I'm not really in a place to judge your math right now to really add anything on that.
(He's also clearly using a different set of data than I have access to. I can't read the context of the Twitter thread so I don't know what numbers he's looking at).
edit:
(let* ((μ 398600.0) ;; km^3/s^2
(r 6371.0) ;; km
(peri (+ r 0.0))
(apo (+ r 180.0))
(a (* 0.5 (+ peri apo))))
(sqrt (* μ
(- (/ 2.0 apo)
(/ 1.0 a)))))
;; 7.745844595118488> 27,900 kph
Seems like they want to test the limit. Same speeds as LEO, but guaranteed to come down.
In the form I'm using, I'm using standard parameters of an elliptical orbit: the periapsis (the closest approach to the center of mass of the massive body (which is a focal point of the ellipse which the orbit traces)), apoapsis (farthest distance), and semimajor axis (their arithmetic mean [1]). I'm evaluating the orbital velocity at the highest point, the apoapsis. μ is a short form for the product G*M, the standard gravitational parameter [2] of Earth (which is known to much higher precision than either the universal gravitational constant G, or the mass of the earth M, individually).
The particular orbit I'm applying it to is one whose periapsis is equal to the Earth's radius—an orbit that touches the surface of the Earth. This is the dividing line for orbital / suborbital: a suborbital trajectory is one that (mathematically) goes beneath the Earth's surface.
[0] https://en.wikipedia.org/wiki/Vis-viva_equation#Equation
[1] https://en.wikipedia.org/wiki/Semi-major_and_semi-minor_axes...
[2] https://en.wikipedia.org/wiki/Standard_gravitational_paramet...
“On orbit” typically means in a stable orbit around a body - but in the case of starship, it could have been on orbit, the delta v is more than sufficient, but that’s an unsafe configuration if you don’t know your engines will relight.
This vehicle is actually going orbital speed, but not quite orbital height (or rather, it's in an "orbit" that has a very eccentric elliptical shape that would cause it to hit the atmosphere on its way back around; it'd be well above a typical orbital height at apogee, though).
You just need to get high enough, and be pointing in the right direction.
Orbit is when an object is traveling so fast that it reaches the horizon of a body before the body's gravity can pull it down to the surface, but perpetually. It's basically perpetually falling around the body. Imagine one of those guys in a wingsuit skimming along the surface of a mountain, never actually touching the surface. It's similar to that, but at a much higher scale.