Why don't solar and lunar eclipses happen every month?
Two orders of bodies, umbra and penumbra, orbital nodes and a lunar-shadow model: why new and full Moon are not enough for an eclipse, and how to observe safely.
Articles: 3
Two orders of bodies, umbra and penumbra, orbital nodes and a lunar-shadow model: why new and full Moon are not enough for an eclipse, and how to observe safely.
Why we see crescents, half a disk and full Moon: explore lunar phases with an adjustable diagram and a lamp experiment, and test the shadow explanation.
Where sunlight gets its energy, why dark lunar rock looks bright, and how the Moon emits invisible thermal radiation of its own.