ScienceExplain Like I'm 5Intermediate
Reading the Open Sky, a free science course on Tomo

Reading the Open Sky

Like Duolingo, but for Reading the Open Sky. Tomo turns the whole topic into a game you play five minutes a day, until it actually sticks.

For the part of you with thirty open tabs that never became anything.

91 levels across 8 sections, about 182 minutes end to end, roughly 36 days at five minutes a day. It moves through Daytime Light and Weather Signals; Optical Wonders of Ice, Water, and Air; The Boundary of Night: Twilight and the Upper Atmosphere; The Moving Sky: Meteors, Satellites, and Space Dust; Our Nearest Neighbors: The Moon and Solar System; The Solar Stage: Daylight Astronomy; The Deep Night: Stars, Clusters, and the Galaxy; and Atmospheric Seeing and Perceptual Illusions. It assumes you already know the basics.

91 bite-size levelsAbout 5 minutes each

Free forever · No credit card · iPhone & Android

Skyler the Skylark, the guide who teaches the Reading the Open Sky course
Reading the Open Sky
with Skyler the Skylark
91
Levels
8
Sections
5
Min/day
What you'll learn

Key ideas in Reading the Open Sky

  • Rayleigh scattering scales inversely with the fourth power of wavelength, scattering blue far more than red
  • Short blue wavelengths scatter diffuse light across the sky dome
  • Long slant paths through the atmosphere strip out blues, leaving direct red wavelengths to reach your eyes
  • Aerosols and water droplets are larger than light wavelengths, triggering Mie scattering
  • Mie scattering is largely wavelength-independent, scattering all colors equally to produce white glare
  • Mie scattering strongly focuses light forward, producing a halo around the Sun called an aureole
  • Rayleigh scattering polarizes sunlight most strongly at an angle exactly 90 degrees from the Sun
  • Photographers use the thumb-and-index-finger rule to trace the high-polarization band in the sky
  • Looking directly toward or away from the Sun yields zero net polarization
  • High optical air mass at low solar angles purges virtually all short blue and green wavelengths
  • Fine volcanic sulfate aerosols or stratospheric wildfire smoke dramatically boost twilight coloration
  • Earth's dark shadow rises directly above the eastern horizon as a cool, slate-blue band
  • The Belt of Venus sits immediately above Earth's shadow as a warm, pinkish-orange glow
  • The unshadowed upper atmosphere above the Belt of Venus remains pale ambient blue
  • The vertical sequence of visual atmospheric layers visible on the anti-solar horizon immediately after sunset
  • A wide spread between temperature and dew point forces air to rise higher to saturate.
Why not just Google it

You've tried the other tabs

Wikipedia

Thirty open tabs. Four facts you actually kept.

YouTube

You watched. You nodded. By Sunday it was gone.

ChatGPT

One answer, then back to scrolling.

Online courses

Eight weeks. You meant to finish. You didn't.

Tomo gives Reading the Open Sky the Duolingo treatment: levels, streaks, and quick quizzes that test what you just learned. That game loop is what the tabs above never had, so it's the one you actually finish.

Try a question

Here's what playing it feels like

A real question from this course. Take your best guess.

Why the Sky Changes Color

When you look up at noon on a clear day, why does the entire sky dome look bright blue?

Get it right to open this lesson and 90 more in the app.

Course map

Where Reading the Open Sky takes you

Decode every natural and artificial spectacle visible above your head. Explore the atmospheric optics, orbital mechanics, solar dynamics, and stellar astrophysics that shape daytime, twilight, and nighttime skies.

  1. 1

    Daytime Light and Weather Signals

    • The Sky's Palette: Rayleigh and Mie Scattering
    • Decoding Cloud Geometry and Stratification
    • Solar Shadows, Sundials, and the Equation of Time
  2. 2

    Optical Wonders of Ice, Water, and Air

    • Rainbow Physics: Beyond the Primary Arc
    • Ice Crystal Geometry: Halos, Sundogs, and Pillars
    • Atmospheric Refraction: Mirages and the Green Flash
    • Diffraction Phenomena: Coronas, Glories, and Iridescence
  3. 3

    The Boundary of Night: Twilight and the Upper Atmosphere

    • The Stages of Twilight and Sky Shadows
    • Mesospheric and Ionospheric Light: Auroras and Airglow
    • High-Altitude Transients: Noctilucent Clouds and Plumes
  4. 4

    The Moving Sky: Meteors, Satellites, and Space Dust

    • Spotting Artificial Satellites and Orbital Passes
    • Meteor Showers, Sporadics, and Bolides
    • Interplanetary Dust: Zodiacal Light and Gegenschein
  5. 5

    Our Nearest Neighbors: The Moon and Solar System

    • Decoding the Moon: Phases, Libration, and Earthshine
    • Tracking Planetary Wandering and Retrograde Loops
    • Occultations, Conjunctions, and Planetary Transits
  6. 6

    The Solar Stage: Daylight Astronomy

    • Solar Surface Features: Sunspots and Limb Darkening
    • Total and Annular Eclipses: Shadow Bands to Totality
  7. 7

    The Deep Night: Stars, Clusters, and the Galaxy

    • Naked-Eye Stellar Astrophysics: Temperature and Color
    • Unresolved Light: The Milky Way, Clusters, and Nebulae
    • Variable Stars and Transient Starlight
  8. 8

    Atmospheric Seeing and Perceptual Illusions

    • Atmospheric Scintillation and Seeing Conditions
    • Sky Illusions: The Moon Illusion and Visual Deceptions

8 sections · 23 units · 91 levels. Built to play, not to enroll.

How it's taught

You pick the voice

This course
Explain Like I'm 5

Reading the Open Sky is taught in the Explain Like I'm 5 style: no big words. promise.. Want a different feel? In the app you can spin up the same topic in any of Tomo's teaching styles. Same facts, totally different vibe.

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Start Reading the Open Sky today.

Download Tomo, search Reading the Open Sky, and play your first lesson in under a minute.