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Cosmic influences upon the basic reference system for GAIA Michael Soffel & Sergei Klioner TU Dresden
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Definition of BCRS (t, x) with t = x 0 = TCB, spatial coordinates x and metric tensor g post-Newtonian metric in harmonic coordinates determined by potentials w, w i IAU-2000 Resolution B1.3
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BCRS-metric is asymptotically flat; ignores cosmological effects, fine for the solar-system dynamics and local geometrical optics
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The cosmological principle (CP): on very large scales the universe is homogeneous and isotropic The Robertson-Walker metric follows from the CP
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Consequences of the RW-metric for astrometry: - cosmic redshift - various distances that differ from each other: parallax distance luminosity distance angular diameter distance proper motion distance
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Is the CP valid? Clearly for the dark (vacuum) energy For ordinary matter: likely on very large scales
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Anisotropies in the CMBR WMAP-data
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/ < 10 for R > 1000 (Mpc/h) -4 (O.Lahav, 2000)
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The WMAP-data leads to the present (cosmological) standard model: Age(universe) = 13.7 billion years Lum = 0.04 dark = 0.23 = 0.73 (dark vacuum energy) H 0 = (71 +/- 4) km/s/Mpc
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One might continue with a hierarchy of systems GCRS (geocentric celestial reference system) BCRS (barycentric) GaCRS (galactic) LoGrCRS (local group) etc. each systems contains tidal forces due to system below; dynamical time scales grow if we go down the list -> renormalization of constants (sec- aber) BUT: expansion of the universe has to be taken into account
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BCRS for a non-isolated system Tidal forces from the next 100 stars: their quadrupole moment can be represented by two fictitious bodies: Body 1Body 2 Mass1.67 M sun 0.19 M Sun Distance1 pc 221.56°285.11° -60.92°13.91°
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In a first step we considered only the effect of the vacuum energy (the cosmological constant ) !
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Various studies: - transformation of the RW-metric to ‚local coordinates‘ - construction of a local metric for a barycenter in motion w.r.t. the cosmic energy distribution - transformation of the Schwarzschild de Sitter metric to LOCAL isotropic coordinates - cosmic effects: orders of magnitude
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Transformation of the RW-metric to ‚local coordinates ‘
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‘ Construction of a local metric for a barycenter in motion w.r.t. the cosmic energy distribution
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(local Schwarzschild-de Sitter)
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Cosmic effects: orders of magnitude Quasi-Newtonian cosmic tidal acceleration at Pluto‘s orbit 2 x 10**(-23) m/s**2 away from Sun (Pioneer anomaly: 8.7 x 10**(-10) m/s**2 towards Sun) perturbations of planetary osculating elements: e.g., perihelion prec of Pluto‘s orbit: 10**(-5) microas/cen 4-acceleration of barycenter due to motion of solar-system in the g-field of -Cen solar-system in the g-field of the Milky-Way Milky-Way in the g-field of the Virgo cluster < 10**(-19) m/s**2
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Conclusions If one is interested in cosmology, position vectors or radial coordinates of remote objects (e.g., quasars) the present BCRS is not sufficient the expansion of the universe has to be considered modification of the BCRS and matching to the cosmic R-W metric becomes necessary
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THE END
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