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Melbourne, Australia-37.43° N, 145.34° E

Sunrise & Sunset in Melbourne Today

Welcome to the definitive solar ephemeris for Melbourne (Australia), situated at geographic coordinates -37.4336° N latitude and 145.3431° E longitude within the Australia/Melbourne timezone. Because Melbourne is positioned at subtropical coordinates, daylight duration fluctuates predictably throughout the solar year—reaching its maximum duration during the June solstice and its annual minimum near the December solstice.

All timestamps displayed below are computed using client-side spherical astronomy algorithms derived from the U.S. Naval Observatory Astronomical Almanac 2024 and the NOAA Solar Calculator, accounting for standard 34-arcminute atmospheric refraction and 16-arcminute solar semidiameter at sea level.

Sunrise & Sunset in Melbourne, Australia

US Naval Observatory (USNO) Astronomical Almanac 2024 p.C24 & NOAA Solar Model

cos(H) = (cos(90.833°) - sin(δ)·sin(φ)) / (cos(δ)·cos(φ))
Sunrise
09:13 PM
Official Horizon (90°50′)
Sunset
07:35 AM
Official Horizon (90°50′)
Solar Noon
02:24 PM
Highest solar culmination
Day Length
-14h -38m
Golden Hour Photographic Windows (Sun < 6° Elevation)
Morning Golden Hour
09:13 PM10:13 PM
Warm dawn sidelight for landscapes
Evening Golden Hour
06:35 AM07:35 AM
Soft sunset illumination for portraits
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7-Day Solar Forecast for Melbourne

Updated daily
DateSunriseSolar NoonSunsetDaylight
Thu, Aug 6Today
09:13 PM02:24 PM07:35 AM-14h -38m
Fri, Aug 7
09:12 PM02:24 PM07:36 AM-14h -36m
Sat, Aug 8
09:11 PM02:24 PM07:37 AM-14h -34m
Sun, Aug 9
09:10 PM02:24 PM07:38 AM-14h -32m
Mon, Aug 10
09:09 PM02:24 PM07:39 AM-14h -31m
Tue, Aug 11
09:08 PM02:24 PM07:39 AM-14h -29m
Wed, Aug 12
09:07 PM02:23 PM07:40 AM-14h -27m

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Frequently Asked Questions

Q1.What is the exact solar noon in Melbourne?

Solar noon in Melbourne occurs when the sun crosses the local celestial meridian (145.34° E) and reaches its maximum angular elevation above the horizon. Because Melbourne operates on Australia/Melbourne, solar noon typically occurs around mid-day, adjusted for the seasonal Equation of Time.

Q2.How does atmospheric refraction affect sunrise and sunset in Melbourne?

At latitude -37.43°, standard atmospheric refraction lifts the apparent image of the solar disc by approximately 34 arcminutes (0.566°). Combined with the sun’s 16 arcminute semidiameter, official sunrise and sunset are calculated when the center of the true solar disc is 90°50′ from the zenith.

Q3.When are the golden hour shooting windows in Melbourne?

The morning golden hour begins at sunrise and lasts for approximately 60 minutes as the sun climbs to 6° solar elevation. The evening golden hour begins 60 minutes before sunset and concludes as the sun dips below the horizon, providing warm, diffused lighting ideal for outdoor photography.

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