New Moon Day

Jerusalem · Monday, May 04, 2026
Local time: 03:20:51 UTC+3
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Full Moon
95.1%
illuminated

Current Moon

Moon Age 16.5 days
Phase Full Moon
Illumination 95.1%

Next New Moon

Conjunction Saturday, May 16, 2026 at 23:00
First possible sighting Sunday, May 17, 2026

Upcoming New Moons

May 16, 2026 in 12d A
Jun 15, 2026 in 42d B
Jul 14, 2026 in 71d A
Aug 12, 2026 in 100d C
Sep 11, 2026 in 130d D
Oct 10, 2026 in 159d D

Spring Equinox 2026

Date Friday, March 20, 2026
Time 16:45 (UTC+3)
Elapsed 45 days ago

Spring Equinox 2027

Date Saturday, March 20, 2027
Time 22:24 (UTC+3)
Countdown In 320 days

First Evening

Evening Sunday, May 17, 2026
Moon Age at Sunset 20.4 hours
Sunset 19:27
Moonset 20:34
Lag Time 67.6 min
Odeh V Value 7.24
Arc of Vision (ARCV) 12.31°
Relative Azimuth (DAZ) 0.06°
Crescent Width (W) 0.34 arcmin
Prediction Easily visible to the naked eye

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).