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Satellite galaxy of the Milky Way
The Large Magellanic Cloud (LMC) is a dwarf galaxy and satellite galaxy of the Milky Way. At a distance of around 50 kiloparsecs (163,000 light-years)
Large_Magellanic_Cloud
Two dwarf galaxies orbiting the Milky Way
as Magellanic spiral galaxies. The two galaxies are the following: Large Magellanic Cloud (LMC), about 163 kly (50 kpc) away Small Magellanic Cloud (SMC)
Magellanic_Clouds
Dwarf irregular galaxy, satellite galaxy of the Milky Way
The Small Magellanic Cloud (SMC) is a dwarf galaxy near the Milky Way. Classified as a dwarf irregular galaxy, the SMC has a D25 isophotal diameter of
Small_Magellanic_Cloud
Spiral galaxies with one spiral arm
SBm, SABm); the prototype galaxy and namesake for Magellanic spirals is the Large Magellanic Cloud, an SBm galaxy. They are usually smaller dwarf galaxies
Magellanic_spiral
SAGE-Spec Spitzer Legacy program: the life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification – III". Monthly Notices of the Royal
List_of_largest_stars
HVCld in Sculptor by MClds
The Magellanic Stream is a stream of high-velocity clouds of gas extending behind the Large and Small Magellanic Clouds over 100° through the Galactic
Magellanic_Stream
Heterogeneous class of stars with unusual spectra
somewhat lower in M31, lower still in the Large Magellanic Cloud, and much lower in the Small Magellanic Cloud. Strong metallicity variations are seen across
Wolf–Rayet_star
H II region in the constellation Dorado
The Tarantula Nebula (also known as 30 Doradus) is a large H II region in the Large Magellanic Cloud (LMC), forming its south-east corner (from Earth's
Tarantula_Nebula
of the Large Magellanic Cloud. This is a list of luminous blue variable stars in order of their distance from Earth. The Large Magellanic Cloud (LMC) is
List of luminous blue variable stars
List_of_luminous_blue_variable_stars
Stream of neutral hydrogen gas linking the two Magellanic clouds
stream of stars throughout the Magellanic Bridge linking the Large Magellanic Cloud (LMC) with the Small Magellanic Cloud (SMC). This stellar bridge is
Magellanic_Bridge
Group of galaxies that includes the Milky Way
satellite system comprises the Sagittarius Dwarf Galaxy, Large Magellanic Cloud, Small Magellanic Cloud, Canis Major Dwarf Galaxy (disputed, considered by some
Local_Group
Binary star in the constellation Dorado
WOH G64 (IRAS 04553–6825) is a symbiotic binary in the Large Magellanic Cloud, roughly 50 kiloparsecs (163,000 light-years) from Earth. The primary component
WOH_G64
Supernova remnant
LHG 26 or MC SNR J0519−6902) is a supernova remnant (SNR) in the Large Magellanic Cloud. The supernova occurred around 163,000 light-years away in the constellation
SNR_0519−69.0
Constellation in the southern sky
also been depicted as a swordfish. Dorado contains most of the Large Magellanic Cloud, the remainder being in the constellation Mensa. The South Ecliptic
Dorado
Wolf–Rayet star in the constellation Dorado
bright stars in the Large Magellanic Cloud (LMC). Among the objects cataloged was RMC 136 (Radcliffe observatory Magellanic Cloud catalog number 136)
R136a1
Star cluster in the constellation Dorado
NGC 1910, or LH-41, is an OB association in the Large Magellanic Cloud. NGC 1910's right ascension is 5h 18m 42.5s and its declination is -69° 14′ 12.1″
NGC_1910
Topics referred to by the same term
navigation Magellanic Clouds, two major Milky Way neighbouring galaxies, matter streams, or systems related to them: Large Magellanic Cloud, a major satellite
Magellanic
Hypervelocity star in the constellation Dorado
direction of the Dorado constellation, 16 degrees northwest of the Large Magellanic Cloud (LMC) and farther away than the LMC. The star appears to be receding
HE_0437−5439
Red supergiant star in the constellation Dorado
referred to as [W60] B90) is a large and highly luminous red supergiant star similar to Betelgeuse in the Large Magellanic Cloud. It is one of the largest
B90_(star)
List from the Alphabet Direction (αβ)
or Magellanic Catalogue of Stars MACHO — MACHO Project lensing events (Massive Compact Halo Object) MACHO-LMC — MACHO Project Large Magellanic Cloud Microlensing
List of astronomical catalogues
List_of_astronomical_catalogues
Large, low-density interstellar cloud of partially ionized gas
thousands of stars. Examples include the 30 Doradus region in the Large Magellanic Cloud and NGC 604 in the Triangulum Galaxy. The term H II is pronounced
H_II_region
Small galaxy composed of up to several billion stars
stars, as compared to the Milky Way's 100–400 billion stars. The Large Magellanic Cloud, which closely orbits the Milky Way and contains over 30 billion
Dwarf_galaxy
H II region in the Large Magellanic Cloud
(N70) is a faint emission nebula and superbubble located in the Large Magellanic Cloud in the constellation of Dorado. Henize 70 was first observed in
Henize_70
Irregular version of a barred spiral galaxy
shape. Examples include the Large Magellanic Cloud (LMC) and NGC 6822, although LMC is more often classified as a magellanic spiral galaxy. Some barred
Barred_irregular_galaxy
Super star cluster in the constellation Dorado, in the Large Magellanic Cloud
cluster, which lies at the centre of the Tarantula Nebula in the Large Magellanic Cloud. When originally named it was an unresolved stellar object (catalogued
R136
Extraterrestrial view of outer space
would be easily visible to the naked eye. From a viewpoint in the Large Magellanic Cloud, the Milky Way's total apparent magnitude would be −2.0—over 14
Extraterrestrial_sky
Star in the Large Magellanic Cloud
Doradus (also known as S Dor) is one of the brightest stars in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way, located roughly 160
S_Doradus
Binary star in the Large Magellanic cloud
30 Doradus complex (also known as the Tarantula Nebula) in the Large Magellanic Cloud. Both components are amongst the most massive and most luminous
Melnick_34
2008. "Magellanic Cloud". Astronomy Knowledge Base. University of Ottawa. Archived from the original on 5 July 2006. "The Large Magellanic Cloud, LMC"
List_of_galaxies
Star in the constellation Dorado
BAT99-98 is a Wolf–Rayet star located in the Large Magellanic Cloud, in NGC 2070 near the R136 cluster in the Tarantula Nebula (30 Doradus). At estimates
BAT99-98
Cavity hundreds of light years across created by strong stellar winds in a galaxy
Perseus-Taurus Shell The Local Bubble Very Large Telescope image of superbubble LHA 120-N 44 in the Large Magellanic Cloud. Credit: ESO/Manu Mejias. The Per-Tau
Superbubble
Open star cluster within the Large Magellanic cloud
cluster located in the Dorado constellation which is part of the Large Magellanic Cloud. It was discovered by John Herschel on November 30, 1834. Its apparent
NGC_1997
Subclass of pulsating star
standard candles. They have been used to establish the distance to the Large Magellanic Cloud, globular clusters, open clusters, and the Galactic Center. The
Delta_Scuti_variable
1994 novel by Jack McDevitt
– were observing the Large Magellanic Cloud because they evacuated to that location. The implications were that the Omega clouds menace the entire galaxy
The_Engines_of_God
Globular cluster in the Large Magellanic Cloud
located within the Large Magellanic Cloud in the constellation Dorado. Compared to other globular clusters of the Large Magellanic Cloud, NGC 2005 has a
NGC_2005
Type of star that is luminous, blue, and variable in brightness
Doradus variables after S Doradus, one of the brightest stars of the Large Magellanic Cloud. The LBV stars P Cygni and η Carinae have been known as unusual
Luminous_blue_variable
Class of galaxy
irregular galaxies. The Large Magellanic Cloud has since been re-classified as type SBm (barred Magellanic spiral). The Small Magellanic Cloud remains classified
Irregular_galaxy
Hypergiant star in the constellation Dorado
HD 32034 (or R 62) is one of seven blue hypergiants in the Large Magellanic Cloud and is suspected to be a shell star. It lies within the loose association
HD_32034
Globular star cluster
NGC 2210 is a globular cluster located in the Large Magellanic Cloud, in the constellation Dorado. It is situated south of the celestial equator and, as
NGC_2210
Wolf–Rayet star in the constellation Dorado
LMC195-1 is a Wolf–Rayet star located in the Large Magellanic Cloud (LMC). It is an extremely rare member of the WO oxygen sequence, at WO2 the hottest
LMC195-1
Interstellar absorption and scattering of light
extinction curves are those of the Milky Way, the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). In the LMC, there is significant variation
Extinction_(astronomy)
cluster in Large Magellanic Cloud. BSDL 2527 is a star cluster in Large Magellanic Cloud. DEM S10 is a H II region in Small Magellanic Cloud. DEM S80 is
List_of_most_massive_stars
Nebula in the Large Magellanic Cloud
LMC N79 (or LHα 120-N79) is an emission nebula in the Large Magellanic Cloud. The nebula is part of the catalog of H-alpha stars and nebulae by Karl G
LMC_N79
Satellite galaxy of the Milky Way
the core of the Milky Way (about one third of the distance of the Large Magellanic Cloud). In its looping, spiraling path, it has passed through the plane
Sagittarius Dwarf Spheroidal Galaxy
Sagittarius_Dwarf_Spheroidal_Galaxy
H II region in the constellation Dorado
LH 95 is a modestly sized stellar nursery in the Large Magellanic Cloud. It is related to the HII-region LHA 120-N 55, that is, a region of hydrogen ionized
LH_95
X-ray Binary in the Large Magellanic Cloud
LMC X-2 is a low-mass X-ray binary (LMXB) located in the Large Magellanic Cloud (LMC), a satellite galaxy of Milky Way. It is one of the five brightest
LMC_X-2
Supernova remnant in the constellation Mensa
(also known as SNR 0509–68.7) is a supernova remnant located in the Large Magellanic Cloud. It is relatively close to Earth, allowing astronomers to observe
N103B
X-ray binary in the Large Magellanic Cloud
eclipsing high-mass X-ray binary (HMXB) pulsar system located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way approximately 163,000
LMC_X-4
Galaxy morphological types and objects that are members of the Large Magellanic Cloud are identified using the NASA/IPAC Extragalactic Database. The other
List of NGC objects (1001–2000)
List_of_NGC_objects_(1001–2000)
Spiral galaxy in the constellation Triangulum
second-smallest spiral galaxy in the Local Group after the Large Magellanic Cloud, which is a Magellanic-type spiral galaxy. It is believed to be a satellite
Triangulum_Galaxy
Star in the constellation Dorado
hypergiant in the Large Magellanic Cloud. It is surrounded by an unexpected dust disk. R126, formally RMC (Radcliffe observatory Magellanic Cloud) 126, is a
HD_37974
Physics apparatus designed to study neutrinos
2018[update] are the Sun and the supernova 1987A in the nearby Large Magellanic Cloud. Another likely source (three standard deviations) is the blazar
Neutrino_detector
1987 supernova event in the constellation Dorado
SN 1987A was a Type II supernova in the Large Magellanic Cloud, a dwarf satellite galaxy of the Milky Way. It occurred approximately 51.4 kiloparsecs (168
SN_1987A
Star in Large Magellanic Cloud
HD 37836 is a candidate luminous blue variable located in the Large Magellanic Cloud and one of the brightest stars in its galaxy. The star was first mentioned
HD_37836
Emission nebula in the constellation Dorado
is an emission nebula with superbubble structure located in the Large Magellanic Cloud, a satellite galaxy of the Milky Way in the constellation Dorado
N44_(emission_nebula)
Red emission nebula in the constellation Dorado
red emission nebula surrounding an open cluster of stars in the Large Magellanic Cloud, at a distance of about 163,000 light-years. The nebula was discovered
NGC_2014
American astronomer (1889–1953)
Gravitational Lensing Experiment. Cepheids in the Magellanic Clouds. IV. Catalog of Cepheids from the Large Magellanic Cloud". Acta Astronomica. 49: 223–317. arXiv:astro-ph/9908317
Edwin_Hubble
Yellow hypergiant in the Large Magellanic Cloud
an Alpha Cygni variable. It is one of the brightest stars in the Large Magellanic Cloud (LMC), positioned in the deep southern constellation of Dorado.
HD_271182
Open star cluster in the constellation Mensa
2000 is an open cluster located in the constellation Mensa, in the Large Magellanic Cloud. It is around 160-165 thousand light-years away. It was discovered
NGC_2000
Spiral shaped H II region in the constellation Dorado
LHA 120-N 119) is a spiral-shaped H II region in the Large Magellanic Cloud. Its dimensions are large, at 131 x 175 pc (430 × 570 ly). It contains several
N119
Pulsar in the constellation Dorado
J0540−6919 (PSR B0540−69) is a pulsar in the Tarantula Nebula of the Large Magellanic Cloud. It is the first extragalactic gamma-ray pulsar discovered. A rotation
PSR_J0540−6919
Star in the constellation Dorado
spectroscopic binary star system in the LH 54 OB association within the Large Magellanic Cloud in the constellation Dorado. The OB association LH 54 was catalogued
LH_54-425
Open cluster in the constellation Dorado
2710, LH 9) is an open cluster in the Dorado constellation in the Large Magellanic Cloud. It encompasses a group of about 50 massive hot young stars. These
NGC_1761
System of stars and interstellar matter
to the unaided eye, including the Andromeda Galaxy, Large Magellanic Cloud, Small Magellanic Cloud, and the Triangulum Galaxy. In the 10th century, Persian
Galaxy
Fictional alien race in Marvel Comics
are plant-like aliens who originate from the planet Hala in the Large Magellanic Cloud, the same planet as the Kree. They were once more humanoid in appearance
Cotati_(comics)
Alexander P.; et al. (2026). "A nearly pristine star from the Large Magellanic Cloud". Nature Astronomy. 10 (6): 842–857. arXiv:2509.21643. Bibcode:2026NatAs
List_of_oldest_stars
Open cluster in the constellation Dorado
cluster located in the Dorado constellation and is part of the Large Magellanic Cloud. NGC 2001 was discovered by James Dunlop on September 27, 1826.
NGC_2001
Type of variable star that pulsates radially
Swan Leavitt when she studied thousands of variable stars in the Magellanic Clouds. The discovery establishes the true luminosity of a Cepheid by observing
Cepheid_variable
Galaxy that orbits a larger galaxy due to gravitational attraction
is the Large Magellanic Cloud. Moreover, satellite galaxies are not the only astronomical objects that are gravitationally bound to larger host galaxies
Satellite_galaxy
Open cluster in the constellation Dorado
cluster located in the Dorado constellation and is part of the Large Magellanic Cloud. It is not visible to the naked eye and requires a telescope to
NGC_2003
Constellation in the southern celestial hemisphere
Alpha Mensae, is barely visible in suburban skies. Part of the Large Magellanic Cloud, several star clusters and a quasar lie in the area covered by the
Mensa_(constellation)
Large self-illuminated object in space
pressure on the accreting gas cloud. Several stars in the R136 cluster in the Large Magellanic Cloud have been measured with larger masses, but it has been
Star
1998 American film
(Peter Boyle) claims that they originated in the Large Magellanic Cloud (also called the Magellanic Galaxy), due to it apparently being the only other
Species_II
Emission nebula in the constellation Dorado
emission nebula located in the Dorado constellation and part of the Large Magellanic Cloud. It was discovered by John Herschel on November 23, 1834. Its apparent
NGC_1934
Emission nebula in the constellation Dorado
as N 180B (LHA 120-N 180B), is an emission nebula located in the Large Magellanic Cloud. "Hubble heritage project". Results for N 180B. Archived from the
NGC_2122
Emission nebula in the constellation Dorado
is the brightest emission nebula in the north-west part of the Large Magellanic Cloud in the Dorado constellation. The N11 complex is the second largest
N11_(emission_nebula)
Red giant in the constellation Volans
highly eccentric orbit are spatially and dynamically linked to the Large Magellanic Cloud (LMC). The star formed in the LMC's halo during an early epoch of
SDSS_J0715-7334
Candidate luminous variable star in the constellation Dorado
Observatory Magellanic Clouds catalog) is a candidate luminous blue variable located in the LH-41 OB association in the Large Magellanic Cloud. R85 has been
R85
Experiment deployed on the lunar surface
atmosphere and aurora, various nebulae and star clusters, and the Large Magellanic Cloud. The film was digitally scanned and saved on tape. Files from these
Far Ultraviolet Camera/Spectrograph
Far_Ultraviolet_Camera/Spectrograph
1973 science fiction novel by Arthur C. Clarke
to propel itself out of the Solar System in the direction of the Large Magellanic Cloud. After Rama leaves, a member of the Rama Committee considers that
Rendezvous_with_Rama
Star in the constellation Dorado
concentration of stars of the large NGC 2070 open cluster in the Tarantula Nebula, a massive H II region in the Large Magellanic Cloud which is a nearby satellite
R136a2
Astrophysical phenomenon
observed was Kepler's Supernova in 1604. SN 1987A occurred in the Large Magellanic Cloud, a satellite galaxy of our galaxy, in 1987. Several thousand supernovae
Supernova
Supernova remnant in the constellation Dorado
J052559-660453), also known as Brasil Nebula, is a supernova remnant in the Large Magellanic Cloud. On March 5, 1979, Venera 11, Venera 12, and seven other spacecraft
LMC_N49
Star in the Large Magellanic Cloud
R71 (RMC 71, HD 269006) is a star in the Large Magellanic Cloud (LMC) in the constellation Mensa. It is classified as a luminous blue variable and is one
R71_(star)
Small Magellanic Cloud star in the constellation Tucana
HV 2112 is a cool luminous variable star in the Small Magellanic Cloud. Until 2018, it was considered to be the most likely candidate for a Thorne–Żytkow
HV_2112
Supernova Remnant in the Large Magellanic Cloud
J052501-693842) is a prominent supernova remnant (SNR) located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way Galaxy, in the constellation
LMC_N132D
Open star cluster in the constellation Dorado
open cluster in the Dorado constellation which is located in the Large Magellanic Cloud. It was discovered by John Herschel on 16 December 1835. It has
NGC_1994
Nebula in the constellation Dorado
N41, LHA 120-N 41) is an emission nebula in the north part of the Large Magellanic Cloud in the Dorado constellation. Originally catalogued in Karl Henize's
N41_(nebula)
Emission nebula in the constellation Dorado
surrounding the Wolf-Rayet star BAT99-59. It is located in the Large Magellanic Cloud. The nebula was discovered on 30 December 1836 by polymath John
NGC_2020
Star in the constellation Dorado
R136b is a blue supergiant star in the R136 cluster in the Large Magellanic Cloud. It is one of the most massive and most luminous stars known. It is found
R136b
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
LBV, but variability has not been confirmed. S Doradus, in the Large Magellanic Cloud, in the southern constellation of Dorado. Prototype variable, LBVs
Hypergiant
Study of the movement of stars
velocities, or even ejected. A large-scale example is the gravitational interaction between the Milky Way and the Large Magellanic Cloud. A supernova explosion
Stellar_kinematics
Emission nebula in Dorado
emission nebula in the constellation of Dorado. It is located in the Large Magellanic Cloud and was discovered by John Herschel on 2 November 1834. A study
NGC_1714
Supernova remnant in the Dorado constellation
Constellation of Dorado around 160,000 light years from Earth in the Large Magellanic Cloud (LMC). The supernova occurred around 6660±770 years ago and had
DEM_L71
Massive star in the Large Magellanic Cloud
O-type star located in the Tarantula Nebula (30 Doradus) within the Large Magellanic Cloud (LMC). Identified as part of the VLT-FLAMES Tarantula Survey (VFTS)
VFTS_16
Variable star in the constellation Mensa
W Mensae (W Men) is an unusual yellow supergiant star in the Large Magellanic Cloud in the southern constellation Mensa. It is an R Coronae Borealis variable
W_Mensae
Spherical collection of stars
clusters contain multiple populations; the globular clusters in the Large Magellanic Cloud (LMC) exhibit a bimodal population, for example. During their youth
Globular_cluster
Wolf Rayet star in the constellation Dorado
VFTS 682 is a Wolf–Rayet star in the Large Magellanic Cloud. It is located over 29 parsecs (95 ly) north-east of the massive cluster R136 in the Tarantula
VFTS_682
Galaxy morphological classification scheme advocated by Edwin Hubble
fork. Examples of irregular galaxies: M82, NGC 1427A, Large Magellanic Cloud, Small Magellanic Cloud. Elliptical and lenticular galaxies are commonly referred
Hubble_sequence
Star cluster in the constellation Dorado
NGC 1852 is a star cluster in the Large Magellanic Cloud in the constellation Dorado. It was discovered in 1826 by James Dunlop with a 9-inch reflecting
NGC_1852
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