Lunar Eclipses3.9 - Understand the appearance of the Moon during partial and total lunar eclipses, including the terms first, second, third and fourth umbral contact
Lunar eclipses take place when the Moon enters Earth's shadow. First to last contact can last several hours however totality lasts up to 1 hour 42 minutes. This is larger than a solar eclipse because the Earth is larger than the Moon. Totality can be observed by most observers on the night hemisphere of the Earth, not necessarily along a line of totality like a solar eclipse.
A lunar eclipse only takes place during a full Moon when the Moon is on the opposite side of the Earth from the Sun.
Total Lunar Eclipse
The Moon enters Earth's penumbra and a partial lunar eclipse occurs. The moon may appear darker or greyer at this point.
The Moon moves into the Earth's umbra. Sunlight passing through Earth's atmosphere refracts (bends) red light onto the Moon's surface. The colour depends on atmospheric conditions on Earth. Other observed colours are copper, orange, or dull burgundy.
The Moon moves out of the Earth's umbra.
The Moon moves out of the Earth's penumbra.
PARTIAL ECLIPSEA partial lunar eclipse occurs when the Earth's shadow intrudes into the disc of the Moon but does not block it entirely as in a total lunar eclipse. Sometimes partial eclipses happen at the same time as total lunar eclipses but are partial to an observer due to the rotation of the Earth and the time of moonrise and moonset.
- Takes place over hours
- Visible from hemisphere facing moon
- Colour caused by refraction of Earth's atmosphere
- Draw a diagram with labels of a Lunar eclipse.
- Write down times and appearance of the Moon.