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Increase of the mean Sun-Earth distance caused by a secular mass accumulation

dc.contributor.authorWilhelm K.; Dwivedi B.N.
dc.date.accessioned2025-05-24T09:18:10Z
dc.description.abstractBased on many planetary observations between the years 1971 and 2003, Krasinsky and Brumberg (Celest. Mech. Dyn. Astron. 90:267-288, 2004) have estimated a rate of increase in the mean Sun-Earth distance of (15±4) m per century. Together with other anomalous observations in the solar system, this increase appears to be unexplained (Lämmerzahl et al. in Astrophys. Space Sci. Lib., vol. 349, pp. 75-101, 2008). We explain these findings by invoking a recently proposed gravitational impact model (Wilhelm et al. in Astrophys. Space Sci. 343:135-144, 2013) that implies a secular mass increase of all massive bodies. This allows us to formulate a quantitative understanding of the effect within the parameter range of the model with a mass accumulation rate of the Sun of (6.4±1.7)×1010 kg s-1. © 2013 Springer Science+Business Media Dordrecht.
dc.identifier.doihttps://doi.org/10.1007/s10509-013-1487-1
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/13839
dc.relation.ispartofseriesAstrophysics and Space Science
dc.titleIncrease of the mean Sun-Earth distance caused by a secular mass accumulation

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