Meteor Shower & Radiant
Meteoroid streams are distributed along parent comet orbits. When Earth intersects the stream, many particles enter the atmosphere on nearly parallel trajectories; perspective makes their apparent paths diverge from a point on the celestial sphere called the radiant. This page uses a toy star field, a fixed radiant marker, and streaks radiating outward to illustrate the geometry; the inset shows a highly simplified Sun–Earth orbit and a debris stream crossing, not a real ephemeris for a named shower.
Who it's for: Complements the comet orbit & tails page; introductory astronomy.
Key terms
- meteor shower
- radiant
- debris stream
- comet orbit
- perspective
How it works
**Meteor showers** occur when **Earth passes through** a **debris stream** left along a **comet’s orbit**. The particles move on **nearly parallel** paths; perspective makes them appear to diverge from a single point on the celestial sphere called the **radiant**. This page is **not** a real ephemeris for Perseids or Geminids — it shows the **geometry** (inset) and the **radiant + streaks** on a toy star field. **Rotation of Earth** and **latitude** change which radiants are up at night; here the radiant is fixed on the canvas for clarity.
Key equations
Frequently asked questions
- Why do meteors appear to radiate from one point?
- The meteoroids move on parallel trajectories; like parallel railroad tracks, their directions appear to converge at a vanishing point on the sky.
- Is the radiant position accurate for Perseids?
- No — the radiant is placed for visibility; real shower coordinates and peak dates come from IAU and observational data.
More from Astronomy & The Sky
Other simulators in this category — or see all 28.
Cosmological Expansion (FLRW)
a(t), z, χ and c/H vs time; flat Ω_m + Λ (toy ΛCDM).
Galaxy Rotation Curve
Keplerian decline vs flat v(r); toy halo slider (dark matter motivation).
Stellar Life Cycle
Cloud → MS → giant/SN → WD / NS / BH vs initial mass (schematic).
Exoplanet Radial Velocity
K from masses & P; sinusoidal V_r(t); M sin i.
Exoplanet Transit (light curve)
Uniform disk overlap; R_p/R_*; impact b; F(t) vs period.
Sphere of Influence (Hill)
r_H ≈ a (m/3M)^(1/3): schematic secondary orbit and Hill radius vs masses and a.