Determination of the barycentric velocity of an astrometric satellite using its own observational data

TL;DR

This paper investigates how to accurately determine an astrometric satellite's orbital velocity from its own data, addressing degeneracies and constraints to improve velocity estimation for high-precision astrometry.

Contribution

It introduces a mathematical framework with constraints for recovering satellite velocity from observational data, applicable to various astrometric missions.

Findings

Velocity and astrometric parameters can be reliably estimated with constraints

Numerical simulations confirm the effectiveness of the proposed method

The approach is applicable to both scanning and pointing astrometric missions

Abstract

The problem of determination of the orbital velocity of an astrometric satellite from its own observational data is studied. It is well known that data processing of microarcsecond-level astrometric observations imposes very stringent requirements on the accuracy of the orbital velocity of the satellite (a velocity correction of 1.45 mm/s implies an aberrational correction of 1 $\mu$as). Because of a number of degeneracies the orbital velocity cannot be fully restored from observations provided by the satellite. Seven constraints that must be applied on a velocity parameterization are discussed and formulated mathematically. It is shown what part of velocity can be recovered from astrometric data by a combined fit of both velocity parameters and astrometric parameters of the sources. Numerical simulations show that, with the seven constraints applied, the velocity and astrometric parameters can be reliably estimated from observational data. It is also argued that the idea to improve the velocity of an astrometric satellite from its own observational data is only useful if the a priori information on the orbital velocity justifies the applicability of the velocity constraints. The proposed model takes into account only translational motion of the satellite and ignores any satellite-specific parameters. Therefore, the results of this study are equally applicable to both scanning missions similar to Gaia, and pointing ones like SIM, provided that enough sources were observed sufficiently uniformly.