Telescope Resolution: Sharper Eyes

Telescopes • Both • 10 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: Telescope Resolution (6–8 minutes) Artifact: a “can this telescope resolve it?” card.

Choose:

  • one telescope preset,
  • one wavelength (UV/Visible/Near-IR/Mid-IR/Radio),
  • one binary separation that is “marginal.”

Record:

  • the resolution (arcsec),
  • the resolved/marginal/unresolved status,
  • one sentence explaining why (link to λ\lambda and DD, optionally atmosphere).

Word bank + sanity checks Word bank:

  • Resolution (diffraction limit): the smallest angular separation a telescope can distinguish.
  • Aperture DD: bigger DD → better (smaller) diffraction limit.
  • Wavelength λ\lambda: longer λ\lambda → worse (larger) diffraction limit.
  • Seeing (atmosphere): turbulence can blur images beyond the diffraction limit; AO can partially correct.

Key relationship (diffraction-limited scaling):

θ∝λD\theta \propto \frac{\lambda}{D}

Sanity checks:

  • Increasing DD should decrease the resolution number (better detail).
  • Increasing λ\lambda should increase the resolution number (worse detail).
  • With “Include Atmosphere” on, the limit may stop improving unless AO is enabled.