HOTNASA EclipseMarch 2026๐ŸŒ GLOBALScience
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March 2026 Blood Moon: Last Total Lunar Eclipse Visible from the US Until 2029

The March 3, 2026 total lunar eclipse turned the Moon blood-red for 58 minutes, visible across Asia, Australia, and the Americas. With the next total lunar eclipse not until December 31, 2028, this calculator helps you plan for upcoming eclipses by computing exact local timing, Moon altitude, Danjon brightness prediction, visibility score, and photography exposure settings for any location on Earth.

Concept Fundamentals
58 min
Totality Duration
Mar 2026
1.151
Umbral Magnitude
Saros 141
Dec 2028
Next Total
~3 years
384,400 km
Moon Distance
avg

Ready to run the numbers?

Why: With the last total lunar eclipse from US soil until 2029 just occurred, millions are searching for when the next blood moon is and how to view it. This calculator provides precise local timing, visibility predictions, and photography settings.

How: Uses NASA/EclipseWise contact times with timezone conversion, astronomical altitude/azimuth calculations, Danjon scale atmospheric brightness modeling, and camera field-of-view geometry to produce location-specific eclipse viewing plans.

Exact local timing for all 7 eclipse contact phasesMoon altitude and direction at mid-eclipse for your location

Run the calculator when you are ready.

Calculate Eclipse TimingUse the calculator below to see how this story affects you personally

Eclipse & Location

Photography Settings

lunar_eclipse_analysis.sh
CALCULATED
$ analyze_lunar_eclipse --eclipse=2026-03-03 --lat=40.71 --lon=-74.01 --tz=UTC-5
Eclipse Type
Total Lunar Eclipse
Umbral Magnitude
1.151
Totality Duration
58 min
Visibility Score
95%
Moon Altitude
56.3ยฐ
Moon Azimuth
193.4ยฐ
Danjon Scale
L3
Brick-red eclipse with bright yellow-orange rim
Next Total Eclipse
Dec 31, 2028 (Saros 113)
Eclipse Phase Timeline (Local Time)
P1
03:50
Penumbral start
U1
04:55
Partial start
U2
06:04
Totality start
MID
06:33
Greatest eclipse
U3
07:02
Totality end
U4
08:11
Partial end
P4
09:17
Penumbral end
Photography Settings (for 300mm f/5.6)
ISO
400-800
Shutter
1/4 - 1s
Aperture
f/4 - f/5.6
Moon in Frame
8%
Saros 141 โ€” repeats every 18.03 years (6585 days)
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Eclipse Phase Durations

Moon Altitude During Eclipse

Moon below 0ยฐ = below horizon. Red dot = mid-eclipse. Higher altitude = better viewing.

Upcoming Eclipse Types (2026-2030)

Umbral Magnitude Comparison

Red = selected eclipse. Orange = total. Blue = partial. Gray = penumbral. Magnitude >1.0 = total eclipse.

For educational and informational purposes only. Verify with a qualified professional.

Answer Capsule: A blood moon occurs during a total lunar eclipse when Earth's atmosphere refracts red light onto the Moon. The March 3, 2026 eclipse had 58 minutes of totality with magnitude 1.151. Next total: Dec 31, 2028. No special glasses needed โ€” lunar eclipses are safe to watch with the naked eye.

Key Takeaways

  • โ€ข In India, a lunar eclipse is called Chandra Grahan โ€” traditionally observed with rituals and fasting practices
  • โ€ข Umbral magnitude >1.0 means total eclipse โ€” the higher the magnitude, the deeper the Moon enters Earth's umbra
  • โ€ข The Danjon scale rates eclipse brightness from L0 (nearly invisible) to L4 (bright copper-orange)
  • โ€ข Unlike solar eclipses, lunar eclipses are completely safe to view without any eye protection
  • โ€ข The March 2026 blood moon was the last total lunar eclipse visible from the US until December 31, 2028

What Are the Types of Lunar Eclipses?

๐Ÿ”ด Total Lunar Eclipse

Moon fully enters Earth's umbra. Turns blood-red from refracted sunlight. Totality lasts 30-100 minutes. Magnitude >1.0. Most spectacular type.

๐ŸŸ  Partial Lunar Eclipse

Moon partially enters umbra. Part appears dark/reddish while the rest stays bright. Magnitude 0.0-1.0. Visible worldwide where Moon is up.

โšช Penumbral Lunar Eclipse

Moon passes through Earth's penumbral shadow only. Subtle darkening โ€” often imperceptible to casual observers. Most common but least dramatic.

The Danjon Luminosity Scale

L0
Very Dark
Moon almost invisible at mid-totality
L1
Dark Gray/Brown
Details barely discernible, dark coloring
L2
Deep Red/Rust
Dark red center, brighter outer umbral edge
L3
Brick Red
Bright rim, yellow-orange edge to umbra
L4
Copper/Orange
Very bright with blue rim โ€” clear atmosphere

Scale created by Andrรฉ Danjon in 1921. Volcanic eruptions (e.g. Pinatubo 1991) can darken eclipses to L0 for years.

Why Does the Moon Turn Red?

Rayleigh Scattering

Sunlight passing through Earth's atmosphere bends around our planet and onto the Moon. Blue wavelengths (~450nm) scatter away, while red wavelengths (~620-750nm) refract through โ€” the same physics that makes sunsets red. During totality, the Moon effectively sees every sunset and sunrise on Earth simultaneously.

Umbra and Penumbra

Earth casts two shadows: the dark inner umbra (no direct sunlight reaches the Moon) and the lighter outer penumbra (partial sunlight). The umbra cone at the Moon's distance is roughly 2.65 times the Moon's diameter, which is why totality can last over an hour.

Magnitude and Gamma

Umbral magnitude measures how deeply the Moon enters the umbra โ€” values above 1.0 indicate totality. Gamma measures the closest approach of the Moon's center to the shadow axis. Lower absolute gamma = deeper, longer totality.

Did You Know?

๐ŸŒUnlike solar eclipses, a lunar eclipse is visible from the entire night side of Earth โ€” over 3.5 billion people can see each oneSource: NASA
๐Ÿ”ดThe term "blood moon" became popular after a 2013 book by John Hagee. Astronomers call it a total lunar eclipseSource: Sky & Telescope
๐ŸŒ‹After the 1991 Mt. Pinatubo eruption, the December 1992 eclipse was rated Danjon L0 โ€” the Moon was nearly invisibleSource: Wikipedia/Danjon
๐Ÿ“…A tetrad (4 total lunar eclipses in a row with no partials between) last occurred 2014-2015. The next is in 2032-2033Source: NASA Eclipse
โฑ๏ธThe longest possible totality is ~107 minutes. The July 27, 2018 eclipse had 103 minutes โ€” near the theoretical maximumSource: EclipseWise
๐Ÿ”ญColumbus used a predicted lunar eclipse on Feb 29, 1504 to intimidate Jamaican natives into providing food for his stranded crewSource: History.com

Frequently Asked Questions

What causes a blood moon during a lunar eclipse?

During totality, sunlight refracts through Earth's atmosphere. Blue light scatters away (Rayleigh scattering) while red/orange wavelengths bend around Earth onto the Moon's surface, producing the characteristic blood-red color โ€” the same physics behind red sunsets.

When is the next total lunar eclipse visible from North America?

The March 3, 2026 total lunar eclipse was the last visible from the US until December 31, 2028. The August 28, 2026 partial eclipse is visible from the Americas, followed by a January 12, 2028 partial eclipse.

Do I need special glasses to watch a lunar eclipse?

No. Unlike solar eclipses, lunar eclipses are completely safe to watch with the naked eye, binoculars, or a telescope. The Moon reflects only a tiny fraction of sunlight, so there is zero risk of eye damage during any phase of a lunar eclipse.

How long does a total lunar eclipse last?

Totality typically lasts 30-100 minutes, while the entire event from first penumbral contact to last can span 5-6 hours. The March 2026 blood moon had ~58 minutes of totality. The December 2029 eclipse will have ~84 minutes of totality.

What is the Danjon scale for lunar eclipses?

French astronomer Andrรฉ Danjon created a 5-point brightness scale (L0-L4) for total lunar eclipses. L0 is nearly invisible (major volcanic eruptions darken the atmosphere), L4 is bright copper-orange with a blue rim. Most eclipses rate L2-L3.

How do I photograph a blood moon?

During totality use ISO 800-3200, shutter speed 0.5-4 seconds, aperture f/4-f/5.6, and a 200-300mm+ telephoto lens on a sturdy tripod. During partial phases drop to ISO 100-400 and 1/125-1/250s. Shoot RAW and bracket exposures.

Blood Moon Photography Guide

๐Ÿ“ท Partial Phases

ISO 200-400 | 1/60-1/125s | f/8 | Use manual focus on the Moon's terminator for sharpest results.

๐Ÿ”ด Totality (Blood Moon)

ISO 800-3200 | 0.5-4s | f/4-5.6 | Exposure changes dramatically โ€” bracket heavily. The Moon dims by 10,000x during totality.

๐Ÿ”ญ Essential Gear

200-500mm telephoto lens, sturdy tripod, remote shutter release, extra batteries (cold nights drain them fast). No solar filter needed.

๐Ÿ’ก Pro Tips

Shoot RAW format. Practice Moon photography before the eclipse. Tape down focus ring after achieving focus. Use mirror lock-up to reduce vibration.

Upcoming Lunar Eclipses (2026โ€“2030)

DateTypeMagnitudeTotalityVisibility
Mar 3, 2026total1.15158 minAsia, Australia, Pacific, Americas
Aug 28, 2026partial0.930โ€”Americas, Europe, Africa, western Asia
Jan 12, 2028partial0.066โ€”Americas, Europe, Africa
Jul 6, 2028partial0.389โ€”Asia, Australia, Pacific, Americas
Dec 31, 2028total1.24359 minAmericas, Europe, Africa, western Asia
Jun 26, 2029total1.17842 minAmericas, Europe, Africa
Dec 20, 2029total1.11784 minAmericas, Europe, Africa, Asia
Jun 15, 2030partial0.500โ€”Asia, Australia, Pacific

Disclaimer: Eclipse contact times are based on NASA/EclipseWise data and may vary by a few minutes. Moon altitude calculations are approximate โ€” atmospheric refraction and local horizon obstructions affect actual visibility. Always verify with TimeAndDate.com for precise local times. Photography settings are starting points; adjust based on actual conditions.

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