HD 61330 (f Puppis) is a binary star in the constellation Puppis. Its apparent magnitude is 4.53 and it is approximately 360 light years away based on parallax.
The primary and secondary, with respective labels A and C, take 78 years to complete an orbit, with a considerable eccentricity of 0.655. Another closer component, B, has been reported at 6.1 magnitude and 0.1" separation, but subsequent observers have repeatedly failed to confirm it. Vizier catalog entry
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