B Velorum

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The Bayer designations b Velorum and B Velorum are distinct. Due to technical limitations, both designations link here. For the star

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<span class="mw-page-title-main">Vela (constellation)</span> Constellation in the southern celestial hemisphere

Vela is a constellation in the southern sky, which contains the Vela Supercluster. Its name is Latin for the sails of a ship, and it was originally part of a larger constellation, the ship Argo Navis, which was later divided into three parts, the others being Carina and Puppis. With an apparent magnitude of 1.8, its brightest star is the hot blue multiple star Gamma Velorum, one component of which is the brightest Wolf-Rayet star in the sky. Delta and Kappa Velorum, together with Epsilon and Iota Carinae, form the asterism known as the False Cross. 1.95-magnitude Delta is actually a triple or quintuple star system.

<span class="mw-page-title-main">Delta Velorum</span> Triple star system in the constellation Vela

Delta Velorum is a triple star system in the southern constellation of Vela, near the border with Carina, and is part of the False Cross. Based on parallax measurements, it is approximately 80.6 light-years from the Sun. It is one of the stars that at times lies near the south celestial pole due to precession.

<span class="mw-page-title-main">Phi Velorum</span> Star in the constellation Vela

Phi Velorum is a star in the constellation Vela. It is a blue-white B-type supergiant with an apparent magnitude of +3.53. It is approximately 1,590 light years from Earth.

The Bayer designations n Velorum and N Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations c Velorum and C Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations a Velorum and A Velorum are distinct. Due to technical limitations, both designations link here. For the star

H.R. 3440 may refer to:

<span class="mw-page-title-main">Omicron Puppis</span> Variable Star in the constellation Puppis

Omicron Puppis (ο Puppis) is candidate binary star system in the southern constellation of Puppis. It is visible to the naked eye, having a combined apparent visual magnitude of +4.48. Based upon an annual parallax shift of 2.30 mas as seen from Earth, it is located roughly 1,400 light years from the Sun.

The Bayer designations q Velorum and Q Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations b Carinae and B Carinae are distinct and the designation b Carinae is shared by two stars in the constellation Carina:

The Bayer designations d Velorum and D Velorum are distinct. Due to technical limitations, both designations link here.

The Bayer designations e Velorum and E Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations f Velorum and F Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations h Velorum and H Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations i Velorum and I Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations k Velorum and K Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations l Velorum and L Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations m Velorum and M Velorum are distinct. Due to technical limitations, both designations link here. For the star

The Bayer designations b Centauri and B Centauri are distinct. Due to technical limitations, both designations link here. For the star