Apparent Positions of Planets
Chol Jun Kim, Kyong Il Pak, Sin Chol Hwang, Chol Min Choe, Jin Hyok, Choe, Ui Ri Mun

TL;DR
This paper develops a system for calculating the apparent positions of planets using updated models and compares the results with established references, confirming their accuracy.
Contribution
It introduces a new system based on recent models for precise planetary position calculations and validates it against authoritative sources.
Findings
Results agree with the Astronomical Almanac
Updated models improve calculation accuracy
System confirms correctness of planetary positions
Abstract
The apparent positions of planets are determined by means of the fundamental ephemerides, the precession-nutation models of the Earth, the gravitational effects and aberrations et al. Around 2000, many astrometrical conceptions, models and theories had been newly defined and updated:for the fiducial celestial reference system, the ICRS is introduced, the fundamental ephemerides - DE405/LE405 et al.,precession-nutation model - IAU 2000A/IAU 2006 model. Using the traditional algorithm and the updated models, we develop the system of calculating the apparent positions of planets. The results are compared with the Astronomical Almanac and proved in their correctness.
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Inertial Sensor and Navigation · Geophysics and Gravity Measurements
