Article Outline: World’s Largest Telescopes

Metadata

  • Date: 10th December 2025
  • Title: Research with the World’s Largest Telescopes
  • Speaker: Dr Katharine Johnston

Structure (Condensed ~450 words)

1. Hook/Introduction

  • First black hole image (2019)
  • Answer: Earth-sized telescope

2. Why Size Matters

  • Resolution = lambda/D
  • Sensitivity: bigger bucket, more photons
  • Radio telescopes larger due to longer wavelengths

3. Seeing Through Dust

  • Dust blocks visible light like fog
  • Longer wavelengths penetrate (Wi-Fi analogy)
  • Submillimetre sky as “treasure trove”

4. Interferometry: Combining Telescopes

  • ALMA: 66 antennas at 5,000m
  • Resolution from baseline, not dish size
  • Earth rotation fills effective aperture

5. The Event Horizon Telescope

  • Global baselines: 12,000 km effective diameter
  • 20 microarcseconds resolution
  • Data shipped on hard drives

6. Seeing Black Holes

  • M87 (2019), Sagittarius A* (2022)
  • Tests of general relativity: shadows match predictions

7. Take-Home Message

  • Larger = sharper and more sensitive
  • Longer wavelengths see through dust
  • Interferometry creates planet-sized instruments

External Sources to Include

  1. Reference: ESO website on VLT/ALMA specifications
  2. Quote: Scientific statement on interferometry capabilities

Context Points

  • Societal: Understanding cosmic origins, technology development
  • Research: Black hole physics, star formation, testing general relativity

Style Notes

  • Use relatable comparisons (Wi-Fi through walls)
  • Explain interferometry simply (combining signals, not complex physics)
  • Highlight the human achievement (telescope the size of Earth)
  • Include specific results (black hole images)