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Open star cluster in the constellation Orion
The Lambda Orionis Cluster (also known as the Collinder 69) is an open star cluster located north-west of the star Betelgeuse in the constellation of
Lambda_Orionis_Cluster
Star in the constellation Orion
Meissa /ˈmaɪsə/, designated Lambda Orionis (λ Orionis, abbreviated Lambda Ori, λ Ori) is a star system in the constellation of Orion. It is a binary star
Meissa
Star-forming region in the constellation Orion
association Orion's Belt Sigma Ori cluster 25 Ori cluster Lambda Orionis molecular ring (Sh2-264) Lambda Ori cluster Barnard 30 Barnard 35 (Angelfish nebula)
Orion_molecular_cloud_complex
Binary star system in the constellation Orion
068 days and an eccentricity of 0.22. It is a member of the young Lambda Orionis cluster and is roughly 7 million years old. The primary component is a B-type
Phi1_Orionis
Constellation straddling the celestial equator
Orionis, Iota Orionis, and 42 Orionis. Three stars comprise a small triangle that marks the head. The apex is marked by Meissa (Lambda Orionis), a hot blue
Orion_(constellation)
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
Dark nebula in the constellation Orion
the regions in the Lambda Orionis Ring where the population of young stars is concentrated, together with the Lambda Orionis cluster and Barnard 35. It
Barnard_30
This is a list of open clusters located in the Milky Way. An open cluster is an association of up to a few thousand stars that all formed from the same
List_of_open_clusters
Interstellar cloud in Orion
Sharpless 264, also known as the Lambda Orionis Ring, is a molecular cloud and H II region, which can be seen in the northern region of the Orion molecular
Sh_2-264
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)
Topics referred to by the same term
Structures in the constellation Orion: Lambda Orionis, binary star Collinder 69, star cluster including Lambda Orionis This disambiguation page lists articles
Orion's_head
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
Catalogue of open clusters made by Swedish astronomer Per Collinder
properties of open galactic clusters and their spatial distribution. The catalogue contains 452 open clusters, 11 globular clusters, 6 asterisms, 1 stellar
Collinder_catalogue
; Zavala, R. T. (2013). "Dynamical mass of the O-type supergiant in ζ Orionis A". Astronomy & Astrophysics. 554: A52. arXiv:1306.0330. Bibcode:2013A&A
List_of_most_massive_stars
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
Stars sorted by absolute magnitude
ISSN 0004-6361. S2CID 15874925. Murdin, P.; Penston, M. V. (1977-12-01). "The Lambda Orionis association". Monthly Notices of the Royal Astronomical Society. 181
List_of_most_luminous_stars
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)
O-type_star
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
69 (1.64–1.74var) Alnilam ε Orionis 1,180 B0 Ia Southern 30 1.74 Alnair α Gruis 0100 B6 V Southern 31 1.77 Alnitak ζ Orionis 01,300 O9.5 Iab, B1 IV, B0
List_of_brightest_stars
Large self-illuminated object in space
Michelson, A. A.; Pease, F. G. (1921). "Measurement of the diameter of Alpha Orionis with the interferometer". Astrophysical Journal. 53 (5): 249–259. Bibcode:1921ApJ
Star
Continuous band of stars that appears on plots of stellar color versus brightness
them "giant" and "dwarf" stars. The following year he began studying star clusters; large groupings of stars that are co-located at approximately the same
Main_sequence
Binary star system in the constellation Orion
Xi Orionis (ξ Orionis) is a binary star system in the northeastern part of the constellation of Orion, well above the red giant star Betelgeuse in the
Xi_Orionis
Main-sequence star of spectral type O
5 main sequence star. It is a runaway star. θ1 Orionis C is the brightest star in the Trapezium Cluster in the Orion Nebula, an O6 main sequence star with
O-type_main-sequence_star
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
Flow of gas ejected from the upper atmosphere of a star
This image shows the wind from the star LL Orionis generating a bow shock (the bright arc) as it collides with material in the surrounding Orion Nebula
Stellar_wind
Gas and dust surrounding a newly formed star
like HL Tauri (artist concept). Image of the circumtrinary disc around GW Orionis. An artist's concept of a protoplanetary disk Components of proplyd 177-341W
Protoplanetary_disk
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
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
Early stage in the process of star formation
definitive evidence for this identification. Video about the protostar V1647 Orionis and its X-ray emission (2004). Protostar outburst - HOPS 383 (2015). Protostar
Protostar
List from the Alphabet Direction (αβ)
star cluster Caballero-Solano 1 at Delta Orionis, also known as the Mintaka cluster) Calvet — (telescopic asterisms) Camargo — (open star clusters) Canali
List of astronomical catalogues
List_of_astronomical_catalogues
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
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
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
Type of star larger than main-sequence but smaller than a giant
Cassiopeiae, δ Scorpii, B0.5: β Scorpii, ε Persei B1: ο Persei, β Cephei B2: γ Orionis, π Scorpii, θ Ophiuchi, λ Scorpii, ω Canis Majoris B2.5: γ Pegasi, ζ Cassiopeiae
Subgiant
Small number of stars that orbit each other
A large group of stars bound by gravitation is generally called a star cluster or galaxy, although, broadly speaking, they are also star systems. Star
Star_system
Caballero, J. A. (2014-10-01). "Stellar multiplicity in the sigma Orionis cluster: a review". The Observatory. 134: 273–287. arXiv:1408.2231. Bibcode:2014Obs
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Overview of the scientific field of astronomy
Hayashi track Hayashi limit Henyey track Orion variable T Tauri star FU Orionis star Herbig Ae/Be Luminosity class Subdwarf star Dwarf star Blue dwarf
Outline_of_astronomy
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
Constellation in the northern celestial hemisphere
APIN, this name was also applied to the pairs of Pi3 and Pi4 Orionis and Zeta and Xi Orionis. The meaning of MASH.TAB.BA evolved as well, becoming the twin
Canis_Minor
Grouping of evolved cool luminous stars
typically found in oxygen-rich M-type AGB stars such as R Cassiopeiae and U Orionis, while HCN and SiS masers are generally found in carbon stars such as IRC
Asymptotic_giant_branch
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
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
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
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
Star that has a supergiant luminosity class, with a spectral type of F or G
(1997). "Abundance Analyses of the Field RV Tauri Variables: EP Lyrae, DY Orionis, AR Puppis, and R Sagittae". The Astrophysical Journal. 479 (1): 427–440
Yellow_supergiant
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
Stellar classification
define the system, are considered to be 78 Ursae Majoris (F2 V) and Pi3 Orionis (F6 V). In addition to those two standards, Morgan & Keenan (1973) considered
F-type_main-sequence_star
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
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
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
Stellar classification distinguished by bright blue luminosity
stars that have remain unchanged since at least the 1940s, are Upsilon Orionis (B0 V), Eta Aurigae (B3 V), and Alkaid (B3 V). Besides these anchor standards
B-type_main-sequence_star
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
Astronomical object without the mass to sustain hydrogen fusion
September 17, 2007. A search for substellar members in the Praesepe and σ Orionis clusters, B. M. González-García, M. R. Zapatero Osorio, V. J. S. Béjar, G. Bihain
Substellar_object
Matter and radiation in the space between the star systems in a galaxy
in 1904, when Johannes Hartmann observed the binary star Mintaka (Delta Orionis) with the Potsdam Great Refractor. Hartmann reported that absorption from
Interstellar_medium
1541″ A0pSiEuHg 2.84 to 2.98 COCONUTS-3 (WISE J0813-1522) A 100.7 M5 B L6 Lambda Geminorum 100.9 ± 0.6 Gemini 07h 18m 05.58012s +16° 32′ 25.3964″ A3V +3
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
Star in the constellation of Draco
Enclosure, refers to an asterism consisting of Alpha Draconis, Kappa Draconis, Lambda Draconis, 24 Ursae Majoris, 43 Camelopardalis, Alpha Camelopardalis and
Thuban
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
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
Visible star that is nearly aligned with Earth's axis of rotation
Cepheus, about six degrees from Polaris Delta Octantis Uranus Eta Ophiuchi 15 Orionis Neptune midway between Gamma Cygni and Delta Cygni Gamma Velorum
Pole_star
Star whose brightness fluctuates, as seen from Earth
particularly extreme example is UX Orionis, which is the prototype of "UXORs"; these protostars vary by 2 to 3 magnitudes. FU Orionis variables A small fraction
Variable_star
Star system in the Centaurus constellation
ˈkɛnt/) or even Rigil, though the latter name is better known for Rigel (β Orionis). An alternative name found in European sources, Toliman, is an approximation
Alpha_Centauri
"Spatially Resolved Hubble Space Telescope Spectra of the Chromosphere of alpha Orionis". Astronomical Journal. 116 (5): 2501. Bibcode:1998AJ....116.2501U. doi:10
List of stars with resolved images
List_of_stars_with_resolved_images
stellar cluster or association membership, because it is difficult to calculate accurate distances for red supergiants that are not part of any cluster or
List_of_largest_stars
Small patches of nebulosity associated with newly born stars
light-years (0.26 parsec) and is located in the vicinity of the sigma Orionis cluster. Previously only small mini-jets (≤0.03 parsec) were found around proto-brown
Herbig–Haro_object
Substellar object
confirmed class "M" brown dwarf. This object, found in the Pleiades open cluster, received the name Teide 1. Teide 1 was discovered in images collected
Brown_dwarf
Molecular cloud complex in the constellation Monoceros
and Orion B complexes and the Orion Nebula, which also includes the Lambda Orionis ring and some of the peripheral regions of the complex, such as gas
Monoceros_R2
Classification of stars based on spectral properties
mechanics. Example spectral standards: B0V – Upsilon Orionis B0Ia – Alnilam B2Ia – Chi2 Orionis B2Ib – 9 Cephei B3V – Alkaid B3V – Haedus B3Ia – Omicron2
Stellar_classification
Type of star, larger and brighter than the Sun
become peculiar[clarification needed] blue giants. Examples: Meissa (λ Orionis A), an O-type giant. Alcyone (η Tauri), a B-type giant, the brightest star
Giant_star
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
Exoplanets confirmed or discovered from direct imaging
Bouy H (1 June 2007). "The young, wide and very low mass visual binary Lambda Orionis 167". Astronomy and Astrophysics. 468 (1): L5–L8. arXiv:0704.2469. Bibcode:2007A&A
List of directly imaged exoplanets
List_of_directly_imaged_exoplanets
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
A K0V 5.82 6.27 01h 39m 47.54s −56° 11′ 47.0″ 25.5 B K5V 5.95 6.40 π3 Orionis F6V 3.19 3.67 04h 49m 50.41s +06° 57′ 40.6″ 26.3 χ Draconis A F7V 3.68
List_of_nearest_bright_stars
(4): 71. doi:10.3847/2515-5172/adc739. Kaler, James B. "BELLATRIX (Gamma Orionis)". Stars. University of Illinois. Retrieved 2012-12-27. van Leeuwen, F
List_of_supernova_candidates
Observatory in Urbana, Illinois, U.S.
Astrophysical Journal on eclipsing binaries Lambda Tauri, Algol, 1H Cassiopeiae (HR 8926), ellipsoidal variables π5 Orionis, and b Persei, and Nova Aquilae (V603
Astronomical Observatory (University of Illinois Urbana-Champaign)
Astronomical_Observatory_(University_of_Illinois_Urbana-Champaign)
Type of cool giant star
(1988). "A white dwarf companion to the main-sequence star 4 Omicron(1) Orionis and the binary hypothesis for the origin of peculiar red giants". Astrophysical
S-type_star
Intermediate-mass Stars. XXXVII. Uncovering a 0.53M⊙, 0.75 au Companion to h Orionis". Research Notes of the American Astronomical Society. 10 (5): 125. Bibcode:2026RNAAS
List_of_smallest_known_stars
Resolution ALMA Observations of Richly Structured Protoplanetary Disks in σ Orionis". The Astrophysical Journal. 976 (1): 132. arXiv:2410.03823. Bibcode:2024ApJ
List of resolved circumstellar disks
List_of_resolved_circumstellar_disks
LAMBDA ORIONIS-CLUSTER
LAMBDA ORIONIS-CLUSTER
Female
Native American
Native American Indian name ALAMEDA means "grove of cottonwood."
Boy/Male
Greek American
Rising in the sky; dawning. Mythological Orion was a mighty hunter and son of Poseidon. The...
Surname or Lastname
English
English : from a pet form of Lamb 1 and 2.English : from an Old Norse personal name Lambi, from lamb ‘lamb’.
Girl/Female
Arabic, Indian, Muslim, Pashtun, Sanskrit
Flame; Large; Spacious; Tall; Another Name for Durga and Lakshmi
Male
Greek
(ΩÏίων) Greek name, probably ORION means "mountain man." But some sources say that the name may actually be of Akkadian origin; if so, it means "light of heaven." In mythology, this is the name of one of the Titan gods, a primordial hunter who was killed by a scorpion. A constellation was named after him. Orion had two dogs; their names were: Arktophonos and Ptoophagos.Â
Surname or Lastname
English
English : from Middle English lamb, a nickname for a meek and inoffensive person, or a metonymic occupational name for a keeper of lambs. See also Lamm.English : from a short form of the personal name Lambert.Irish : reduced Anglicized form of Gaelic Ó Luain (see Lane 3). MacLysaght comments: ‘The form Lamb(e), which results from a more than usually absurd pseudo-translation (uan ‘lamb’), is now much more numerous than O’Loan itself.’Possibly also a translation of French agneau.
Girl/Female
British, English, Greek, Spanish
From Dionysus God of Wine; Follower of Dionysius
Female
Greek
(Λαμία) Greek myth name of an evil spirit who abducts and devours children, LAMIA means "large shark." The name means "vampire" in Latin and "fiend" in Arabic.
Girl/Female
Spanish
From Dionysus god of wine.
Female
Italian
Italian form of English Amber, AMBRA means "amber."
Girl/Female
Muslim
Flame
Girl/Female
Indian
Flame
Girl/Female
American, Australian, British, English, Greek
A Flowering Vine; The Name of a Flowering Vine Used in Folk Medicine
Girl/Female
Greek
Mother of Aesculapius.
Boy/Male
Hindu
Lord Ganesh, The huge bellied Lord
Boy/Male
British, English, French, Greek, Latin
Greek God of Wine
Surname or Lastname
English
English : habitational name from Lambden in Berwickshire.
Female
Spanish
Feminine form of Spanish Amado, AMADA means "beloved."
Girl/Female
English Greek
The name of a flowering vine used in folk medicine.
Girl/Female
Indian
Ambitious
LAMBDA ORIONIS-CLUSTER
LAMBDA ORIONIS-CLUSTER
Girl/Female
Gujarati, Hindu, Indian, Kannada, Marathi, Sanskrit, Sindhi, Telugu
Visible; Cute; Brilliant
Surname or Lastname
English (mainly southeastern)
English (mainly southeastern) : topographic name for someone who lived near a conspicuous tree, Middle English tre(w).
Boy/Male
Spanish
Savior.
Boy/Male
Arabic, Australian, Muslim, Turkish
Strong; Certain; Well-established; Sure
Male
English
Variant spelling of English Blaize, BLAZE means "talks with a lisp."
Girl/Female
American, Anglo, Australian, British, English
Delight; Joy; Happy; Intense Happiness
Boy/Male
Muslim
Vision, Propitious, Auspicious, Prudent, Bringer of glad tidings
Boy/Male
Tamil
Astitva | அஸà¯à®¤à®¿à®¤à¯à®µ
Existence
Boy/Male
Indian
The most exalted
Boy/Male
American, British, English, Scottish
White Falcon; Battle Hawk
LAMBDA ORIONIS-CLUSTER
LAMBDA ORIONIS-CLUSTER
LAMBDA ORIONIS-CLUSTER
LAMBDA ORIONIS-CLUSTER
LAMBDA ORIONIS-CLUSTER
n.
In Greek grammar, a sign ['] sometimes placed over a contracted syllable.
v. i.
To bring forth a lamb or lambs, as sheep.
a.
Feeding upon onions.
n.
The point of junction of the sagittal and lambdoid sutures of the skull.
n.
Any person who is as innocent or gentle as a lamb.
n.
A lamp or candlestick.
n.
The blade of a leaf; the broad, expanded portion of a petal or sepal of a flower.
a.
Having two heads or origins, as a muscle.
a.
Having three heads, or three origins; as, a tricipital muscle.
imp. & p. p.
of Lamb
n.
The curved line or flourish at the end of a book or chapter; hence, the end.
n.
A thin plate or lamina.
a.
Of or pertaining to the genus Allium, or garlic, onions, leeks, etc.; having the smell or taste of garlic or onions.
n.
A thin plate or scale; specif., one of the thin, flat processes composing the vane of a feather.
n.
The name of the Greek letter /, /, corresponding with the English letter L, l.
pl.
of Lamina
pl.
of Lamina
n.
A viola da gamba.
n.
A thin plate or scale; a layer or coat lying over another; -- said of thin plates or platelike substances, as of bone or minerals.
n.
The lamb's-quarters (Chenopodium album).