Full Moon
97.1%
illuminated
Current Moon
Moon Age
15.6 days
Phase
Full Moon
Illumination
97.1%
Next New Moon
Conjunction
Thursday, March 19, 2026 at 03:23
Spring Equinox
Date
Friday, March 20, 2026
Time
16:45 (UTC+2)
Countdown
In 15 days
First Evening
Evening
Thursday, March 19, 2026
Moon Age at Sunset
14.4 hours
Sunset
17:47
Moonset
18:22
Lag Time
35.1 min
Odeh V Value
0.924
Arc of Vision (ARCV)
7.31°
Relative Azimuth (DAZ)
1.29°
Crescent Width (W)
0.13 arcmin
Prediction
May need optical aid to find
Second Evening
Evening
Friday, March 20, 2026
Moon Age at Sunset
38.4 hours
Sunset
17:47
Moonset
19:29
Lag Time
101.3 min
Odeh V Value
18.917
Arc of Vision (ARCV)
20.6°
Relative Azimuth (DAZ)
0.48°
Crescent Width (W)
0.96 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:
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:
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).