Curiosity
This is a place where I put curious things. Check it out!
Great Circle Globe
Did you know that, unless you’re ON the equator, you have to constantly turn a little bit to walk due east or due west? Play around with this interactive globe and map to get a sense of what I mean. Double-click to drop a marker anywhere on the globe. This tool also allows you to draw a great circle from that marker starting in any direction (N, NE, E, and so on). You can also draw a latitude circle from the same marker. Notice how different these circles look on the Mercator projection map next to the globe. You can toggle the globe's transparency to see through it, and add a diameter connecting each marker to its antipode to help build your 3D sense of things.
When you traverse a sphere (I know the Earth is technically an oblate spheroid, don’t come at me) in a straight line, you always follow a great circle. This path will go around the globe to the antipode of your starting point (the point exactly opposite your marker)before coming back. If you start out at 90 degrees (east) or 270 degrees (west), you’ll begin tangent to the latitude circle of your starting point but will follow a great circle. You can use this to see just how much you need to turn to stay at the same latitude while traveling due east (or west). The farther away from the equator, the smaller the radius of the latitude circle.
*This tool was vibe-coded (poorly) by me. As such, it only really works on desktop. If you’re a developer and want to review the code and make suggestions, let me know by submitting the contact form.
Interactive Earth Orbit
This is an interactive model of Earth's orbit around the Sun. In “Orbit View,” we see the elliptical nature of Earth's orbit (you can scale it up to make it more obvious). Note that the point in our orbit that is farthest from the sun (aphelion) is in July. I think it is curious that the moment we are farthest from the sun occurs during the hottest month of the year for residents of the Northern Hemisphere.
*This tool was vibe-coded (poorly) by me. As such, it only really works on desktop. If you’re a developer and want to review the code and make suggestions, let me know by submitting the contact form.
Two-body Kepler model of Earth's orbit (e = 0.0167, anomalistic year 365.2596 d), anchored to the published 2026 perihelion (January 3, 17:15 UTC). Event buttons use published 2026 dates. Moon position is approximate (mean synodic month from the mid-January new moon) and its orbit is drawn ~40× too large so it is visible. In the side view the camera sits in the ecliptic plane with the Sun always to the left, so the axis lean shows its component toward or away from the Sun: the full 23.4° at the Solstices, zero at the Equinoxes.