Two-body orbit from published elements
TESS is placed by solving a Keplerian orbit around earth at the simulation time (a = 250,000 km, e = 0.55, period 13.7 d). Shown from 2018-04-18 onward.
NASA's TESS surveys nearly the whole sky for exoplanets transiting bright nearby stars, from a unique high Earth orbit.
One record per aspect. The origin says what kind of thing each value is; the source says where it came from; the limit says what it cannot tell you.
TESS is placed by solving a Keplerian orbit around earth at the simulation time (a = 250,000 km, e = 0.55, period 13.7 d). Shown from 2018-04-18 onward.
TESS: mass 3.620 × 10^2 kg. These values are bundled with the object record and drive the rendered size.
The close-up shows a published 3D model scaled to 4 m deployed solar-array span. Distributed through NASA 3D Resources; original mission-agency credit applies.
The short description and the fact list are written by the Space Time authors for orientation. They are not quoted from a catalog field and carry no citation of their own.