It varies slightly, as Earth's orbit is not perfectly circular, but rather a slight ellipse.
At its nearest (ironically, for the Northern Hemisphere) in Winter, Earth is 147,098,100 km (91,402,520 miles) from the Sun.
At its furthest, Earth is 152,097,700 km (94,509,130 miles) - which is only 3.4% further.
Still, this slight difference means Southern Hemisphere Summers are slightly warmer, and Southern Hemisphere Winters are slightly colder than they are in the Northern Hemisphere.
The average distance from the sun to the Earth is about 149.6 million kilometers. This distance remains fairly constant throughout the year due to the nearly circular orbit of the Earth around the sun, so it does not change significantly during the summer in either the Northern or Southern Hemisphere.
While it is certainly possible to calculate the distance from the Sun to the Earth in millimeters, it would be foolish to do so. The use of millimeters as a unit of measurement should be restricted to cases when precision requires it, or when the distances are small.
The distance from the Sun to the Earth varies on a moment-by-moment basis, and the "edge" of the Sun itself is indistinct; it would be impossible to say "This is the precise boundary of the Sun".
The distance varies because the Earth's orbit is not circular, but an ellipse. The mean distance is about 150 million kilometers or 93 million miles. The semi-major axis is measured as 149,598,261 kilometers.
Perihelion (when the earth is the closest to the sun) occurs around the first week or Janurary. The distance is roughly 147 million km (91.4 million miles)
Aphelion (when the earth is farthest from the sun) occurs around the first week of Janurary. The distance is about 152 million km (94.5 million miles)
1,392,000 kilometers
109 × Earths
Roughly 92,935,700 miles. This may be wrong.
alot and noone knows exactly because it is to hot to get to close to .
The distance from Earth to the Sun varies throughout the year due to Earth's elliptical orbit. On average, it is about 93 million miles (150 million kilometers). However, during summer in the Northern Hemisphere, Earth is actually farthest from the Sun in a point called aphelion, which is about 94.5 million miles (152 million kilometers) away.
The minimum distance between the Earth and the Sun occurs during perihelion, which is when the Earth is closest to the Sun in its elliptical orbit. This usually happens around January 3rd of each year.
Aphelion -- the point on its orbit when the Earth is farthest from the sun Perihelion -- the point on its orbit when the Earth is closest to the sun so== == == ==
The average distance of Earth from the Sun during its orbit is about 93 million miles (150 million kilometers). This distance is known as an astronomical unit (AU) and is used as a convenient way to measure distances within our solar system.
Venus has an average distance from the Sun that is about 108% of Earth's distance. This makes Venus the planet closest to having a distance from the Sun that is 150% of Earth's distance.
The Earth reaches its greatest distance from the Sun during the summer season in the Northern Hemisphere. Though it may seem counterintuitive, the distance between the Earth and the Sun varies due to the elliptical shape of Earth's orbit, with the Earth being farthest from the Sun during the summer months.
The distance between the Earth and the Sun varies due to its elliptical orbit. During the Earth's summer in the Northern Hemisphere, it is actually at its farthest point from the Sun, called aphelion. At this point, the distance is about 94.5 million miles (152 million km).
The distance from Earth to the Sun during summer solstice is about 1.6 million miles further than the average distance of 93 million miles. This is because the orbit is an elliptical shape.
When Earth is closer to the Sun, it is in winter in the Northern Hemisphere and summer in the Southern Hemisphere. The distance between Earth and the Sun (known as Earth's orbital distance) doesn't significantly affect the seasons; the tilt of Earth's axis is the primary factor that determines the seasons.
The sun is warmer in the summer because during this season, the Earth's axis is tilted towards the sun. This means that sunlight hits more directly and for longer periods, leading to warmer temperatures.
The Earth's changing distance from the Sun during the year causes the seasons.
The Earth's orbit around the Sun is elliptical, not a perfect circle. This means that the distance between the Sun and Earth is constantly altering during the orbit of the Earth.
The closest the earth gets to the sun is 146 million km (91 million miles) at perihelion, during winter in the Northern Hemisphere, which is summer in the Southern Hemisphere.We are farthest away at aphelion, during Northern Hemisphere summer, maximum distance is 152 million km (94.5 million miles).The average distance between the sun and the earth is 149 million kilometers (93 million miles).
In the summer
The Earth's revolution around the Sun, combined with its axial tilt. In summer at a particular latitude the heating effect of the Sun is usually a lot more than in the winter at that latitude. This is because the tilt is "towards" the Sun in the summer, but "away" from the Sun in the winter. The seasons are not caused by the small changes in the Earth's distance from the Sun during its orbit.
No. As it happens the Earth is closest to the sun when it is winter in the northern hemisphere. Seasons like summer and winter are related to the tilt of the earth with respect to the plane of its orbit about the sun, not to the distance from the sun.
The distance from Earth to the Sun varies throughout the year due to Earth's elliptical orbit. On average, it is about 93 million miles (150 million kilometers). However, during summer in the Northern Hemisphere, Earth is actually farthest from the Sun in a point called aphelion, which is about 94.5 million miles (152 million kilometers) away.