REFERENCE LIBRARY

Learn how the major sky phenomena actually behave.

Each page separates observation clues from external evidence, explains common misidentifications and shows what would make an identification stronger.

FAST ATMOSPHERIC EVENTS

Meteors & Fireballs

How to recognize a meteor, when a bright event becomes a fireball, what fragmentation means, and what public sensor data can actually confirm.

Motion: Usually a rapid streakDuration: Fractions of a second to several secondsBlinking: No repeating strobe pattern
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STEADY ORBITAL LIGHTS

Satellites & the ISS

Why satellites move smoothly, why they fade suddenly, what makes the ISS unusually bright, and why an orbital catalog is not the same as an exact pass prediction.

Motion: Smooth, usually constantDuration: Tens of seconds to several minutesBlinking: Normally no navigation strobes
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LINES OF ORBITAL LIGHTS

Starlink Trains

How newly deployed satellites create the famous line-of-lights effect, what weakens a Starlink explanation, and why launch timing matters.

Pattern: Many points on one trackSpacing: Often regular after deploymentBlinking: Normally none
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AVIATION PATTERNS

Aircraft Lights at Night

How navigation lights, strobes, landing lights and perspective make aircraft appear stationary, multicolored or stranger than expected.

Motion: Steady or apparently stationary head-onBlinking: Common and often regularColors: Red, green, white
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HUMAN SPACEFLIGHT EFFECTS

Rocket Plumes & Space-Debris Reentry

Twilight plumes, spirals, fuel dumps and slow fragment trains can look extraordinary. Learn which timing and geometry clues matter.

Motion: Plumes expand; reentries translate slowlyDuration: Tens of seconds to many minutesFragments: Common in reentry
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GEOMAGNETIC SKY GLOW

Aurora

How auroral arcs, curtains and rays behave, how local probability differs from global Kp, and why cloud cover still matters.

Shape: Arcs, curtains, rays, diffuse glowColors: Green common; red/purple possibleDuration: Minutes to hours
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STATIONARY CELESTIAL LIGHTS

Bright Planets & Stars

Why Venus, Jupiter and bright stars trigger unusual-light reports, how scintillation changes color, and what stationary really tells you.

Motion: Effectively stationary over minutesBlinking: Planets usually steadier; stars can scintillateDuration: Minutes to hours
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SKY EFFECTS WITHOUT AN OBJECT

Atmospheric & Optical Effects

Cloud glow, halos, reflections, light pillars and perspective effects can create convincing objects that are really light interacting with atmosphere or glass.

Shape: Point, pillar, halo, glow or moving reflectionDuration: Seconds to hoursMovement: Often tied to cloud, observer or light source
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