Understanding Time Calculation and Earth's Rotation
This page explores the concept of time calculation as a result of the Ruch obrotowy Ziemi Earth′srotationalmovement. It delves into the intricacies of solar time and provides practical examples of calculating time differences across various global locations.
Definition: Czas słoneczny Solartime, also known as local or place time, is identical for all locations on the same meridian, as it is determined by the sun's position above the horizon.
The document illustrates the Earth's rotation in relation to time:
- A complete 360° rotation corresponds to 24 hours
- 180° equals 12 hours
- 90° represents 6 hours
- 45° is equivalent to 3 hours
Highlight: The key relationship for time calculations is that 15° of longitude corresponds to 1 hour, 1° to 4 minutes, and 15' minutesofarc to 1 minute of time.
The page provides a detailed example of Obliczanie czasu słonecznego calculatingsolartime for Tokyo 139°46′E when it's 11:36 in Warsaw 21°E:
- Calculate the longitude difference: 139°46' - 21° = 118°46'
- Convert to minutes: 118° = 472 minutes, 46' ≈ 3 minutes
- Total time difference: 7 hours 55 minutes
- Result: 11:36 - 7:55 = 3:41 in Tokyo
Example: For Mexico City 98°57′W and New Orleans 90°40′W, similar calculations are performed, considering that time is added for western longitudes:
- Mexico City: 11:36 + 8:00 = 19:36
- New Orleans: 11:36 + 7:26 = 19:02
Vocabulary: Górowanie refers to the sun's highest point in the sky, corresponding to local noon.
This comprehensive guide on Rachuba czasu zadania timecalculationtasks provides students with a solid foundation for understanding global time differences and the practical application of Earth's rotational principles in geography and everyday life.