New Moon Day

Jerusalem · Thursday, July 02, 2026
Local time: 14:35:08 UTC+3
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Waning Gibbous
94.4%
Illuminated
17.4d
Moon Age
11d
To New Moon
Next New Moon
Wednesday, July 15, 2026
first possible crescent sighting, looking west after sunset
Easily visible to the naked eye
Conjunction · Tuesday, July 14, 2026 at 12:43

Sighting Conditions

First Evening
Wednesday, July 15, 2026
Sunset 19:42
Moonset 20:48
Lag time 66.0 min
Moon age at sunset 31.0 h
Odeh V 9.673
Arc of vision 12.78°
Crescent width 0.69′
Easily visible to the naked eye

Upcoming New Moons

Jul 14, 2026 in 12d A
Aug 12, 2026 in 41d C
Sep 11, 2026 in 71d D
Oct 10, 2026 in 100d D
Nov 09, 2026 in 130d D
Dec 09, 2026 in 160d D

Spring Equinox

Friday, March 20, 2026 · 16:45 104 days ago
Saturday, March 20, 2027 · 22:24 In 261 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).