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Occultation events / predictions

CeTNOs prediction coverage: 2023-12-29 to 2030-01-01.
Coverage of all prediction databases
DatabaseFirst date (UTC)Last date (UTC)Status
Asteroids2026-03-262026-07-02 Expired
CeTNOs2023-12-292030-01-01 Includes future dates
NEOs2025-11-292027-01-02 Includes future dates
PHAs2025-11-292027-01-02 Includes future dates
Comets2024-01-012028-01-01 Includes future dates
Special2023-01-012026-12-18 Includes future dates

Worldwide stored predictions, before your search filters. Date ranges do not imply continuous coverage. Coverage summaries refresh within five minutes.

(Start date, Format: yyyy-mm-dd or yyyy-mm or yyyy)
(Ende date, Format: yyyy-mm-dd or yyyy-mm or yyyy)
(If checked the date filter is active. Otherwise query the whole db date range)
(Longitude Latitude in deg (Lng. > 0 to the East) OR MPC code (XXX))
(Free name, just for the header. Optional)
(Show events with this minimum occultation probability 0-100% at observer site. See info below !)
(Show events with maximum altitude of the sun at observing site below this limit (for t0))
(If checked the site filter constraints are active. If unchecked => 'worldwide')
(Filter for object name: examples: (41), Pallas, 1997 RB7)
(Show events with object diameter larger than this)
(Show events down to this star magnitude)
(Just objects with selected tag)
(Sort resulting table according to this criteria)
(Select database with occultation events (see explanation at bottom))
 
(Depending on your input response may take some ten seconds!)

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Basic information and usage

Usage: As quick start you only have to enter the latitude and longitude of your observing site in decimal degrees (long: + is east of Greenwich), seperated by a comma or space. Alternatively you can enter the 3-letter MPC station code (always in the form XXX, even for stations 000...099). In that case the site name will be taken from the MPC record.

Min P1: For asteroids, a high P1 (~ 50% or more) filters events close to your site. For CeTNOs, Comets, PHAs, and NEOs, use a much lower P1 (~ 3-10% or less), as their probabilities are generally small(er). P1 is computed on the fundamental plane, not on the Earth’s surface, so it may be imperfect. If too few events appear, lower P1 or disable the distance filter.

Occultation Databases

Asteroids: This database contains worldwide predictions of stellar occultations by asteroids. See the coverage summary above for the dates currently stored. Predictions are for asteroids (sometimes plus some special targets) with diam > 10 km and Gaia DR3 stars brighter than G = 15 mag.

CeTNOs: This database contains occultations by Centaurs (diam > 50 km) and TNOs (diam > 150 km) over the stored date range shown above. Gaia DR3 stars brigther than G = 18 mag.

Comets: A small list of numbered comets with expected diameter > 5 km (JPL SBDB). Currently ~25 comets. Gaia (e)DR3 stars brighter than G = 15 mag.

NEOs & PHAs: Contains those objects listed in the corersponding MPC files NEA.txt and PHA.txt. These DBs are seperated, but overall are a subset of the Asteroids DB.

Several other databases for special purposes or dedicated projects.

Orbits and ephemerides: JPL Horizons (JPLH) ephemerides are used by default. CORA bulk ephemerides, which are also high precision due to a sophisticated integrator and dynamic model, use astorb.dat elements (Moskovitz+2022) and are indicated by "PEE+ASTORB(epoch)" as the orbit reference. CORA's own orbit solutions are indicated by "CORA+some version indicator".

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