A sundial located in New York City (longitude
W) shows a local apparent solar time of 12:00 PM when the sun is at its highest point in the sky. However, the standard time in New York (Eastern Time Zone, UTC-5) is different due to the equation of time and longitude correction.
- Calculate the mean solar time corresponding to this observation.
- Determine the difference between local apparent solar time and mean solar time if the equation of time on that day is
minutes.
- What is the standard clock time (Eastern Time) for this event, considering the longitude-based time zone adjustment?
- Longitude of New York City:
W.
- Reference longitude for Eastern Time Zone:
W.
- Equation of Time on the given day:
minutes.
1. Mean Solar Time (MST) is related to Local Apparent Solar Time (LAST) by the equation:
MST  LAST 
Since LAST is 12:00 PM,
2. Longitude Correction: The time zone is based on
W, but New York City is at
W. The difference is:
Since
hour, the time difference is:
3. Standard Clock Time: The mean solar time must be adjusted by to get the standard time:
The mean solar time is
PM, and the standard clock time is approximately
PM.
This is an example problem generated from DeepSeek AI using prompt, "For a physics class can you give an example problem for mean solar time and write it in latex".
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