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Seasons, solstices and equinoxes are related to the angular tilt of the Earth's axis of rotation as compared to the ecliptic, which is the plane of the Earth's orbit. They have nothing to do with the elliptical orbit of the Earth.

The Earth's orbit is an ellipse, but it is very nearly circular; the eccentricity is only about 3%. If the Earth's orbit were perfectly circular, we probably wouldn't notice any difference.

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The Solstice or equinox would not change. These are related to the tilt of earth.

Earth is at its closest to our star during December and January, at about 91 million miles, and farthest during June and July at 93 Million miles.

While a perfect circular orbit would not effect your questions it would also be very unlikely that it would ever occur.

As a thought experiment, If there were only Earth and our star, as each orbited while Earth is small in comparison would still pull at the star a small amount.

The Star and earth would be orbiting each other.

Given that objects have mass,

Given mass is attracted to mass,

I do not know of a method other than computer modeling,

to map the orbital patten of our star moving with all of the planets influence.

This is why I do not think it could ever be possible to have a perfect circular orbit.

It would be very complex

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13y ago
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11y ago

A lot would depend on "How much?" additional tilt and eccentricity of the orbit. The Earth's axis of rotation is currently 23 and change degrees "tilted" to the ecliptic, the plane of the Earth's orbit around the Sun. If the angle increased to 30 degrees, it probably wouldn't make all THAT much difference; the temperate zones would be somewhat expanded while the polar weather would become a little more extreme.

Earth's orbit around the Sun is an ellipse, but with only about 3% eccentricity; it's nearly circular. The Earth is at perihelion - closest to the Sun - on January 4 (plus or minus a day, depending on the cycle of leap years) and is at aphelion around July 2. The difference in the distance is only about a million miles or so. If the Earth's orbit were made more eccentric, swinging closer to the sun and farther away, it could easily render the Earth uninhabitable. Over the course of the last 3 million years or so, we've had wild swings between warm weather and ice ages. (We're currently near the peak of one of the warm periods.) Scientists studying human DNA and evolution have calculated that during the last ice age (with a push from a whopping HUGE volcanic eruption!) the human population was down to perhaps 100 breeding pairs of humans. We very nearly became extinct, 70,000 years ago.

An extended winter caused by moving 20 or so million miles away from the Sun could easily finish the job.

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14y ago

Without doing any complex calculations, we can say that the dates of any given equinox

or solstice might move a day one way or another, but the positions of these points in the

sky wouldn't change at all.

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13y ago

While the Earth's orbit is not exactly circular, it's so close that you can't tell it from a circle by eye. Making it a perfect circle would have only a very small impact on the seasons (the fact that the Earth is actually closest to the Sun in early January should give those who live in the Northern hemisphere some idea of how little the shape of the orbit matters).

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Q: How would the solstices and equinoxes change if the earth's orbit were circular instead of elliptical. explain how a circular orbit would effect seasonal changes?
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Seasonal changes occur because of .?

because the earth is tilted 23.5 degrees towards the north star, so we have two equinoxes in the spring and fall


What does the solstices mean?

The word solstice is derived from the Latin sol (sun) and sistere (to stand still), because at the solstices, the Sun stands still in declination (degrees above the horizon at a given time -say noon); that is, the seasonal movement of the Sun's path (as seen from Earth) comes to a stop before reversing direction.When the Sun is at its greatest distance from the celestial equator; the point in the apparent path of the Sun at which the Sun is farthest north or south of the equator.There are two solstices every year on about June 20-21 and December 21-22.Solstice means either of the 2 times in the year, the northern (summer) solstice and the southern (winter) solstice, when the sun reaches its highest or lowest point in the sky at noon, these are also the longest and shortest days (though the difference in daylight duration from day to day around the solstices is least during the year and hardly noticeable.At the instant of solstice the axis of the Earths rotation lies in a plane that intersects the Sun. Coincidentallyly the Earths elliptical orbit now has its major axis close to the solstices so that the Earth is furthest from the Sun about two weeks after the northern (summer) ssolstice and closest to the Sun around January 4-5, less than two weeks after the southern (winter) solstice.The word solstice is derived from the Latin sol (sun) and sistere (to stand still), because at the solstices, the Sun stands still in declination; that is, the seasonal movement of the Sun's path (as seen from Earth) comes to a stop before reversing direction.


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Present thinking that Stonehenge was a calculator and timekeeper for solar and lunar events such as eclipses, solstices and the equinoxes is now going out of favour. Few British archaeologists either believe, or can see any evidence that Stonehenge was was used for complex astronomical 'computations'. There is however considerable evidence that it was carefully designed (as a mirrored symmetrical structure), and that the premeditated design, whatever its contemporary cosmological significance, was set on the axis of the midwinter and midsummer solstices.


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What does the the word solstice mean?

The word solstice is derived from the Latin sol (sun) and sistere (to stand still), because at the solstices, the Sun stands still in declination (degrees above the horizon at a given time -say noon); that is, the seasonal movement of the Sun's path (as seen from Earth) comes to a stop before reversing direction.When the Sun is at its greatest distance from the celestial equator; the point in the apparent path of the Sun at which the Sun is farthest north or south of the equator.There are two solstices every year on about June 20-21 and December 21-22.Solstice means either of the 2 times in the year, the northern (summer) solstice and the southern (winter) solstice, when the sun reaches its highest or lowest point in the sky at noon, these are also the longest and shortest days (though the difference in daylight duration from day to day around the solstices is least during the year and hardly noticeable.At the instant of solstice the axis of the Earths rotation lies in a plane that intersects the Sun. Coincidentallyly the Earths elliptical orbit now has its major axis close to the solstices so that the Earth is furthest from the Sun about two weeks after the northern (summer) ssolstice and closest to the Sun around January 4-5, less than two weeks after the southern (winter) solstice.The word solstice is derived from the Latin sol (sun) and sistere (to stand still), because at the solstices, the Sun stands still in declination; that is, the seasonal movement of the Sun's path (as seen from Earth) comes to a stop before reversing direction.


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