✨ Caelus • Lunar Eclipse on April 11, 1922

September 09, 2026 17:07:34 UTC+02:00 [48.85° N, 2.35° E]

‹ All eclipses in 1922
The Moon in Earth's shadow Penumbral Lunar Eclipse: at greatest eclipse the Moon's centre passes 4.12 Moon radii north of the axis of Earth's shadow, with none of its diameter inside the umbra and 78% inside the penumbra.

Penumbral Lunar Eclipse

April 11, 1922
Umbra Penumbra Moon
Greatest Eclipse
21:31
20:31 UTC
Duration
3h 43m
first to last penumbral contact
Deepest Phase
3h 43m
Penumbral phase
Umbral Magnitude
-0.186
of the diameter in the umbra
Penumbral Magnitude
0.781
of the diameter in the penumbra
Gamma
1.123
7 162 km north of the axis

🕐 Contacts

Times in Europe/Paris, with UTC underneath.

  1. First penumbral contact (P1)
    The Moon touches Earth's penumbra and starts to dim.
    19:40
    18:40 UTC
    PA 152.9°
    2.2° alt · 104° az
  2. Greatest eclipse
    The Moon's centre is least distant from the axis of Earth's shadow.
    21:31
    20:31 UTC
    PA 16.5°
    17.9° alt · 126° az
  3. Last penumbral contact (P4)
    The Moon leaves Earth's penumbra and the eclipse ends.
    23:23
    22:23 UTC
    PA 240.0°
    29.1° alt · 153° az

The position angle is measured on the Moon's limb from celestial north through east, the convention IMCCE and NASA publish, so these values can be compared with a published table directly.

👁 Visibility

From your location.

The Moon is up from the first to the last contact.
Penumbral phase
Entirely visible
Moon above the horizon
19:40 – 23:23

A lunar eclipse happens at the same moment everywhere. All that changes from place to place is whether the Moon is above the horizon.

⏳ Durations

Penumbral phase 3h 43m

🌍 About This Eclipse

A penumbral lunar eclipse occurs when the Moon passes through the Earth's penumbral shadow. This type of eclipse is subtle and often hard to observe, as the Moon only slightly darkens. It is not as dramatic as a partial or total lunar eclipse, but it is still an interesting astronomical event.

A lunar eclipse is a geocentric event. The contacts and magnitudes on this page are the same for every observer who can see the Moon at that moment.