New Moon Day

Jerusalem · Monday, August 31, 2026
Local time: 13:34:42 UTC+3
change location view a date
or
Enter coordinates manually
Leave UTC offset blank to use your browser's timezone
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 – 19:20 best chance around 19:01
Visible under perfect conditions
Conjunction · Friday, September 11, 2026 at 06:26

Sighting Conditions

First Evening
Friday, September 11, 2026
Sunset 18:47
Moonset 18:52
Lag time 4.4 min
Moon age at sunset 12.3 h
Odeh V -5.519
Arc of vision 0.97°
Crescent width 0.11′
Not visible even with optical aid
Second Evening
Saturday, September 12, 2026
Sunset 18:46
Moonset 19:20
Lag time 34.3 min
Moon age at sunset 36.3 h
Odeh V 4.771
Arc of vision 7.19°
Crescent width 0.82′
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, 2026 in 11d D B
Oct 10, 2026 in 40d D A
Nov 09, 2026 in 70d D C
Dec 09, 2026 in 100d D A
Jan 07, 2027 in 129d C A
Feb 06, 2027 in 159d B

Spring Equinox

Friday, March 20, 2026 · 16:45 164 days ago
Saturday, March 20, 2027 · 22:24 In 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).