Seasons due to Earth's elliptical orbit

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Discussion Overview

The discussion centers on the causes of Earth's seasons, specifically examining the roles of the Earth's axial tilt and its elliptical orbit. Participants explore how these factors contribute to temperature variations and seasonal changes, with a focus on both theoretical and observational aspects.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants assert that the tilt of the Earth's axis is the primary factor in determining seasons, with the northern hemisphere tilted toward the sun during summer and away during winter.
  • Others argue that while the Earth's elliptical orbit does affect distance from the sun, its impact on seasonal temperature variations is minimal compared to the effects of axial tilt.
  • One participant notes that the Earth's distance from the sun varies by about 5 million km, but this variation does not significantly influence temperature compared to the effects of daylight length and sun angle.
  • Some contributions highlight that the uneven distribution of land and ocean between hemispheres also plays a role in seasonal temperature differences.
  • A later reply mentions the complexity of Mars' seasons, which involve both axial tilt and distance variations due to its more eccentric orbit.
  • Participants also discuss the challenges of observing the effects of the Earth's orbit amidst other influencing factors, such as ocean currents and climate patterns.

Areas of Agreement / Disagreement

Participants generally agree that the axial tilt is the major determining factor for seasons. However, there is some contention regarding the significance of the Earth's elliptical orbit and its distance from the sun, with multiple views presented on its impact.

Contextual Notes

Some participants mention the complexity of seasonal changes on Mars compared to Earth, indicating that the discussion may not fully account for all variables influencing seasonal effects.

Who May Find This Useful

This discussion may be of interest to those studying Earth sciences, astronomy, or climate science, as well as individuals curious about the mechanisms behind seasonal changes on Earth and other planets.

MisterAmrani
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Hello there! What I have never understood is that our seasons are the result of the tilt of the Earth's axis, and I've always interpreted that to mean that the northern hemisphere is closer to the sun in June, July, and August, and the southern in December, January, and February. If that is the case, I don't understand why a shift in the axis results in temperature variations of ~50 degrees (around 40 degrees N), yet a variation of distance from the sun of 3 million+ miles does not affect the temperature. Or do I have this all wrong, and the elliptical orbit also plays a part in the temperatures?
 
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There is an effect, it's just hard to see in the middle of everything else that is happening.

The day length changes quite drastically summer to winter. In Toronto, where I live, a winter day can be as short as 6 hours. Plus the sun does not get very high in the sky. In summer, a day can be 14 hours. So more than double. And it gets higher in the sky so the sun light is falling closer to vertical. So this produces much more heat per square meter.

The Earth's orbit is slightly non-circular, as you refer to. And it is slightly closer for part of the year. This amounts to a change of about 3 percent. (To one digit.) So, crank out your inverse-square law and work out how much this increases total solar radiation. (Hint 1.03 * 1.03 is just a bit more than 1.06.) So comparing that to the more-than-doubling of daylight in Toronto means that the distance effect is probably pretty small.

There are other perturbations and effects that make the effect hard to see. For example, the southern hemisphere has a lot more ocean than the northern. Ocean currents and clouds tend to be very different in the southern hemisphere.
 
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MisterAmrani said:
Hello there! What I have never understood is that our seasons are the result of the tilt of the Earth's axis, and I've always interpreted that to mean that the northern hemisphere is closer to the sun in June, July, and August, and the southern in December, January, and February. If that is the case, I don't understand why a shift in the axis results in temperature variations of ~50 degrees (around 40 degrees N), yet a variation of distance from the sun of 3 million+ miles does not affect the temperature. Or do I have this all wrong, and the elliptical orbit also plays a part in the temperatures?

Actually, it is the tilt of the Earth's axis which is the major determining factor in creating the seasons. In the northern hemisphere, the axis is tilted toward the sun during the summer months, while the southern hemisphere is tilted away at the same time, producing winter in that region. The opposite holds true in the winter season of the northern hemisphere.

As to the influence of the Earth's orbit on the seasons, it is relatively minimal and surprisingly the opposite of what is expected. The distance of the Earth from the sun varies by about 5 million km out of 150 million km average during the year. However, the Earth reaches perihelion, or the closest point from the sun, about January 3 every year, and aphelion, or the farthest point from the sun, about July 4.

http://en.wikipedia.org/wiki/Perihelion_and_aphelion
 
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Take a look at these attached sketches also:
(main sketch and enlarged views of the solstices)
(you will have to rotate them)
The red line is a daily path of a point at about 45 degrees latitude above the equator.
 

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If you read between the lines of the very complete answers you have gotten above, you can see that the difference in distance to the Sun that is caused by the tilt is indeed completely negligible. So you have that part right-- the tilt has nothing to do with distance to the Sun. But what you did not understand is what is being explained above-- all the other important things that tilt does do (it changes the length of the day, and how close to overhead the Sun gets, and you know from daily experience that the temperature rises when the Sun is closer to directly overhead). In fact, when teaching the simplest understanding of the seasons, the first thing we usually say is completely forget distance to the Sun, you can understand seasons on Earth without even thinking about distance variations. If you do want to think about distance, consider Mars' seasons instead-- they combine tilt and distance variations from the elliptical orbit, so are quite a bit more complicated than Earth seasons.
 
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Thank you all for your answers, you cleared things up for me!
 
Me too! Thanks for asking the question Mister!
 
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SteamKing said:
As to the influence of the Earth's orbit on the seasons, it is relatively minimal and surprisingly the opposite of what is expected.
For the northern hemisphere, that is. The Aussies don't know they are upside-down!
 
Ken G said:
n fact, when teaching the simplest understanding of the seasons, the first thing we usually say is completely forget distance to the Sun, you can understand seasons on Earth without even thinking about distance variations. If you do want to think about distance, consider Mars' seasons instead-- they combine tilt and distance variations from the elliptical orbit, so are quite a bit more complicated than Earth seasons.
These are very good points.

As everyone has already said, the primary driver of seasons on the Earth is the Earth's axial tilt. The Earth as a whole is cooler in January (when it is closest to the Sun) than it is in July (when it is furthest from the Sun), showing how unimportant distance is when it comes to driving the seasons. The reason the Earth as a whole is cooler in January than in July is because of the uneven distribution of ocean and land between the northern and southern hemispheres. This is a secondary cause of the seasons. Distance from the Sun? That's at best tertiary, at least for the Earth.

Mars doesn't have oceans and its orbit about the Sun is much more eccentric than that of the Earth. Mars' seasons are a complex mix of eccentricity and axial tilt.
 
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T
SteamKing said:
Actually, it is the tilt of the Earth's axis which is the major determining factor in creating the seasons. In the northern hemisphere, the axis is tilted toward the sun during the summer months, while the southern hemisphere is tilted away at the same time, producing winter in that region. The opposite holds true in the winter season of the northern hemisphere.

As to the influence of the Earth's orbit on the seasons, it is relatively minimal and surprisingly the opposite of what is expected. The distance of the Earth from the sun varies by about 5 million km out of 150 million km average during the year. However, the Earth reaches perihelion, or the closest point from the sun, about January 3 every year, and aphelion, or the farthest point from the sun, about July 4.

http://en.wikipedia.org/wiki/Perihelion_and_aphelion
There is also the 25000 Earth wobble the Southern Hemisphere is close now but over time it will be the northern hemisphere. the Sahara will be wet not dry ect ect
 
  • #11
DEvens said:
In Toronto, where I live, a winter day can be as short as 6 hours.
You must live waaaaay up near Steeles (just shy of the Arctic Circle). Down here, near the lake, Toronto never gets less than a 9 hour day. :wink:

http://www.timeanddate.com/sun/canada/toronto?month=12
 

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