
It’s difficult to project a sphere onto a flat, two-dimensional surface. All maps of the Earth have flaws; the same is true for the cosmos.
The Universe is a vast and expansive place. From any location, you have total freedom to look in any direction you like: up or down, left or right, and near or far, to any distance in any direction that you choose. (Well, so long as there isn’t anything nearby in the way of a more distant object that you want to observe.) It’s like you have a buffet, an omnidirectional buffet, of targets to choose from. You can even imagine observing it all: not just the half of the sky you can see by lying down in a field on a clear night, but in all directions all at once, like if you had an array of lenses that looked around in all 360° at once (plus the ability to view 90° up and down from the horizontal), that gathered light from all possible angles simultaneously.
And yet, when we show images of the cosmic microwave background — whether from COBE, WMAP, Planck, or a different mission — they’re almost always shown as oval-shaped. What does that oval shape actually show us, and why do astronomers make that specific visualization choice? That’s what Ed Matzenik wants to know, writing in to ask:
“I don’t understand the projections we see of the CMB. They are usually a circle or an oval. Is that the whole sky or just a section? If I was looking at a sphere from inside I don’t know how I’d represent it on a flat sheet… hope you can clear up this mystery for me.”
Honestly, the first time I encountered them — and remember, I’m a professional cosmologist who first encountered them in graduate school — I suffered from almost exactly the same puzzlement. Let’s begin with something we’re much more familiar with in order to get started: planet Earth.
This is going to sound obvious, but the first thing you have to realize about planet Earth is that, to a first approximation, its shape is spherical. The most accurate tool we use to model and represent…
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