Physical aspects of our Solar System

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Discussion Overview

The discussion revolves around the physical aspects of the Solar System that influence the Earth's seasons and the resulting variations in daylight hours. Participants explore how to calculate the shortest and longest days at specific locations on Earth, touching on concepts such as Earth's orbit, axial tilt, and latitude.

Discussion Character

  • Exploratory
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant inquires about the relationship between Earth's dynamics and the variability of daylight hours, suggesting a need for data on orbital velocity, rotation speed, and axial tilt.
  • Another participant expresses a lack of data but proposes that daylight hours can be generalized based on city locations and their daylight experiences on a specific date, indicating a potential relationship involving latitude, longitude, and the day of the year.
  • A formula for calculating hours of sunlight is presented, which includes latitude and a cosine function, but is noted to be potentially incorrect for extreme latitudes like the poles.
  • Another participant critiques the initial formula, suggesting it does not account for extreme conditions and shares a different formula derived from their past experience, which incorporates axial tilt and uses arcsine functions.
  • Participants discuss the complexity of deriving accurate formulas and the availability of online calculators for determining daylight hours.

Areas of Agreement / Disagreement

Participants express differing views on the accuracy and applicability of the proposed formulas for calculating daylight hours. There is no consensus on a definitive method or formula, and the discussion remains unresolved regarding the best approach.

Contextual Notes

Limitations include the potential inaccuracy of the proposed formulas for extreme latitudes and the need for a deeper understanding of the underlying mathematics to derive accurate calculations.

decs
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Consider the physical aspects of our Solar System that result in the Earth having seasons... how does this gives us variable hours of daylight.

How would i calculate the shortest or longest day for a specific point on earth?

cheers.
 
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Err, what is your level of understanding of the dynamics of the Earth? I mean what do you know about how it travels around the sun? What measurements do you have about velocity of orbit, speed or rotation, tilt of axis etc..?
 
Zurtex said:
Err, what is your level of understanding of the dynamics of the Earth? I mean what do you know about how it travels around the sun? What measurements do you have about velocity of orbit, speed or rotation, tilt of axis etc..?

i have absolutely no data about any of the prior. what i DO have is various cities locations and the amount of daylight they experienced on the 4th of July.

I should be able to extend these findings to make a generalisation about the hours of daylight for any latitude and longitude.

there should be a relationship that relates the day of the year, the hours of daylight, the latitude and the longitude.
 
decs said:
i have absolutely no data about any of the prior. what i DO have is various cities locations and the amount of daylight they experienced on the 4th of July.

I should be able to extend these findings to make a generalisation about the hours of daylight for any latitude and longitude.

there should be a relationship that relates the day of the year, the hours of daylight, the latitude and the longitude.
Yeah, I wouldn't imagine it's all that complex but you need to know a bit about ellipses and spheres.

However by the sounds of it you don't really have the mathematical knowledge to construct a method to work out day light given the latitude and longitude and the date. There are calculators all over the web that will just give an output for you though, like the above poster says, you could just use Google.
 
i formula so far is

12+(12/67)*latitude*cos(2pi.t)=hours of sunlight

where t=days/365

its ALMOST right ppl...
 
decs said:
i formula so far is

12+(12/67)*latitude*cos(2pi.t)=hours of sunlight

where t=days/365

its ALMOST right ppl...
May I ask how you derived that? I may be able to help you.

Edit: Oh and it clearly isn't right as it wouldn't work for extreme places like such as the north and south poles where there can be daylight for days.

I speant about 5 minuites attempting to draw out a model to caclulate it when I realized quite a lot of data. Anyway here is something I found while looking it up: http://www.spsu.edu/math/stinger/101-115/109.htm

I have a feeling that is a bit simplified but I think it might do you nicely.
 
Last edited:
I remembering figuring this one out years ago when I was a student. I'm not sure if the equation I got was exact, but I think it was pretty close. The formula I arrived at was

daylight_hours = 12 ( 1 + 2/Pi arcsin( tan(tilt) tan(lat) sin(2 Pi * n / 365.25) ) )

Where,
tilt = Constant of 0.4093 radians (23.45 degrees)
lat = Latitude of location on Earth.
n = Number of days elapsed since the northern hemishpere spring equinox.

Notes.

1. I've used radian throughout, just change each literal occurrence of "Pi" to 180 if you want to use degrees throughout.

2. The equation should apply without modification to both northern and southern hemispheres provided that southern latitudes are entered as negative.
 
Last edited:

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