An Astronomical Re-Appraisal of the Star of Bethlehem - A Nova in 5 BC

Details An Astronomical Re-Appraisal of the Star of Bethlehem - A Nova in 5 BC An Astronomical Re-Appraisal of the Star of Bethlehem - A Nova in 5 BC

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977qjras..18..443c&link_type=abstract

Quarterly Journal of the Royal Astronomical Society, Vol. 18, p.443-449

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Evidence is presented that New Stars recorded in the Far Eastern annals may be
independent sightings of the Star of Bethlehem. A bright nova which appeared
in the spring of 5 BC appears to be the most likely explanation of the event.
The Jupiter-Saturn planetary conjunction hypothesis of Kepler, perpetuated by
several subsequent investigators, receives its quietus

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