Many observers searched the skies in 2017 for the next blood moon, a dramatic total lunar eclipse that turns the moon a deep red. Understanding the exact timing and visibility windows helps photographers, astronomy clubs, and casual skywatchers plan ahead.
Below is a structured overview of the key dates and regional visibility for the 2017 total lunar eclipse events, followed by dedicated sections for timing, visibility, science, and photography tips.
| Region | Partial Eclipse Start | Total Eclipse Start | Maximum Eclipse | Total Eclipse End | Partial Eclipse End |
|---|---|---|---|---|---|
| North America | 08:07 UTC | 09:41 UTC | 10:04 UTC | 10:27 UTC | 12:02 UTC |
| Europe | 10:07 UTC | 11:41 UTC | 12:04 UTC | 12:27 UTC | 14:02 UTC |
| Asia | 15:50 UTC | 17:24 UTC | 17:47 UTC | 18:11 UTC | 19:44 UTC |
| Australia | 19:25 UTC | 20:30 UTC | 21:04 UTC | 21:37 UTC | 22:51 UTC |
Total Lunar Eclipse Timing in 2017
The first total lunar eclipse of 2017 occurred on 10 August, with the total phase centered near 12:04 UTC. The moon passed deeply into Earth’s umbra, producing a vivid red hue that varied depending on atmospheric clarity and lunar position. Unlike solar eclipses, this event was visible from any location on the night side of Earth where the moon was above the horizon.
Regional Visibility and Viewing Windows
Skywatchers in North America enjoyed the most favorable conditions, with the entire eclipse sequence above the horizon before dawn. European observers saw the latter half of the eclipse during the early morning hours, while Asia experienced the total phase at dusk. Australia witnessed the moon high in the sky as it turned red, offering excellent photographic opportunities.
Scientific Explanation of a Blood Moon
Why the Moon Turns Red
During a total lunar eclipse, sunlight filters through Earth’s atmosphere, bending toward the shadowed surface and scattering shorter blue wavelengths. The longer red wavelengths illuminate the lunar surface, creating the blood moon appearance, which can shift in shade based on dust and cloud conditions.
Orbital Mechanics and Ecliptic Geometry
A lunar eclipse requires the sun, Earth, and moon to align closely along the ecliptic plane. In 2017, the moon’s orbit intersected Earth’s shadow at a shallow angle, extending the duration of the total phase and intensifying the reddish color across multiple regions.
Photography and Observation Tips
- Use a tripod to keep long exposure shots sharp during the dim total phase.
- Balance ISO settings to capture red hues without introducing too much noise.
- Include foreground elements such as trees or cityscapes to add scale to wide-angle shots.
- Monitor weather forecasts and choose locations with minimal light pollution for best results.
Observing Practices and Future Planning
Tracking eclipse cycles encourages consistent sky observation and helps enthusiasts coordinate public outreach events. Planning for future blood moons involves checking lunar eclipse seasons, which occur roughly every six months, and aligning personal schedules with global visibility maps.
FAQ
Reader questions
When did the next blood moon occur after August 2017?
The next total lunar eclipse took place on 31 January 2018, followed by another on 31 July 2018, making 2017 a transition year with fewer total events.
Was the 10 August 2017 eclipse visible worldwide?
No, visibility depended on local horizon conditions and whether the moon was above the horizon at the time of the eclipse for each region.
How long did the total phase last on 10 August 2017?
The total phase lasted approximately 7 minutes, with the moon fully immersed in Earth’s umbra between 09:41 UTC and 10:27 UTC.
What equipment is best for photographing a blood moon in 2017?
A DSLR or mirrorless camera with a telephoto lens, a sturdy tripod, and a remote shutter release produces the clearest images, especially when paired with manual exposure settings.