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Star in the constellation Vela
Phi Velorum (φ Vel, φ 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
Phi_Velorum
Combined magnitude derived from adding the magnitudes of Gamma2 Velorum (1.83) and Gamma1 Velorum (4.173 ± 0.009) as per the formula: 1.71 ≈ − 2.5 log 10
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
American astronaut and pilot (1935–1967)
involved in the fraternity Phi Kappa Sigma. He transferred to Purdue University in 1954, continuing his involvement in Phi Kappa Sigma serving as chapter
Roger_B._Chaffee
Multiple star system in the constellation Hercules
different meanings) is also the Chinese name of the stars Phecda and λ Velorum (Suhail). van Leeuwen, F. (November 2007), "Validation of the new Hipparcos
Zeta_Herculis
not documented in Yixiang Kaocheng. Sun & Kistemaker (p. 186) identify q Velorum as the principal star, citing the star catalogue of Zhou Cong of the Song
List_of_Chinese_star_names
Type of star cluster
Ptolemy Cluster, while the Persian astronomer Al-Sufi wrote of the Omicron Velorum cluster. However, it would require the invention of the telescope to resolve
Open_cluster
companion star. Zeta Puppis (Naos) 1,080 ± 40 1 O4If(n)p 2.24 - 2.26 Gamma² Velorum B (Regor) 1096+26 −23 2 O7.5III 1.83 Has a Wolf-Rayet companion star. Theta²
List_of_O-type_stars
; Colling, M. D.; Barlow, M. J. (2012-11-21). "The Outer Wind of gamma Velorum". Monthly Notices of the Royal Astronomical Society. 427 (1): 581–588.
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Idealized physical body that absorbs all incident electromagnetic radiation
reflectivity, and transmissivity". Fundamentals of heat and mass transfer. PHI Learning Pvt. Ltd. pp. 385–386. ISBN 978-81-203-4031-2. Planck 1914, p. 10
Black_body
A:57.9 ± 0.5 B:58.91 ± 0.07 +4.59 (4.60 + 7.15) F6 V + ? + K0 351 Psi Velorum Vela 61.4 ± 0.4 +3.58 (3.91 + 5.12) F0 IV + F3 IV 354 Theta Ursae Majoris
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
Star whose brightness fluctuates, as seen from Earth
magnitude are known as AI Vel-type variables, after their prototype, AI Velorum. SX Phoenicis variables These stars are metal-poor, population II analogues
Variable_star
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PHI VELORUM
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PHI VELORUM
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