Partial Lunar Eclipse of July 6, 2028
- Type
- Partial lunar eclipse
- Peak (UTC)
- July 6, 2028, 18:19 UTC
- Moon covered
- 33% of the Moon's disk inside the umbra at maximum
- Umbral phase lasts
- about 2 hours 25 minutes
- Saros series
- 120
Best from Africa, Europe, Asia and Australia; the Americas largely miss it.
A moderate partial eclipse: at maximum, roughly the northern third of the Moon sits inside Earth's umbra.
Global timeline (UTC)
A lunar eclipse happens at the same instant for everyone; only your clock and your Moon's position differ. Convert from UTC, or use the location panel below to check whether the Moon is up at each stage for you.
| Stage | Time |
|---|---|
| Penumbral eclipse begins | 15:43 UTC |
| Partial (umbral) eclipse begins | 17:08 UTC |
| Maximum eclipse | 18:19 UTC |
| Partial (umbral) eclipse ends | 19:30 UTC |
| Penumbral eclipse ends | 20:55 UTC |
What you will see from your location
Enter a location (or use your device's) and we check whether the Moon is above your horizon at each stage of the eclipse, all in your browser.
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What a partial lunar eclipse is
In a partial lunar eclipse only part of the full Moon passes through Earth's umbra, the dark core of our planet's shadow. The shadowed portion darkens dramatically, often with a reddish cast, while the rest of the Moon stays bright. Lunar eclipses are visible from the whole night side of Earth and are completely safe to watch with the naked eye.
Frequently asked questions
When is the partial lunar eclipse of July 2028?
Greatest eclipse comes on July 6, 2028 at 18:19 UTC. What you see, and when, depends on where you stand; use the location panel on this page for your own local timeline.
Where will the July 2028 lunar eclipse be visible?
Best from Africa, Europe, Asia and Australia; the Americas largely miss it.
Is it safe to watch a lunar eclipse?
Completely. A lunar eclipse is just the full Moon passing through Earth's shadow; it needs no filters or equipment. Binoculars simply make it better.
What is a Saros series?
Eclipses repeat in families called Saros series: 6,585.3 days (about 18 years 11 days) after any eclipse, the Sun, Moon and lunar nodes return to nearly the same geometry and produce a near-copy shifted a third of the way around Earth. This eclipse belongs to Saros series 120. Our Saros cycle profile explains the whole mechanism.
Keep exploring: the Eclipse Explorer for any date and location, our Saros cycle profile for why eclipses repeat, and how eclipses work from first principles.