A Density Scale

Server Sky will deploy at 6411 km altitude. Gas density at that altitude is 6E-18 kg/m², mostly hydrogen. That is 5E-18 times smaller than air density at the surface; it is difficult to comprehend just how tenuous the exosphere is, so here is a density scale. The densities below assume average solar activity, F107 = 150 , averaged over the day, on the equator, at the equinox .

"zone"	density kg/m³	pressure	altitude
zepto	2e-21			interstellar space "average"
zepto	1e-20			interplanetary space 1 A.U.
atto?	?		35786 km	geosynchronous orbit
atto	6e-18		6411 km	m288 server sky
atto	3e-17			beamline Large Hadron Collider
femto	1e-15		1250 km	lowest sustainable solar sail
femto	1e-14		778 km	Iridium
pico	2e-12		410 km	International Space Station
nano	1.2e-09		160 km	temporary low earth orbits
micro	6.8e-07		100 km	"edge of space", suborbitals
micro	8.5e-06		85 km	drag zone for suborbital
milli	1.1e-03		50 km
	1.2	1.01 Bar	0 km	Sea level
Kilo	≈ 1e3	1.1 KBar	-11 km	Deepest Ocean

average density from Earth Satellite Parameters, back end papers of Space Mission Analysis and Design, 3rd Ed., Wertz

The air is too dense at ISS altitudes (in the pico zone) to experiment with server sky - thinsats must be in orbit long enough to test maneuvering and to be observed from the earth, in the femto circular orbit zone or higher. Low earth orbits in the nano zone have a million times as much drag, and a suborbital in the micro zone has a billion times as much density as the femto zone.

A suborbital falling for 100 seconds plunges at more than 900 meters per second, and descends almost 50 kilometers, into the "milli zone". A single turn and stop thinsat maneuver takes 300 seconds. Quite impractical for thinsat testing, even inside a vacuum chamber inside the suborbital.