Pi1 Columbae is a star in the southern constellation of Columba. Its name is a Bayer designation that is Latinized from π1 Columbae, and abbreviated Pi1 Col or π1 Col. With an apparent visual magnitude of 6.13, it is a dim, white-hued star that is near the limit of visibility for the naked eye. It is located at a distance of approximately 280 light-years (86 pc) from the Sun based on parallax, and has an absolute magnitude of +1.55. This is an Am star with a stellar classification of A2mA5-A9, which means it is a chemically peculiar star that displays strong absorption lines of higher mass elements in its spectrum. At an estimated age of 1.1 billion years, this star is spinning with a projected rotational velocity of 70 km/s. It has 1.75 times the mass of the Sun and 2.5 times the Sun's radius. The star is radiating 20 times the luminosity of the Sun from its photosphere at an effective temperature of 7,765 K. A 2024 study of stellar pulsation in Am and Fm stars suggested that π1 Col is a Gamma Doradus variable.
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