A lunar eclipse occurs when the Moon passes through the Earthβs shadow, which consists of two concentric parts: the dark umbra and the lighter penumbra. The geometry of the encounter determines whether the eclipse is total, partial, or merely penumbral.
The key parameter is the Moonβs offset distance (d) from the central axis of the Earthβs shadow at the lunar distance. By comparing this offset to the radii of the umbra (Ru) and penumbra (Rp), we can classify the eclipse type.
If the Moonβs center stays completely inside the umbra (d β€ Ru), the eclipse is total; if it lies between the umbra and penumbra (Ru < d β€ Rp), the eclipse is partial; otherwise (d > Rp) only a faint penumbral shading occurs.
R_{u} = Umbra radius at lunar distance (km)
R_{p} = Penumbra radius at lunar distance (km)
What are the three types of lunar eclipses?
How does the calculator determine the eclipse type?
What does the term 'umbra' mean in a lunar eclipse?
Can you explain what 'penumbra' refers to in a lunar eclipse?
What factors affect the visibility of a lunar eclipse?
How often do lunar eclipses occur?
Is it possible for the Moon to pass through both umbra and penumbra during an eclipse?
Results are for informational purposes only and do not constitute professional advice.
