Support for stellar catalogs
Conversion from star catalog mean place to apparent
place, topocentric place, and local horizon coordinates
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Apparent place: Position of star at some date and time
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In the coordinates system defined by the true equator and equinox
of date
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Ignoring atmospheric refraction
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As seen from the Earth's center of mass
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Topocentric place: Position of star
at some date and time
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In the coordinate system defined by the true equator and equinox
of date
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Ignoring atmospheric refraction
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As seen from a specific location on Earth
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Local horizon coordinates: Position of star at some date and time
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In local azimuth and elevation coordinates
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Including atmospheric refraction (optional)
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As seen from a specific location on Earth
Time conversions among UT1, UTC, TAI, TDT, TDB
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UT1 – Time corresponding to Earth rotation
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UTC – Universal coordinated time (Civil time)
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TAI – Atomic time
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TDT – Terrestrial dynamic time (TAI + 32.184 sec)
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TDB – Barycentric dynamic time (removes general relativistic tidal
effects from TDT)
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General conversion chain:
TDB ↔ TDT ↔ TAI ↔ UTC ↔ UT1
ECF ↔ ECI conversion using quaternions
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XECI = q XECF q*
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q = qP* qN* qS qW
expresses that attitude of the ECF system relative to the ECI
system
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qP (precession) accounts for precession of the mean celestial
system
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qN (nutation) accounts for the nutation correction from the mean
celestial system of date
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qS (spin) accounts for earth rotation
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qW (wobble) accounts for polar motion
Earth Orientation Parameters
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Precision offsets and corrections that must be measured, not
computed
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Interpolated from files containing the IERS CO4 solution (daily values from 1962
to present)
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