All-in-One Outdoor Photography Suite

Sun, Golden Hour & Outdoor Photography Tools

Pinpoint precise morning & evening golden hours, blue hour color balance, twilight transitions, exact solar azimuth, elevation angles, and shadow lengths for any coordinate on Earth.

14 Integrated Solar & Light Planning Tools Direct Mode Switch
Location & Ephemeris
Solar Noon: Calculating...
Solar Time Simulator 17:30
00:00 (Midnight) 12:00 (Noon) 23:55
EVENING GOLD
Evening Golden Hour
18:42 - 19:22
Duration: 40 mins • Altitude +6° to -4°
Sunrise & Sunset
06:27 / 19:03
Daylight: 12h 36m • Elevation: -0.833°
Blue Hour Windows
05:54 19:22
Civil Twilight • Sun -6° to -4°
Sun Position & Angle
+16.4° Alt
Azimuth: 263.8° WSW
Shadow Length
5.94 m
Ratio: 3.40x • Dir: 83.8° ENE
24-Hour Solar Timeline • Daylight Phase
Simulated: 17:30
00:00 Night Astro Dawn Sunrise Noon Sunset Astro Dusk 24:00
Interactive Solar Horizon Dome & Direction Compass
Elevation: +16.4° | Azimuth: 263.8°
+6° Golden Hour -6° Blue Hour 0° True Horizon Max Altitude: +58.2° EAST (90°) SE (135°) SOUTH (180°) SW (225°) WEST (270°) 264° WSW
Solar Noon 12:45 PM
Total Daylight 12h 36m
Golden Window 40 mins
Sun Declination +5.8°
Shadow Length & Solar Direction Simulation
Height: 1.75m • Length: 5.94m • Angle: +16.4°
1.75m 5.94 m (3.4x) Sun: +16.4°
Twilight Phases & Astrophotography Darkness Window
Sun elevation stages below horizon
Civil Twilight (0° to -6°)
Dawn: 05:54 - 06:27
Dusk: 19:03 - 19:36
Includes the Blue Hour window. Brightest stars emerge. Streetlights illuminate. No artificial light required for outdoor movement.
Nautical Twilight (-6° to -12°)
Dawn: 05:18 - 05:54
Dusk: 19:36 - 20:12
Horizon remains distinguishable at sea. General terrestrial shapes discernible. Deep navy skies for dramatic long exposure cityscapes.
Astronomical Twilight (-12° to -18°)
Dawn: 04:40 - 05:18
Dusk: 20:12 - 20:50
Atmospheric light completely ceases once the sun dips below -18°. Pitch-black sky perfect for Milky Way, aurora, and faint deep-sky photography.
Master Outdoor Photography Lighting Schedule
Chronological Daily Phases
Phase Solar Elevation Time Window Recommended Photography Style Light Characteristics

Complete Outdoor Photography Lighting Guide

Natural light is the defining element of landscape, architectural, portrait, and street photography. The altitude and azimuth of the sun fundamentally dictate contrast, shadow length, white balance, and exposure latitude. Understanding how to calculate solar transitions empowers you to arrive on location with optimal preparation.

1. The Golden Hour Explained

Photographic Golden Hour occurs when the sun sits between -4° and +6° relative to the horizon (encompassing the 10-15 minutes prior to sunrise and following sunset, as well as the immediate post-sunrise / pre-sunset light). At this shallow angle, atmospheric Rayleigh scattering removes shorter blue wavelengths, allowing predominantly warm, reddish-gold photons to reach the earth.

Golden Hour Elevation Range: -4.0° ≤ Solar Elevation ≤ +6.0°
Key Benefits: Ultra-low contrast, saturated warm tones, flattering skin highlights, elongated directional shadows.

2. The Blue Hour Window

The Blue Hour occupies the portion of Civil Twilight when the sun is between -4° and -6° below the horizon. As direct sunlight ceases, ozone absorption (the Chappuis effect) causes remaining indirect skylight to turn rich cobalt and indigo. For urban photographers, this period balances natural deep blue skies with artificial city lights (1:1 exposure ratio).

Blue Hour Elevation Range: -6.0° ≤ Solar Elevation ≤ -4.0°
Best Practice: Tripod mandatory, base ISO 100, f/8 - f/11, 2s to 20s exposure time, bracketed 3-shot HDR for dynamic scenes.

3. Shadow Length & Solar Direction Math

The length of any shadow cast by an upright vertical subject can be precisely calculated using basic trigonometry based on the solar elevation angle $\alpha$:

Shadow Length = Subject Height / tan(α)
Shadow Azimuth = (Solar Azimuth + 180°) mod 360°

When the sun is at 10° elevation, a 1.75m photographer casts a shadow nearly 10 meters long. When the sun reaches 45°, the shadow length precisely equals the subject height. At solar noon in summer when the sun reaches 70°, shadows shorten to a fraction of the subject, creating unflattering downward eye shadows for portraiture.

4. Twilight Hierarchy for Astrophotographers

Photographers planning nightscapes, Milky Way captures, or star trails must identify the start of Astronomical Darkness (when the sun drops below -18°). Between -12° and -18° (Astronomical Twilight), the sky appears dark to the naked eye, but camera sensors will still record faint skyglow on long exposures.

Frequently Asked Questions

Despite the name "hour", the duration varies drastically based on latitude and season. Near the equator (e.g., Singapore or Ecuador), the sun sets vertically at high speed, making golden hour last only 20 to 25 minutes. In mid-latitudes (e.g., Paris or New York), it lasts 40 to 50 minutes. Near the Arctic Circle (e.g., Iceland or Norway) in summer, the sun glances along the horizon, creating a golden hour that can persist for 3 to 5 continuous hours or even all night!
Golden Hour features direct sunlight passing horizontally through the atmosphere, imparting a warm color temperature (2,500K - 3,500K) with golden highlights. Blue Hour occurs after sunset (or before sunrise) when no direct sunlight reaches the ground, leaving diffuse indirect Rayleigh and ozone scattering with a cool color temperature (8,000K - 10,000K) and rich royal blue skies.
Clock noon (12:00 PM) rarely matches solar noon (when the sun reaches its highest celestial altitude). This is due to two astronomical factors: the Equation of Time (caused by Earth's elliptical orbit and axial tilt) and the observer's position relative to the central meridian of their standard civil time zone.
For portraits, plan your session during the 40 minutes prior to sunset. Place the sun behind your subject for backlight (rim lighting or hair light) while using a 5-in-1 reflector or fill flash to illuminate the face. As the sun drops below 4° altitude, contrast softens so much that you can face subjects directly into the sun without squinting.
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