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World desk5 min

How to Track Asteroid Missions and Read Their Orbital Data

Follow asteroid missions visually with Eyes on Asteroids, then use SBDB and Horizons for orbital elements and time-dependent positions. Learn what each output means and how to check trajectory freshness.
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Use NASA/JPL’s Eyes on Asteroids for a visual overview, the Small-Body Database (SBDB) to look up an asteroid’s orbital elements, and Horizons to calculate where a body will appear over a specified time span. These tools answer different questions: a displayed orbit is useful for orientation, while numerical work requires the right data product and its epoch, coordinate frame, and update status.

Choose the right NASA/JPL tool

Tool Best for What it provides Important qualification
Eyes on Asteroids Getting a visual overview of asteroids, comets, close approaches, and missions Interactive visualization of thousands of small bodies and missions past, present, and future It is an orientation tool; use SBDB or Horizons when you need specific numerical data. The visualization uses CNEOS data. [c001]
SBDB Lookup Identifying a small body and inspecting its orbit and related information Orbital elements, uncertainties where available, orbit diagrams, and other object details The built-in orbit viewer uses two-body methods and is not intended for accurate long-term trajectories or planetary encounter circumstances. [c005]
Horizons Calculating time-dependent positions or generating other numerical output Ephemerides, orbital elements, and SPK trajectory files Results depend on the selected target, observer or reference center, dates, step size, and output settings. Spacecraft trajectories may be outdated. [c002] [c003]

For a general explanation of how orbit descriptions and ephemerides differ, see JPL’s orbits and ephemerides guide. [c008]

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Track a mission or asteroid visually

  1. Open Eyes on Asteroids and select an object or mission in the visualization.
  2. Use the display to understand the broad relationship between the object, its orbit, close approaches, and mission trajectories. The tool also offers a view of the next five close approaches. [c001]
  3. For a specific orbit value, time-stamped position, or precision-sensitive question, continue to SBDB or Horizons rather than treating the visual display as a numerical forecast.

Eyes on Asteroids draws on data from CNEOS, the Center for Near-Earth Object Studies, which computes high-precision orbits for near-Earth objects. Its purpose is to make the overall picture easy to explore, not to replace the data services used for a defined calculation. [c001]

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Look up the object unambiguously in SBDB

  1. Open SBDB Lookup.
  2. Search using an IAU number, formal designation, name, or JPL SPK-ID. Prefer a number or formal designation when a name might refer to more than one object. [c005]
  3. Inspect the available orbital elements and uncertainties along with the object’s other record details, such as physical parameters, close-approach information, radar astrometry, discovery circumstances, and alternate designations. Availability varies by object. [c005]

Do not use SBDB’s orbit viewer to determine accurate long-term trajectories or planetary encounter circumstances: JPL says it uses two-body methods. Use Horizons for those calculations. [c005]

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Know whether you need elements, an ephemeris, or an SPK

Orbital elements describe an orbit at an epoch

Elements are a compact description of orbital geometry or state at a specified time, relative to a selected body or barycenter. They are not timeless constants. Horizons can return an osculating-elements set, meaning an instantaneous representation for the selected epoch and reference. [c003]

Ephemerides give values over time

An ephemeris provides quantities such as sky position and rates across a time interval for a specified observing location. Use one when the question is “Where will this object appear, and when?” rather than “What elements describe its orbit?” [c003]

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SPK files are for downstream software

Horizons can generate SPK files, a binary trajectory format for use in other software workflows. Choose this output when the next step requires a trajectory file rather than a human-readable table. [c002] [c003]

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Read orbital elements with their context

Depending on the selected output, Horizons may list epoch, eccentricity, periapsis distance, inclination, longitude of ascending node, argument of periapsis, mean anomaly, true anomaly, semimajor axis, and period. Read each value together with the metadata that makes it interpretable:

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  • Epoch: the time the element set represents.
  • Reference: the selected body or barycenter and reference plane or frame.
  • Coordinate system and units: the conventions used for the output.
  • Uncertainty: the SBDB record includes orbital-element uncertainties where available; retain them when using the values for observation, hazard, or mission planning. [c002] [c003]

Orbit solutions are fitted to astrometric observations using debiasing, weighting, perturbation models, and numerical methods. As observations accumulate, the solution can improve, so a quoted value should be tied to the specific solution or retrieval date rather than presented as permanent. [c006]

Request Horizons output deliberately

Horizons can be used interactively or through its API. The API supports observer ephemerides, orbital elements, and SPK output; requests need a valid target command and settings appropriate to the question. [c003]

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  • Choose the target carefully, using an unambiguous designation or identifier.
  • Select the observer or center that matches the question: an apparent sky position depends on where it is observed from.
  • Set the start and end times and the step size for a time series.
  • Select only the output quantities you need, then confirm the reported units and coordinate conventions.
  • For API use, follow JPL’s URL-encoding requirements and the documented parameter names rather than assembling a request by guesswork. [c003]

These choices define what the result means. An ephemeris for one observer and interval is not interchangeable with an orbital-element set or a view from another location.

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Check spacecraft trajectory freshness before relying on it

Asteroid orbit solutions and spacecraft trajectories do not necessarily update on the same schedule. The Horizons manual warns that externally produced spacecraft trajectories may lag planning changes or maneuvers. In the spacecraft data sheet, check the revision date in the upper-left corner and read the comments for mission-status information. [c003]

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The manual states: “Always check the revision date in the upper left corner of the Horizons spacecraft data-sheet to determine the last time the spacecrafts’ trajectory was updated, and read the data-sheet comments for mission status information.” For high-precision interplanetary applications, JPL advises contacting Solar System Dynamics if the revision status is uncertain. Do not infer current navigation status from an old trajectory alone. [c003]

Check mission targets and close-approach context

JPL’s selected small-body mission-target table lists target body, mission type, arrival, mission name, launch, and status, with links to SBDB and mission pages where available. Its entries change over time, so consult the live table for current status and dates rather than relying on a saved arrival date. [c004]

For context on risk terminology, NASA/JPL’s Asteroid Watch defines potentially hazardous asteroids as asteroids more than about 460 feet (140 meters) in size whose orbits bring them within 4.6 million miles (7.5 million kilometers) of Earth’s orbit around the Sun. This classification is not a statement that an object is on an impact trajectory. [c007]

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