How to Calculate Hour Angle and Solar Noon: Simplified Guide"

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In summary, the conversation discusses finding the hour angle and solar noon for any day of the year. Different formulas and methods are mentioned, including using Julian Day Numbers, sidereal time, right ascension, and calculations based on location and longitude. The conversation also touches on the concept of solar time and how it corresponds to solar noon. Ultimately, the goal is to calculate the hour angle and solar noon accurately.
  • #1
dacruick
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Hi. I want to be able to find the hour angle at each day of the year. Wikipedia sent me on a wild goose chase of Julian Day Numbers and some useless formulas that place solar noon at the same time every day. For those who may be used to different terms, hour angle is the amount of time (in degrees) that a position on Earth is away from solar noon. Ideally I would like to be able to find the hour angle, but finding solar noon will also be acceptable as well, as I can find the hour angle from that.

One site suggested that my hour angle is equal to the local sidereal time subtract the right ascension. The problem with this is I don't know how to calculate sidereal time, or right ascension. If anyone could shed some light for me(no pun intended), it would be much appreciated
 
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  • #2
The Wikipedia article on http://en.wikipedia.org/wiki/Sidereal_time" should help.

Also, this site can calculate it for you based on your location - http://tycho.usno.navy.mil/sidereal.html" .
 
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  • #3
Find solar time:

[tex]Solar\ Time = Standar\ Time + 4\left(L_{st}-L_{loc}\right)+E[/tex]

where Lst is the standard meridian for the local time zone, Lloc is the longitude of the location, and E is defined by:

[tex]E=229.2\left(0.000075+0.001868\ cosB-0.032077\ sinB-0.014615\ cos2B-0.04089\ sin2B\right)[/tex]

where B is

[tex]B=\left(n-1\right)\frac{360}{365}[/tex]

and n is the day of the year.

To get hour angle from time, multiply hours from noon times 15 degrees per hour (negative for before noon, positive for after). For example if solar time is 10:30 am, this is 1.5 hours before noon, so the hour angle would be -22.5 degrees.
 
  • #4
when you say Lst is the standard meridian for the local time zone, what does that mean.
 
  • #5
It is the longitude that corresponds with your time zone. Examples in the US would be Eastern - 75oW, Central - 90oW, Mountain - 105oW, and Pacific - 120oW.
 
  • #6
Yeti08 said:
It is the longitude that corresponds with your time zone. Examples in the US would be Eastern - 75oW, Central - 90oW, Mountain - 105oW, and Pacific - 120oW.

I though Lloc was the longitude corresponding to my time zone.
 
  • #7
If you photograph the position of the Sun at noon (not daylight savings time) every day for a year, you will get an analemma in the sky. See

http://www.1worldglobes.com/analemma.htm

The analemma used to be shown on world globes, usually in the Pacific Ocean, west of South America.

Bob S
 
  • #8
dacruick said:
I though Lloc was the longitude corresponding to my time zone.
That's your actual longitude for the location. That difference in that equation is to correct for your actual location - while your "normal" time will stay the same while traveling across several degrees of longitude, your solar time will change.
 
  • #9
I apologize, I don't think I understand what you are saying. I live in Toronto, so my Lloc would be approximately 79 degrees. But you are saying my Lst will be 75 degrees because I'm in the eastern time zone? So my difference will be -4 degrees correct?
 
  • #10
Furthermore, I am doing this to calculate solar time, but I do not know what solar time is. Is the solar time equal to solar noon?
 
  • #11
dacruick said:
I apologize, I don't think I understand what you are saying. I live in Toronto, so my Lloc would be approximately 79 degrees. But you are saying my Lst will be 75 degrees because I'm in the eastern time zone? So my difference will be -4 degrees correct?
Yes, that is correct.

dacruick said:
Furthermore, I am doing this to calculate solar time, but I do not know what solar time is. Is the solar time equal to solar noon?
For solar time, noon corresponds to solar noon. I stated in my first post how to convert solar time to hour angle.
 
  • #12
So my standard time must be measured in degrees as well?
 
  • #13
Yes, I should have said before that all the equations I listed use degrees, not radians.
 

1. What is an hour angle?

An hour angle is a celestial coordinate used in astronomy to measure the angular distance between a celestial object and the observer's meridian. It is measured in degrees and is used to determine the position of an object in the sky.

2. How is hour angle calculated?

Hour angle is calculated by subtracting the local sidereal time (LST) from the right ascension of the celestial object. LST is the time it takes for the vernal equinox to pass over the observer's meridian and can be calculated using the observer's longitude and the current date and time.

3. What is the significance of hour angle?

Hour angle is important in celestial navigation and astrometry as it allows astronomers to accurately locate objects in the sky. It is also used in calculating the altitude and azimuth of an object, which is necessary for tracking and observing celestial bodies.

4. How does hour angle change over time?

Hour angle changes over time due to the Earth's rotation. As the Earth rotates, the observer's meridian moves and the hour angle of a celestial object changes accordingly. This change is also affected by the observer's location on Earth.

5. Is hour angle affected by the location of the observer?

Yes, the hour angle of a celestial object is affected by the location of the observer on Earth. This is because the Earth's rotation and the observer's meridian are both influenced by the observer's latitude and longitude. Therefore, the same celestial object will have a different hour angle for two observers located at different latitudes or longitudes.

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