Call to adopt a nominal set of astrophysical parameters and constants to improve the accuracy of fundamental physical properties of stars
Petr Harmanec, Andrej Pr\v{s}a

TL;DR
This paper proposes adopting a standardized set of nominal astrophysical parameters and constants to eliminate systematic errors in stellar property measurements, enhancing the precision of astronomical data analysis.
Contribution
It introduces a framework for using exact nominal values for solar parameters and fundamental constants to improve stellar property accuracy.
Findings
Nominal solar radius and luminosity are defined as exact SI values.
Stellar masses should be computed using the product G.Msun, where G is measured separately.
Explicit reference to fundamental constants enhances clarity and consistency.
Abstract
The increasing precision of astronomical observations of stars and stellar systems is gradually getting to a level where the use of slightly different values of the solar mass, radius and luminosity, as well as different values of fundamental physical constants, can lead to measurable systematic differences in the determination of basic physical properties. An equivalent issue with an inconsistent value of the speed of light was resolved by adopting a nominal value that is constant and has no error associated with it. Analogously, we suggest that the systematic error in stellar parameters may be eliminated by: (1) replacing the solar radius Rsun and luminosity Lsun by the nominal values that are by definition exact and expressed in SI units: 1 RnomSun = 6.95508 x 10^8 m and 1 LnomSun = 3.846 x 10^{26} W; (2) computing stellar masses in terms of Msun by noting that the measurement error…
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