jorbit 1.3.1

Solar system orbit fitting and integration with JAX

jorbit is a python/JAX package for simulating and fitting orbits of objects within the solar system. Built primarily in JAX, jorbit can compute exact derivatives even for models that involve complex numerical integrators, like IAS15, and acceleration functions, like Parameterized Post-Newtonian gravitation. It has several high-level convenience wrappers for dealing with standard massless minor planets, but also can enable more complex simulations through user-provided acceleration functions.

For more information, check out the documentation!

Installation

Exact installation instructions may depend on your hardware/environment, so see the installation page for more information. In general, you can install jorbit with pip:

Be aware! The first time you import jorbit, it will automatically download and cache (via the astropy caching mechanisms) about ~1 GB of files required to run its simulations, including the JPL DE400 ephemeris files. Other jorbit functions may also need to download/cache additional files, so be sure to have a good internet connection and enough disk space available.

python -m pip install -U jorbit

jorbit was built with uv, so if you want to replicate the exact development environment, use the uv.lock file. Check out the uv docs for more information.

Example Usage

Many more examples can be found in the docs, but here are two simple examples to get you started:

To create an ephemeris for a minor planet:

from astropy.time import Time
from jorbit import Particle

p = Particle.from_horizons(name="274301", time=Time("2025-01-01"))
ephem = p.ephemeris(
    times=Time(["2025-01-01", "2025-01-02", "2025-01-03"]),
    observer="Kitt Peak"
)

To identify all known minor planets nearby a certain position at a certain time:

import astropy.units as u
from astropy.coordinates import SkyCoord
from astropy.time import Time

from jorbit.mpchecker import mpchecker

mpchecker(
    coordinate=SkyCoord(ra=0 * u.deg, dec=0 * u.deg),
    time=Time("2025-01-01"),
    radius=10 * u.arcmin,
    extra_precision=True,
    observer="Palomar",
)

Contributing

If you have any trouble with the code, feel free to open an issue! We welcome open-source contributions, so if you have a feature request or bug fix, please open a pull request. For more information, see the contributing guide.

Attribution

jorbit is made freely available under the GPL License. If you use this code in your research, please cite the accompanying paper:

@ARTICLE{2025PSJ.....6..252C,
       author = {{Cassese}, Ben and {Rice}, Malena and {Lu}, Tiger},
        title = "{A High-precision, Differentiable Code for Solar System Ephemerides}",
      journal = {\psj},
     keywords = {Astronomy software, Solar system, Orbit determination, Bayesian statistics, 1855, 1528, 1175, 1900, Earth and Planetary Astrophysics, Instrumentation and Methods for Astrophysics},
         year = 2025,
        month = nov,
       volume = {6},
       number = {11},
          eid = {252},
        pages = {252},
          doi = {10.3847/PSJ/ae0a36},
archivePrefix = {arXiv},
       eprint = {2509.19549},
 primaryClass = {astro-ph.EP},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025PSJ.....6..252C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}