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The primary component, Psi Velorum A, is a yellow-white F-typesubgiant with an apparent magnitude of +4.1. The companion, Psi Velorum B, is a yellow-white F-type main sequence dwarf, with an apparent magnitude of +4.6. The two stars are 0.68 arcseconds, or at least 12 astronomical units, apart and complete one orbit every 33.99 years.