Orbit from osculating elements
C/1995 O1 (Hale-Bopp) is placed by solving a Keplerian orbit at the simulation time (a = 186 AU, e = 0.995, i = 89.4°, period 926,000 d).
The Great Comet of 1997. One of the most widely observed comets of the 20th century, visible to the naked eye for 18 months.
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.
C/1995 O1 (Hale-Bopp) is placed by solving a Keplerian orbit at the simulation time (a = 186 AU, e = 0.995, i = 89.4°, period 926,000 d).
C/1995 O1 (Hale-Bopp): mean radius 30 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 |