An upper limit for the solar acceleration

Details An upper limit for the solar acceleration An upper limit for the solar acceleration

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.213p..27t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 213, March 1, 1985, p. 27P, 28P. Research supported by

Astronomy and Astrophysics

Astronomy

1

Center Of Gravity, Companion Stars, Pulsars, Solar System, Solar Velocity, Black Holes (Astronomy), Neutron Stars, Relativity

Scientific paper

It has been suggested that the Sun may be a member of a binary star system. In this case, the barycentre of the (known) Solar System would be accelerated towards the companion object. Consideration of the binary pulsar PSR 1913+16's orbital motion gives an upper limit of |a| ⪉ 10-9m s-2 for the component of any Solar System acceleration in its direction.

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