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Waning Gibbous
88.4%
Illuminated
18.7d
Moon Age
10d
To New Moon
Below the horizon — rises 20:46 in the ENE
Next New Moon
Saturday, September 12, 2026
first possible crescent sighting, looking west after sunset
Look west 18:46 – 19:20best chance around 19:01
Visible under perfect conditions
Conjunction · Friday, September 11, 2026 at 06:26
Sighting Conditions
First Evening
Friday, September 11, 2026
Sunset18:47
Moonset18:52
Lag time4.4 min
Moon age at sunset12.3 h
Odeh V-5.519
Arc of vision0.97°
Crescent width0.11′
Not visible even with optical aid
Second Evening
Saturday, September 12, 2026
Sunset18:46
Moonset19:20
Lag time34.3 min
Moon age at sunset36.3 h
Odeh V4.771
Arc of vision7.19°
Crescent width0.82′
Visible under perfect conditions
Upcoming New Moons
First sighting evening → the evening after, shown when the first is doubtful (C) or impossible (D).
Sep 11, 2026in 11dD→B
Oct 10, 2026in 40dD→A
Nov 09, 2026in 70dD→C
Dec 09, 2026in 100dD→A
Jan 07, 2027in 129dC→A
Feb 06, 2027in 159dB
Spring Equinox
Friday, March 20, 2026 · 16:45164 days ago
Saturday, March 20, 2027 · 22:24In 201 days
About the Visibility Prediction
What do the moon phases look like?
The moon cycles through eight phases over approximately 29.5 days:
New Moon
0%
Waxing Crescent
~15%
First Quarter
50%
Waxing Gibbous
~85%
Full Moon
100%
Waning Gibbous
~85%
Last Quarter
50%
Waning Crescent
~15%
After conjunction (new moon), the crescent grows over the first few evenings.
Day 1 is rarely sighted; naked-eye visibility typically begins on day 2 or 3
depending on sky conditions and location:
Day 1
~1% lit
Day 2
~5% lit
Day 3
~10% lit
Day 4
~17% lit
Day 5
~26% lit
How is crescent visibility calculated?
This site uses the Odeh (2006) criterion for predicting
first crescent visibility, developed by Mohammad Odeh of the
Jordanian Astronomical Society. It is considered one of the most
accurate modern models, based on 737 recorded observations from
around the world.
The model computes a V value from two key factors:
Arc of Vision (ARCV)
The altitude difference between the moon and the sun at sunset. A higher arc means the crescent is further above the sun's glare.
Crescent Width (W)
The topocentric width of the illuminated crescent in arcminutes. A wider crescent is brighter and easier to spot.
The formula is: V = ARCV − (7.1651 − 6.3226W + 0.7319W² − 0.1018W³)
What do the visibility zones mean?
Zone A V ≥ 5.65
The crescent is easily visible to the naked eye. No special conditions or experience needed.
Zone B 2.00 ≤ V < 5.65
Visible under perfect conditions — clear skies, low humidity, an unobstructed western horizon, and an experienced observer.
Zone C −0.96 ≤ V < 2.00
Optical aid (binoculars or telescope) is likely needed to locate the crescent. Once found, it may be visible to the naked eye.
Zone D V < −0.96
The crescent is not visible, even with a telescope. The moon is too close to the sun or the crescent is too thin.
What is lag time?
Lag time is the difference between moonset and sunset.
It tells you how long the crescent moon remains above the horizon
after the sun goes down. A longer lag time means a larger window to
spot the crescent before it too sets below the horizon.
Generally, a lag time of at least 40 minutes is considered
favourable for naked-eye sighting, though the Odeh V criterion is a
more comprehensive predictor since it also accounts for the crescent's
brightness and angular separation from the sun.
Why Jerusalem?
Jerusalem holds deep significance for biblical and lunar calendar traditions.
The sighting of the new crescent moon from the land of Israel has historically
been used to declare the beginning of a new month. This site calculates
visibility specifically for Jerusalem's coordinates (31.77°N, 35.21°E).
Moon Finder
Phone compasses are approximate — once you’re within a few degrees, look up and you’ll see it.