منابع مشابه
Stellar and Planetary Aberration
For some time the writer has been seeking improved understanding of the several kinds of aberration—these being rather superficially explained in most texts, particularly texts of relativity theory. Indeed, in some of the more highly regarded of these (e.g., Møller 1972) the phenomenon of stellar aberration is so slightingly treated that use of the formulas provided would literally yield wrong ...
متن کاملReference Frames for Stellar Aberration
There is some confusion in the literature as to what velocity should appear in the stellar aberration formula. Because the aberration formula is usually derived from the same equations as the Doppler shift, where the relative velocity between source and detector is the relevant one, it is often assumed the same holds for aberration. This is not the case. Authors who choose the orbital velocity ...
متن کاملRelativistic stellar aberration for the Space Interferometry Mission
This paper analyses the relativistic stellar aberration requirements for the Space Interferometry Mission (SIM). We address the issue of general relativistic deflection of light by the massive self-gravitating bodies. Specifically, we present estimates for corresponding deflection angles due to the monopole components of the gravitational fields of a large number of celestial bodies in the sola...
متن کاملRelativistic stellar aberration for the Space Interferometry Mission: parallax analysis
This paper is a continuation of our previous analysis (i.e. Turyshev 2002a, 2002b) of the relativistic stellar aberration requirements for the Space Interferometry Mission (SIM). Here we have considered a problem of how the expected astrometric accuracy of parallax determination will constrain the accuracy of the spacecraft navigation. We show that effect of the spacecraft’s navigational errors...
متن کاملDoppler Shift, Stellar Aberration, and Convection of Light by Moving Media
The characteristics of a beam of light emanating from a source in uniform motion with respect to an observer differ from those measured when the source is stationary. In general, it is irrelevant whether the source is stationary and the observer in motion or vice versa; the observed characteristics depend only on the relative motion. The observed frequency of the light, for example, has been kn...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1950
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/110.5.467