Orbit from osculating elements
67P/Churyumov-Gerasimenko is placed by solving a Keplerian orbit at the simulation time (a = 3.5 AU, e = 0.641, i = 7°, period 2,349.7 d).
Jupiter-family comet explored up close by ESA's Rosetta mission and Philae lander.
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.
67P/Churyumov-Gerasimenko is placed by solving a Keplerian orbit at the simulation time (a = 3.5 AU, e = 0.641, i = 7°, period 2,349.7 d).
67P/Churyumov-Gerasimenko: mean radius 1.7 km. These values are bundled with the object record and drive the rendered size.
The nucleus, coma and tail are identification geometry. Tail direction follows the propagated orbit and the Sun direction; the local shape is representative.
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.
| Dataset | Last refreshed | Horizon | Automated |
|---|---|---|---|
| Searchable comet catalog (all comets) | no snapshot date | Every JPL comet record with elements and photometric parameters | Yes, weekly (Monday data job) npm run generate:comets |