After sharing my eclipse images with friends I had someone ask if I knew how large the prominences were. So I dusted off the trusty slide rule, remembered I have no idea how to use one, and put it back in the drawer. What I came up with is fairly straightforward and based on simple math but I really would like a vote of confidence from some of you before I share it with a wider audience.
Would y'all mind giving me a sanity check?
Deep breath, here goes:
First, the sun's radius is a relatively stable 6.9574 x 105 km (source: https://doi.org/10.1...743921309992304). Converting that radius to diameter in miles:
- Radius = 6.9574 x 10^5 km = 695,740 km
- Diameter = 695,740 km x 2 = 1,391,480 km
- Convert to miles = 1,391,480 km x 0.621371 = 864,625.32 miles
Ok, now we determine how many pixels wide the sun was on my camera sensor. (I initially started down the road of using my system's resolution of 1.72"/pixel and the sun's average angular diameter but that all seemed like a waste of time when I was done. Determining the ratio of pixels to miles was much simpler and more logical to me and I think also to a layperson.)
So then if we divide the width in miles by the width in pixels we determine the image scale.
- 864,625.32 miles / 1,115 pixels = Each pixel represents a linear distance of 775.45 miles
While we’re at it we can determine how large the Earth would appear at the same distance (in pixels).
- 7,917.5 miles / 775.45 miles per pixel = 10.21 pixels
I also created my own scale image of the solar system because I couldn't find a CC licensed one that I liked.
Thanks y'all!