The Earth'’s orbit has a radius of 1.5∙1011 m, and that of Venus has a radius of 1.1 ∙ 1011 m. Consider these two orbits to be perfect circles (though in reality they are ellipses with slight eccentricity). Write the direction and length of a vector from Earth to Venus (take the direction from Earth to Sun to be 0°) when Venus is at the maximum angular separation in the sky relative to the Sun.
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