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Binary star system in the constellation Orion
Nu Orionis (ν Orionis) is a binary star system in the northeastern part of the constellation Orion. It should not be confused with the variable star NU
Nu_Orionis
Quadruple star system in the constellation Orion
NU Orionis (HD 37061) is a quadruple star system in the Orion constellation. It is located in the emission nebula Messier 43 and is the main star ionizing
NU_Orionis
Constellation straddling the celestial equator
and Pi Orionis), and instead of an arm marked out by Mu Orionis, he holds a club (Chi Orionis). His right leg is represented by Theta Orionis and his
Orion_(constellation)
Emission nebula in the constellation Orion
complex. The main ionizing star in this nebula is the quadruple star system NU Orionis (HD 37061), the focus of the H II region, 1,360 ± 30 ly (417.0 ± 9.2 pc)
Messier_43
Binary star system in the constellation Orion
main-sequence star, Nu Orionis, which is somewhat closer at 520 light-years' distance. The apparent visual magnitude of Xi Orionis is 4.47, which is bright
Xi_Orionis
Astronomical treatise by Claudius Ptolemy
north of the zodiac, and 15 to the south. For instance, the stars nu Orionis and 62 Orionis which are now around ecliptic longitude 91° are attributed longitudes
Almagest
Dust ring surrounding large stars thousands of solar radii wide
confirmed proplyds. It was also the first instance where a B-type star, 42 Orionis is responsible for the photoevaporation. In addition, 4 clear and 4 candidate
Proplyd
Star in the constellation Orion
Tau Orionis (τ Ori, τ Orionis) is a binary star in the constellation Orion. If an imaginary line is drawn north-west between the stars Rigel and Mintaka
Tau_Orionis
77 Theta1 Orionis C1 1340±65 O6Vp 33±5 10.6±1.5 204,000 5.13 S Monocerotis Aa 920+150 −110 O7V((f))zvar 29.1 9.9 214,000 4.66 Theta2 Orionis A 1,100 ±
List_of_nearest_massive_stars
Pattern of stars recognized on Earth's night sky
Delta Orionis (Mintaka) which form the belt of Orion. Orion's Sword which hangs from Orion's Belt consists of the stars 42 Orionis, Theta Orionis, Iota
Asterism_(astronomy)
Variable star in the constellation Orion
a result of its rapid rotation, Omega Orionis is a Be class star. Among the stars of this class, Omega Orionis was the first where the magnetic field
Omega_Orionis
Star naming system
are some exceptions such as the chain of stars π1, π2, π3, π4, π5 and π6 Orionis. The most stars given the same Bayer designation but with an extra number
Bayer_designation
Hypothetical moon of Venus
stars which had been in the vicinity of Venus, including Chi Orionis, M Tauri, 71 Orionis, Nu Geminorum and Theta Librae.[citation needed] To date, among
Neith_(hypothetical_moon)
Binary star system in the constellation Orion
Pi4 Orionis (π4 Ori, π4 Orionis) is a binary star system in the western part of the Orion constellation. It is visible to the naked eye with an apparent
Pi4_Orionis
Binary star system in the constellation Orion
Phi1 Orionis is a binary star system in the constellation Orion, positioned less than a degree to the south of Meissa. It is visible to the naked eye
Phi1_Orionis
Star in the constellation Orion
Pi1 Orionis (π1 Ori, π1 Orionis) is a star in the equatorial constellation of Orion. It is faintly visible to the naked eye with an apparent visual magnitude
Pi1_Orionis
Star in the constellation Orion
Phi2 Orionis is a star in the constellation Orion, where it forms a small triangle on the celestial sphere with the nearby Meissa and Phi1 Orionis. This
Phi2_Orionis
Spectroscopic binary star system in the constellation Orion
Pi5 Orionis (π5 Ori, π5 Orionis) is a binary star system in the constellation Orion. It has an apparent visual magnitude of 3.69, which is bright enough
Pi5_Orionis
University Press. p. 170. ISBN 0-521-44921-9. Kaler, James B. "Saiph (Kappa Orionis)". Stars. University of Illinois. Archived from the original on 2012-02-02
List_of_proper_names_of_stars
Binary star system in the constellation Orion
Omicron1 Orionis (ο1 Ori) is a binary star in the northeastern corner of the constellation Orion. It is visible to the naked eye with an apparent visual
Omicron1_Orionis
Hot, luminous star with a spectral type of A9 or earlier
O4I(n)fp Alnilam (Epsilon Orionis) B-type supergiant, spectral type B0Ia, central star of Orion's Belt Saiph (Kappa Orionis) B-type supergiant, spectral
Blue_supergiant
Star in the constellation Orion
Pi6 Orionis (π6 Ori, π6 Orionis) is a solitary star in the eastern part of the constellation Orion. It is visible to the naked eye with an apparent visual
Pi6_Orionis
Star in the constellation Orion
Pi2 Orionis (π2 Ori, π2 Orionis) is the Bayer designation for a solitary star in the equatorial constellation of Orion. Although the Bright Star Catalogue
Pi2_Orionis
Star in the constellation Orion
Omicron2 Orionis (ο2 Ori) is a solitary star in the constellation Orion. It has an apparent visual magnitude of 4.06, which is bright enough to be seen
Omicron2_Orionis
Detail for NSV 4456". www.aavso.org. Retrieved 2022-09-01. "VSX : Detail for nu. Pup". www.aavso.org. Retrieved 2022-09-03. "VSX : Detail for NSV 14656".
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Spectroscopic binary system in the constellation of Orion
Psi2 Orionis a binary star system in the equatorial constellation of Orion. It has an apparent visual magnitude of 4.6, indicating that it is visible
Psi2_Orionis
Mrigashira – "the deer's head". Also known as āgrahāyaṇī λ "Meissa", φ Orionis Lord: Mangala (Mars) Symbol: Deer's head Deity: Soma, Chandra, the Moon
List_of_Nakshatras
String of Pearls النظم النَّظْم Epsilon Orionis Alnitak an-Niṭāq the Girdle (Orion's Belt) النطاق النِّطَاق Zeta Orionis Alphard al-Fard the Solitary one الفرد
List_of_Arabic_star_names
; Jayawardhana, R. (2002-11-01). "Direct detection of the companion of Orionis". Astronomy & Astrophysics. 394 (3): L43–L46. arXiv:astro-ph/0209404. doi:10
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Blue supergiant star in the constellation Cygnus
study of mass loss from the mid-ultraviolet spectrum of α Cygni (A2 Ia), β Orionis (B8 Ia), and η Leonis (A0 Ib)". The Astrophysical Journal. 223: 207. Bibcode:1978ApJ
Deneb
Brightest star in the constellation Lyra
(1981). "The near ultraviolet stellar spectra of alpha Lyrae and beta Orionis". Monthly Notices of the Royal Astronomical Society. 197: 57–74. Bibcode:1981MNRAS
Vega
Constellation split into two non-contiguous parts
297, been found to have a dusty disk surrounding it, and is also a UX Orionis star, meaning that it shows irregular variations in its brightness. The
Serpens
Small number of stars that orbit each other
37..207N. Lee Mohon (12 November 2015). "More Than Meets the Eye: Delta Orionis in Orion's Belt". Schütz, O.; Meeus, G.; Carmona, A.; Juhász, A.; Sterzik
Star_system
European visible and near-infrared space observatory, launched in 2023
These include free-floating planetary-mass objects discovered in the Sigma Orionis cluster, discovery of new gravitational lenses, and the discovery of a
Euclid_(space_telescope)
Constellation in the northern celestial hemisphere
eclipsing binaries - Into the G stars with HS Aurigae, FL Lyrae, and EW Orionis". The Astronomical Journal. 91: 383. Bibcode:1986AJ.....91..383P. doi:10
Lyra
Lunar mansion in Hindu astronomy
Tropical zodiac: 6° – 19°20′ Gemini 5 Mṛgaśiras "The Deer's Head" λ, φ Orionis Astrological leader: Mangala (Mars) Symbol: Deer's head Deity: Soma, the
Nakshatra
Clandestine term
Centauri), Toliman (Alpha Centauri), Kuma (Nu Draconis), Deneb (Alpha Cygni), Propus (Eta Geminorum), Heka (Lambda Orionis), Rana (Delta Eridani), Regor (Gamma
Code_name
Type of star
another 65 stars possible members. Six stars, namely Iota Herculis, 53 Piscium, Nu Eridani, Gamma Pegasi, HD 13745 (V354 Persei) and 53 Arietis had been found
Slowly_pulsating_B-type_star
Ophiuchus 16h 57m 40.09785s +09° 22′ 30.1126″ K2III 3.20# 35.66±0.20 13 Orionis 92 Orion 05h 07m 38.32s +09° 28′ 21.8″ G1IV Theta Pegasi (Biham/26 Pegasi)
List of star systems within 90–95 light-years
List_of_star_systems_within_90–95_light-years
204.1 63.8 ± 0.6 GV HIP 38594 63.8 ± 2.0 MV Gliese 3859 63.9 ± 0.7 GV 74 Orionis 64.0 ± 1.1 Orion 06h 16m 26.61911s +12° 16′ 19.7876″ FV Gliese 3383 64
List of star systems within 60–65 light-years
List_of_star_systems_within_60–65_light-years
5 177.1 HD 30562 Eridanus 85.27 ± 0.09 5.77 G2IV or G5V or F8V 178 Pi³ Orionis/Tabit Orion 26.32 ± 0.04 3.16 F6 V 179 Orion 40.48 ± 0.01 11.94 M2V or
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
NASA space telescope launched in 1999
(2001). "Chandra Discovers a Very High Density X-Ray Plasma on the O Star ζ Orionis". The Astrophysical Journal. 548 (1): L45–L48. arXiv:astro-ph/0012190.
Chandra_X-ray_Observatory
0.5 G 11.72 Has 1 confirmed exoplanet (Kepler-78b). Betelgeuse (Alpha Orionis) A 408 – 548+90 −49 Orion M1–M2 Ia–ab +0.50 The closest red supergiant
List of star systems within 400–450 light-years
List_of_star_systems_within_400–450_light-years
Apparent magnitude (V) Parallax (mas) Notes and additional references Rho Orionis 350 Orion K0 III +4.44 HD 2 350.55 F5 8.2 Zeta¹ Antliae A 350 ± 2 Antlia
List of star systems within 350–400 light-years
List_of_star_systems_within_350–400_light-years
closest core-collapse supernova candidates to Earth. B B2V Bellatrix (Gamma Orionis) 250 ± 10 Orion B2 III 1.64 One of the closest core-collapse supernova
List of star systems within 250–300 light-years
List_of_star_systems_within_250–300_light-years
Constellation in the southern celestial hemisphere
a mere 300,000 years old composed of two pre-main-sequence stars—a FU Orionis star and a Herbig Ae/Be star, which has brightened episodically by two
Canis_Major
B8 V 2.61 Xi Aquilae (Libertas) 186 ± 1 Aquila G9.5 IIIb 4.722 Omicron² Orionis 186 ± Orion K2 IIIb 4.06 Gamma Pictoris 186 ± 2 Pictor 05h 49m 49.66006s
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
author of Celestial Objects for Common Telescopes and discoverer of S Orionis MPC · 3041 3042 Zelinsky 1981 EF10 David S. Zelinsky, American mathematician
Meanings of minor-planet names: 3001–4000
Meanings_of_minor-planet_names:_3001–4000
Unique identifier given to variable stars
the constellation name (e.g. Centaurus becomes Centauri, Orion becomes Orionis) to get the star name. In the early 19th century few variable stars were
Variable-star_designation
(2000-10-06). "Discovery of Young, Isolated Planetary Mass Objects in the σ Orionis Star Cluster". Science. 290 (5489): 103–107. Bibcode:2000Sci...290..103Z
List_of_exoplanet_firsts
List of largest planets by size
2011). "Spectroscopy of very low mass stars and brown dwarfs in the Lambda Orionis star forming region. I. Enlarging the census down to the planetary mass
List_of_largest_exoplanets
Array used for astronomical observations
Abraham; Pease, Francis G. (1921). "Measurement of the diameter of alpha Orionis with the interferometer". Astrophysical Journal. 53 (5): 249–59. Bibcode:1921ApJ
Astronomical_interferometer
light FUOR – (celestial object) FU Orionis objects, a class of variable pre–main sequence stars named after FU Orionis, the archetype for the class also
List_of_astronomy_acronyms
Constellation in the southern celestial hemisphere
study of mass loss from the mid-ultraviolet spectrum of α Cygni (A2 Ia), β Orionis (B8 Ia), and η Leonis (A0 Ib)". The Astrophysical Journal. 223: 207. Bibcode:1978ApJ
Pictor
predicted highly evaporating planet was proposed to orbit the star FU Orionis with a density of about 0.0042 g/cm3. Highest planetary rotation rate Kappa
List_of_exoplanet_extremes
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