Eclipse Geometry: Shadows in Space

EarthSky • Both • 12 min

Name: ________________________________ Section: __________ Date: __________

Station: __________ Group members: ________________________________________________

Goal: Use the demo to make a claim supported by (1) at least one number/readout and (2) at least one sanity check.

Station card: Eclipse Geometry (6–8 minutes) Demo setup: Use New Moon and Full Moon buttons; drag near/far from nodes.
Tip: Click Station Mode to add snapshot rows and print/copy your table.

Your station artifact (fill in):

  1. Control(s): phase angle Δ\Delta, node proximity (nearest-node distance or ∣β∣|\beta|), tilt ii
  2. Observable(s): eclipse type (none/partial/central; penumbral/umbral/total)
  3. Governing relationship: write “eclipse requires syzygy + small ∣β∣|\beta|” in words
  4. Sanity check: what happens when i=0∘i=0^\circ?
  5. Connection sentence: “This connects to angular size because…”

Word bank + sanity checks Word bank:

  • Syzygy: Sun–Earth–Moon aligned (New Moon for solar eclipses; Full Moon for lunar eclipses).
  • Node: where the Moon’s orbit crosses the ecliptic plane.
  • Ecliptic latitude β\beta (degrees): how far the Moon is above/below the ecliptic plane.
  • Inclination ii (degrees): tilt of the Moon’s orbit relative to the ecliptic plane.
  • Near a node: small ∣β∣|\beta| (and/or small “nearest node” distance) at syzygy.

Sanity checks:

  • You need BOTH: (1) New/Full Moon and (2) near a node (small ∣β∣|\beta|). One condition alone is not enough.
  • If i=0∘i=0^\circ, then β=0∘\beta=0^\circ always → eclipses happen every month.
  • Changing Earth–Moon distance can change whether a solar eclipse is total or annular (size matters too).