out. Most of each galaxy's mass is something that does not shine.
She was not first. Fritz Zwicky argued in the 1930s that the Coma cluster held far more mass than its galaxies showed, and radio astronomers were finding fast-moving hydrogen at the edges of galaxies in the same years Rubin worked. Her measurements across many galaxies are a large part of why astronomers came to accept it.
What dark matter is remains unknown. No particle has been detected directly, and a minority of physicists prefer to change the law of gravity instead.
Rubin clocked the edges. The dark side was what they told her.
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)
Field notes
View all-
Thermal Mirages Explained: Optical Magic from H...
Hey there, curious minds! Welcome back to Pixelated Physics, your favorite spot to decode the universe’s coolest tricks. Today, let’s talk about something you might see on a hot day: thermal...
Thermal Mirages Explained: Optical Magic from H...
Hey there, curious minds! Welcome back to Pixelated Physics, your favorite spot to decode the universe’s coolest tricks. Today, let’s talk about something you might see on a hot day: thermal...
-
Beta Decay Unveiled: Dance of the Weak Nuclear ...
Beta Decay Unveiled: Dance of the Weak Nuclear Force Welcome back, physics fans, to Pixelated Physics, your favorite destination for quantum quirks and cosmic mysteries! Today’s topic? The wildly fascinating...
Beta Decay Unveiled: Dance of the Weak Nuclear ...
Beta Decay Unveiled: Dance of the Weak Nuclear Force Welcome back, physics fans, to Pixelated Physics, your favorite destination for quantum quirks and cosmic mysteries! Today’s topic? The wildly fascinating...
-
Particle Annihilation Explained: When Matter Me...
Welcome, curious minds, to another electrifying exploration brought to you by Pixelated Physics! Today, we're diving deep into the astonishing quantum event known as particle annihilation. Hold onto your pixels, because...
Particle Annihilation Explained: When Matter Me...
Welcome, curious minds, to another electrifying exploration brought to you by Pixelated Physics! Today, we're diving deep into the astonishing quantum event known as particle annihilation. Hold onto your pixels, because...