Composite image showing the size of the sun at aphelion (our farthest point) and perihelion (our closest point). The photos were taken 18 months apart, and a few days from the events due to adverse weather conditions, but they show an unmistakable size difference of the sun as viewed from Earth, across our yearly orbit. Image by Peter Lowenstein.
The sun at aphelion appears smaller in our sky, as shown in this composite image. This image consists of two photos, taken just days away from a perihelion (Earth’s closest point to the sun) in January, 2016, and an aphelion (Earth’s farthest point from the sun) in July, 2017. The gray rim around the sun (actually the perihelion photo) illustrates that, as seen in our sky, the sun is about 3.6 percent bigger at perihelion than aphelion. This difference is, of course, too small to detect with the eye.
Although taken 18 months apart, and a few days from the events due to adverse weather conditions, you can see there is an unmistakable size difference of the sun as viewed from Earth when it is closest at perihelion and furthest away at aphelion.
Here are the original photos, used in the composite image above, showing the size difference of the sun between Earth’s perihelion (closest point) and aphelion (farthest point). Image by Peter Lowenstein.
Bottom line: Composite image showing the size of the sun at perihelion and aphelion.
Dr. Peter Lowenstein has contributed many beautiful and fascinating images and stories to EarthSky. Trained as a geochemist, he spent his early years with the Geological Survey of Papua New Guinea, specializing in metals and volcanoes. In 1989, he moved to the Zimbabwe Geological Survey as Chief Economic Geologist and has lived and worked in Zimbabwe ever since. Peter is now retired to Zimbabwe, in a house with a beautiful view in Murambi East, Mutare, where he pursues favorite hobbies including construction of electronic gadgets, listening to music, gardening, surfing the Internet ... and photography.
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