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Binary star in the constellation Canis Major
further away with a radial velocity of +32 km/s. ζ Canis Majoris, Latinized from Zeta Canis Majoris, is the star's Bayer designation assigned by the German
Zeta_Canis_Majoris
Constellation in the southern celestial hemisphere
2013). "Eta Canis Majoris". AAVSO Website. American Association of Variable Star Observers. Retrieved 5 February 2014. "Zeta Canis Majoris – Cepheid Variable"
Canis_Major
Variable star in constellation Canis Major
Omicron2 Canis Majoris is a massive variable star in the constellation Canis Major. Its name is a Bayer designation that is Latinized from ο2 Canis Majoris, and
Omicron2_Canis_Majoris
lion's mane) الضفيرة الْضَّفِيرَة Zeta Leonis Adhara al-ʽAthara the Virgin / Nymph العذارى الْعَذَارَى Epsilon Canis Majoris A Adhil adh-Dhayl the Tail / Annex
List_of_Arabic_star_names
Ursae Majoris Star 3.01 Gamma Gruis (Aldhanab) Star 3.01 Beta Capricorni Quintuple star system 3.02 2.97 Omicron2 Canis Majoris Star 3.03 2.88 Zeta Tauri
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Direction the Sun travels relative to local standard of rest
the direction opposite of the solar apex, is located near the star Zeta Canis Majoris. Animations of star motions around apex and antapex The movement of
Solar_apex
confirmed exoplanets (b,c). K2-198 362 G Has 3 exoplanets. Zeta Canis Majoris (Furud) 362 ± 5 Canis Major B2.5 V 3.025 TOI-125 363 G Has 3 confirmed and 2
List of star systems within 350–400 light-years
List_of_star_systems_within_350–400_light-years
Hot, luminous star with a spectral type of A9 or earlier
supergiant Eta Canis Majoris, a blue supergiant of spectral type B5Ia UW Canis Majoris (UW CMa), two blue (O-type) supergiants in a binary system Zeta Puppis
Blue_supergiant
Philip; Levesque, Emily M.; Plez, Bertrand (2006-08-01). "Bringing VY Canis Majoris down to size: an improved determination of its effective temperature"
List_of_nearest_hypergiants
Second-brightest star in the constellation of Puppis
consisting of π Puppis, δ Canis Majoris, η Canis Majoris, HD 63032, HD 65456, ο Puppis, k Puppis, ε Canis Majoris and κ Canis Majoris. Consequently, π Puppis
Pi_Puppis
Ara Aries Auriga Boötes Caelum Camelopardalis Cancer Canes Venatici Canis Major Canis Minor Capricornus Carina Cassiopeia Centaurus Cepheus Cetus Chamaeleon
Lists_of_stars
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
DFK 1 UY Scuti V602 Carinae V1749 Cygni VV Cephei A VX Sagittarii VY Canis Majoris - potentially the largest star known in the Milky Way Westerlund 1 W26
Hypergiant
J. Michael; Curran, Rachel M.; Topping, Michael W. (2025). "Epsilon Canis Majoris: The Brightest Extreme-ultraviolet Source with Surprisingly Low Interstellar
Historical_brightest_stars
Star in the constellation Columba
IAU-approved Star Names. (The historical form Furud was chosen for Zeta Canis Majoris.) In Chinese, 孫 (Sūn), meaning Grandson, refers to an asterism consisting
Theta_Columbae
Stars with a supergiant luminosity class with a spectral type of K or M
sometimes used for the most extended and unstable red supergiants like VY Canis Majoris and NML Cygni. The "red" part of "red supergiant" refers to the cool
Red_supergiant
Cassiopeia 3,440+930 −610 G2Ia0e Yellow hypergiant IIL VY Canis Majoris 07h 22m 58.3s −25° 46′ 03″ Canis Major 3,930+420 −350 M5eIa Red hypergiant II IRAS 17163-3907
List_of_supernova_candidates
Stellar classification
4 visibly bright O-type stars are Gamma Velorum, Alnitak (Zeta Orionis), Mintaka (Delta Orionis), and Zeta Puppis. Walborn, N. R.; Fitzpatrick, E.L. (1990). "Contemporary
O-type_star
M3 IIIab 5.47±0.01 Beta Sextantis 404 Sextans B5V Epsilon Canis Majoris (Adhara) 405 ± 7 Canis Major B2 II or B2 III-II 1.50 K2-148 407 K7V Has 3 exoplanets
List of star systems within 400–450 light-years
List_of_star_systems_within_400–450_light-years
Classification of stars based on spectral properties
Example spectral standards: F0IIIa – Zeta Leonis F0Ib – Alpha Leporis F1V - 37 Ursae Majoris F2V – 78 Ursae Majoris F7V - Iota Piscium F9V - Beta Virginis
Stellar_classification
star. HD 49798 1,700 ± 46 1 sdO6p 10 Lacertae 1,800±103 1 O9V 4.880 FY Canis Majoris B 1,820 ± 70 2 sdO 4.8 - 6.25 Has a B-type companion star. Mu Columbae
List_of_O-type_stars
Silva, L.; Porto de Mello, G. F. (2000-06-01). "zeta 1 and zeta 2 Reticuli and the existence of the zeta Herculis group". Astronomy and Astrophysics. 358:
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
G-type star in the constellation Puppis
seen east of Sirius, southwest of Procyon, northeast of Delta Canis Majoris, and north of Zeta Puppis. On May 17, 2006, a team of astronomers using the European
HD_69830
Type of eruptive variable star
W. W. (2006-09-16). "MOST Detects g -Modes in the Late-Type be Star β Canis Minoris (B8 Ve)". The Astrophysical Journal. 654: 544–550. arXiv:astro-ph/0609460
Gamma_Cassiopeiae_variable
Type of star
B2/B3Vnn 303 HD 128207 5.73 B8V 0.48 147 HD 27563 5.84 B5III 3.80 242 26 Canis Majoris 5.90 B2IV/V 2.73 257 16 Monocerotis 5.92 B3V 1.94 263 V335 Velorum 5
Slowly_pulsating_B-type_star
System of two stars orbiting each other
was computed in 1827, when Félix Savary computed the orbit of Xi Ursae Majoris. Over the years, many more double stars have been catalogued and measured
Binary_star
40 Upsilon³ Eridani (Beemim) 296 ± 10 Eridanus K4 III 3.96 NR Canis Majoris 297 ± 2 Canis Major F2V 5.60 System Star or (sub-) brown dwarf Distance (ly)
List of star systems within 250–300 light-years
List_of_star_systems_within_250–300_light-years
997 M0V b c 331 Iota Ursae Majoris (Talitha) Ursa Major 47.3 ± 0.1 3.14/10.1/10.3 A7V(n) + M3V + M4V 332 10 Ursae Majoris Lynx 52.4 ± 0.6 3.960 (4.18
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
10.44 392.7529 ±0.0321 two known planets (2019, 2021) Sirius (Alpha Canis Majoris) A$ 8.7094 ±0.0054 CMa* 06h 45m 08.9s −16° 42′ 58″ A1V 2.063 −1.46#
List_of_nearest_stars
Constellation in the northern celestial hemisphere
constellations: Icarius as Boötes, Erigone as Virgo, and Maera as Canis Major or Canis Minor. Following another reading, the constellation is identified
Boötes
Visible star that is nearly aligned with Earth's axis of rotation
South Star at about 2,800 BC and will become the South Star at 22,000 AD Alpha Canis Majoris Sirius −1.46 Canis Major Will be the South Star in 66,270 AD
Pole_star
Detection of AlO (X2Σ+): Metal Oxide Chemistry in the Envelope of VY Canis Majoris", Astrophysical Journal, 694 (1): L59–L63, Bibcode:2009ApJ...694L..59T
List of interstellar and circumstellar molecules
List_of_interstellar_and_circumstellar_molecules
HD 8535 A 180.5 ± 0.2 G0V 7.70 B D Omicron Ursae Majoris (Muscida) 182 ± 1 Ursa Major G5III: 3.35 Zeta Andromedae (Shimu) Aa$ 181±2 Andromeda 00h 47m 20
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
Large self-illuminated object in space
Size comparison of some well-known supergiant and hypergiant stars, featuring Cygnus OB2-12, V382 Carinae, Betelgeuse, VV Cephei, and VY Canis Majoris
Star
Fire. The Well Mansion corresponds to constellations Auriga, Cancer, Canis Major, Canis Minor, Carina, Columba, Gemini, Monoceros, Orion, Pictor, Puppis and
List_of_Chinese_star_names
Class of eclipsing binary stars
distinguishes them from the so-called beta Lyrae variables and W Ursae Majoris variables, where the two components are so close that gravitational effects
Algol_variable
68 Has three confirmed exoplanet (HD 37124b, c & d). Alkaid (Eta Ursae Majoris) 103.9 ± 0.8 Ursa Major 13h 47m 32.43776s +49° 18′ 47.7602″ B3 V +1.86
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
3 Columba 05h 50m 57.5929s −35° 46′ 05.915″ K1III_CN+1 3.105# 37 Ursae Majoris 87.34 ± 0.14 Ursa Major 10h 35m 09.62s +57° 04′ 57.2″ F2V 5.148 HD 4838
List of star systems within 85–90 light-years
List_of_star_systems_within_85–90_light-years
Constellation split into two non-contiguous parts
similar to those seen in the supernova SN 1987A. MWC 922 itself is an FS Canis Majoris variable, meaning that it is a Be star containing exceptionally bright
Serpens
27.81s +6° 11′ 10.5″ 22 F7V b 63.4 1.12 3.06036 0.045 0 2010 Xi Ursae Majoris B Ursa Major 11h 18m 12s +31° 32′ 15″ 4.73 25.11 F8.5V b 37 3.98 0.06 0
List_of_brown_dwarfs
Star system in the constellation of Indus
coordinates RA=10h 03m 21s, Dec=56° 47′ 10″, which is located near Beta Ursae Majoris. The absolute magnitude of the Sun is 4.8, so, at a distance of 3.63 parsecs
Epsilon_Indi
Phoenix 01h 39m 21.7s −39° 36′ 09″ M4.5V 14.403 114.604±0.0402 Xi Ursae Majoris Aa (Alula Australis)$ 28.49±0.11 Ursa Major 11h 18m 10.9s +31° 31′ 45″
List of star systems within 25–30 light-years
List_of_star_systems_within_25–30_light-years
Chemical compound
envelopes in CRL 2688 (alongside HCP) and oxygen-rich envelopes toward VY Canis Majoris, TX Camelopardalis, R. Cassiopeiae, and NML Cygni. ALMA data alongside
Phosphorus_mononitride
Reported for reference Brightest star other than the Sun Sirius (Alpha Canis Majoris) prehistoric m= −1.46 List of brightest stars Dimmest star from the
List_of_star_extremes
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