SUMMARY
The longest day of the year in the tropics does not coincide with the summer solstice but occurs when the sun is directly overhead at solar noon, which varies by latitude. For Honolulu, Hawaii, this phenomenon occurs around May 25 and again in July. The length of day can be calculated using the formula cos(LD/2) = - tan(declination) tan(latitude), where LD is in degrees. While days at the equator average 12 hours, slight variations occur due to atmospheric refraction and the definition of sunrise and sunset.
PREREQUISITES
- Understanding of solar declination and its impact on day length
- Familiarity with the concept of solar noon and its significance
- Basic knowledge of trigonometric functions used in calculating day length
- Awareness of atmospheric refraction and its effects on sunrise and sunset times
NEXT STEPS
- Research the effects of solar declination on different latitudes
- Learn how to calculate solar noon for various locations
- Explore the concept of atmospheric refraction and its impact on daylight hours
- Investigate the phenomenon of Lahaina Noon and its significance in tropical regions
USEFUL FOR
Astronomy enthusiasts, educators, and anyone interested in understanding solar patterns and their effects on day length in tropical regions.