✨ Caelus • Lunar Eclipse on May 6, 2069

September 09, 2026 17:05:58 UTC+02:00 [48.85° N, 2.35° E]

‹ All eclipses in 2069

Total Lunar Eclipse

May 6, 2069

Umbra Penumbra Moon

Greatest Eclipse

11:08

09:08 UTC

Duration

6h 8m

first to last penumbral contact

Deepest Phase

1h 24m

Totality

Umbral Magnitude

1.323

of the diameter in the umbra

Penumbral Magnitude

2.396

of the diameter in the penumbra

Gamma

0.272

1 733 km north of the axis

🕐 Contacts

Times in Europe/Paris, with UTC underneath.

First penumbral contact (P1)

The Moon touches Earth's penumbra and starts to dim.

08:04

06:04 UTC

PA 110.8°

-16.7° alt · 263° az
First umbral contact (U1)

The Moon reaches the umbra and the partial eclipse begins.

09:15

07:15 UTC

PA 116.8°

-28.0° alt · 276° az
Second umbral contact (U2)

The Moon is entirely inside the umbra and totality begins.

10:26

08:26 UTC

PA 318.2°

-39.0° alt · 291° az
Greatest eclipse

The Moon's centre is least distant from the axis of Earth's shadow.

11:08

09:08 UTC

PA 10.9°

-45.0° alt · 301° az
Third umbral contact (U3)

The Moon starts leaving the umbra and totality ends.

11:50

09:50 UTC

PA 63.5°

-50.4° alt · 313° az
Fourth umbral contact (U4)

The Moon leaves the umbra and the partial eclipse ends.

13:01

11:01 UTC

PA 265.0°

-56.8° alt · 338° az
Last penumbral contact (P4)

The Moon leaves Earth's penumbra and the eclipse ends.

14:12

12:12 UTC

PA 270.9°

-58.2° alt · 9° 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 below the horizon for the whole eclipse.

Penumbral phase: Not visible
Partial phase: Not visible
Totality: Not visible

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 6h 8m

Partial phase 3h 46m

Totality 1h 24m

🌍 About This Eclipse

A total lunar eclipse occurs when the Earth passes directly between the Sun and the Moon, causing the Earth's shadow to completely cover the Moon. During a total lunar eclipse, the Moon can take on a reddish color due to the scattering of sunlight through the Earth's atmosphere, often referred to as a "Blood Moon."

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.