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GALACTIC PLANE

  • Galactic plane
  • Plane on which most of a disk-shaped galaxy's mass lies

    The galactic plane is the plane on which most of a disk-shaped galaxy's mass lies.[citation needed] The directions perpendicular to the galactic plane point

    Galactic plane

    Galactic plane

    Galactic_plane

  • Galactic coordinate system
  • Celestial coordinate system in spherical coordinates, with the Sun as its center

    center of the Milky Way Galaxy, and the fundamental plane parallel to an approximation of the galactic plane but offset to its north. It uses the right-handed

    Galactic coordinate system

    Galactic coordinate system

    Galactic_coordinate_system

  • Galactic quadrant
  • One of four circular sectors of the Milky Way galaxy

    (Southern Galactic Plane Survey) focuses on Romulans". "Galactic quadrants" within Star Wars canon astrography map depicts a top-down view of the galactic disk

    Galactic quadrant

    Galactic quadrant

    Galactic_quadrant

  • Ecliptic
  • Apparent path of the Sun on the celestial sphere

    inclined to the galactic plane by 60°. Because Earth's rotational axis is not perpendicular to its orbital plane, Earth's equatorial plane is not coplanar

    Ecliptic

    Ecliptic

    Ecliptic

  • STS-51-F
  • 1985 American crewed spaceflight

    mission, and while it did have some problems, it observed 60% of the galactic plane in infrared light. During launch, Challenger experienced multiple sensor

    STS-51-F

    STS-51-F

    STS-51-F

  • Milky Way
  • Galaxy containing the Solar System

    visible region of the Milky Way's galactic plane occupies an area of the sky that includes 30 constellations. The Galactic Center lies in the direction of

    Milky Way

    Milky Way

    Milky_Way

  • Galactic orientation
  • Spatial orientation of a galactic plane

    A galactic orientation describes the spatial orientation of a galactic plane, where such exists for a given galaxy. For a spiral galaxy, this can be obtained

    Galactic orientation

    Galactic_orientation

  • Supergalactic plane
  • Local-universe structure

    The Supergalactic plane (SGP) is a plane roughly perpendicular to the Galactic plane of the Milky Way. It represents a planar structure in the local distribution

    Supergalactic plane

    Supergalactic plane

    Supergalactic_plane

  • Zone of Avoidance
  • Area of sky obscured by the Milky Way

    the attenuation, interstellar dust and stars in the plane of the Milky Way (the galactic plane) obstruct the view of around 20% of the extragalactic

    Zone of Avoidance

    Zone of Avoidance

    Zone_of_Avoidance

  • Great Attractor
  • Region of gravitational attraction in the local universe

    difficult to observe at visible wavelengths because it lies behind the galactic plane of the Milky Way, within the Zone of Avoidance. Dust, gas, and foreground

    Great Attractor

    Great Attractor

    Great_Attractor

  • Supergalactic coordinate system
  • Astronomical coordinate system

    Way galactic plane) Camelopardalis Ursa Major Coma Berenices (near the Milky Way galactic north pole) Virgo Centaurus Circinus (in the galactic plane) Triangulum

    Supergalactic coordinate system

    Supergalactic coordinate system

    Supergalactic_coordinate_system

  • Virgin Galactic
  • Space tourism company

    Virgin Galactic Holdings, Inc. is a British-American spaceflight company founded by Richard Branson and the Virgin Group conglomerate, which retains an

    Virgin Galactic

    Virgin_Galactic

  • UKIRT Infrared Deep Sky Survey
  • Astronomical survey

    view of the Galactic Plane than is possible at optical wavelengths, due to absorption by material in the disk of the galaxy. The GCS (Galactic) covers an

    UKIRT Infrared Deep Sky Survey

    UKIRT Infrared Deep Sky Survey

    UKIRT_Infrared_Deep_Sky_Survey

  • Bolocam Galactic Plane Survey
  • Astronomical survey

    the Bolocam Galactic Plane Survey (BGPS) took place from June 2005 until September 2007 and covers 170 square degrees of the galactic plane visible from

    Bolocam Galactic Plane Survey

    Bolocam Galactic Plane Survey

    Bolocam_Galactic_Plane_Survey

  • Night sky
  • Appearance of the sky in a clear night

    half of the galactic plane. Main dark nebulae of the Solar antapex half of the galactic plane. Main stellar associations of the galactic plane in the night

    Night sky

    Night sky

    Night_sky

  • Shapley Attractor
  • Attractor in the Shapley Supercluster

    gravitational pull. Like the Great Attractor, it is obscured by the Milky Way's galactic plane, lying behind the Zone of Avoidance (ZOA), so that in visible light

    Shapley Attractor

    Shapley_Attractor

  • Galaxy
  • System of stars and interstellar matter

    account the absorption of light by interstellar dust present in the galactic plane; but after Robert Julius Trumpler quantified this effect in 1930 by

    Galaxy

    Galaxy

    Galaxy

  • 2012 phenomenon
  • Eschatological beliefs about the year

    orbit of the galactic center cause it to regularly pass through the galactic plane. When the Sun's orbit takes it outside the galactic plane which bisects

    2012 phenomenon

    2012 phenomenon

    2012_phenomenon

  • Thin disk
  • Structural component of galaxies

    the center. The thin disk contributes about 85% of the stars in the Galactic plane and 95% of the total stars in the disk. It can be set apart from the

    Thin disk

    Thin disk

    Thin_disk

  • Wolf–Rayet star
  • Heterogeneous class of stars with unusual spectra

    the near-infrared dedicated to discovering this kind of object in the Galactic plane. It is expected that there are fewer than 1,000 WR stars in the rest

    Wolf–Rayet star

    Wolf–Rayet star

    Wolf–Rayet_star

  • Galactic Center
  • Rotational center of the Milky Way galaxy

    The Galactic Center is the barycenter of the Milky Way and a corresponding point on the rotational axis of the galaxy. Its central massive object is a

    Galactic Center

    Galactic Center

    Galactic_Center

  • Galactic Center filament
  • Large structures found in the center of the Milky Way

    exist, running perpendicular and parallel to the galactic plane, respectively, away from the Galactic Center. Vertical filaments possess strong magnetic

    Galactic Center filament

    Galactic Center filament

    Galactic_Center_filament

  • 3I/ATLAS
  • Interstellar comet in 2025

    border of the constellations Serpens Cauda and Sagittarius, near the galactic plane. It was given the temporary designation 'A11pl3Z' and the discovery

    3I/ATLAS

    3I/ATLAS

    3I/ATLAS

  • Spiral galaxy
  • Class of galaxy that has spiral structures extending from their cores

    close to a single plane (the galactic plane) in more or less conventional circular orbits around the center of the galaxy (the Galactic Center), or in a

    Spiral galaxy

    Spiral galaxy

    Spiral_galaxy

  • Open cluster
  • Type of star cluster

    in a more irregular shape. These were generally found in or near the galactic plane of the Milky Way. Astronomers dubbed the former globular clusters, and

    Open cluster

    Open cluster

    Open_cluster

  • Astronomical coordinate systems
  • System for specifying positions of celestial objects

    the direction towards the Galactic Center. Galactic latitude resembles the elevation above the galactic plane and galactic longitude determines direction

    Astronomical coordinate systems

    Astronomical coordinate systems

    Astronomical_coordinate_systems

  • Ionization cone
  • Astronomical phenomenon

    with respect to the galactic plane (galactic disc), however, ionization cones usually align with radio sources near the galactic nucleus. The two large

    Ionization cone

    Ionization cone

    Ionization_cone

  • Scholz's Star
  • Binary stellar systems in the constellation Monoceros

    (6.8 parsecs) from the Sun in the constellation Monoceros near the galactic plane. It was discovered in 2013 by astronomer Ralf-Dieter Scholz. In 2015

    Scholz's Star

    Scholz's_Star

  • Serpens
  • Constellation split into two non-contiguous parts

    galaxies. Part of the Milky Way's galactic plane passes through Serpens Cauda, which is therefore rich in galactic deep-sky objects, such as the Eagle

    Serpens

    Serpens

    Serpens

  • Galactic North
  • 2006 short story collection by Alastair Reynolds

    Galactic North is a collection of science fiction short stories by British author Alastair Reynolds, published by Gollancz in 2006. It comprises most of

    Galactic North

    Galactic_North

  • Perseus (constellation)
  • Constellation in the northern celestial hemisphere

    et Caput Medusae; however, this never came into popular usage. The galactic plane of the Milky Way passes through Perseus, whose brightest star is the

    Perseus (constellation)

    Perseus (constellation)

    Perseus_(constellation)

  • GRO J1655−40
  • Binary star

    the "Solar circle", d~8,500 pc, and within 150 pc (~500 ly) of the galactic plane. For comparison, the Sun and other nearby stars have typical speeds

    GRO J1655−40

    GRO J1655−40

    GRO_J1655−40

  • Galaxy filament
  • Largest structures in the universe, made of galaxies

    are the largest known structures in the universe, consisting of walls of galactic superclusters. These massive, thread-like formations can commonly reach

    Galaxy filament

    Galaxy filament

    Galaxy_filament

  • Scutum Supershell
  • Superbubble in the Scutum-Centaurus arm

    diameter of approximately 290 pc and extends about 400 pc from the galactic plane, which was derived from a kinematic distance of 3.3 kpc calculated from

    Scutum Supershell

    Scutum Supershell

    Scutum_Supershell

  • Butterfly Cluster
  • Open cluster in Scorpius

    of 204.2 Myr. At present it is 23 ly (7 pc) below the galactic plane, and it will cross the plane every 29.4 Myr. List of open clusters List of Messier

    Butterfly Cluster

    Butterfly Cluster

    Butterfly_Cluster

  • Wild Duck Cluster
  • Open cluster in the constellation Scutum

    The cluster is located 6.8 kpc (22,000 ly) from the Galactic Center, close to the galactic plane, and is not far from its birthplace. A portion of M11

    Wild Duck Cluster

    Wild Duck Cluster

    Wild_Duck_Cluster

  • Star-forming regions of Cassiopeia
  • Star-forming regions in the constellation Cassiopeia

    complex [it], situated in a very northern position relative to the galactic plane and first observed by Edwin Hubble. The more visible and extensive areas

    Star-forming regions of Cassiopeia

    Star-forming regions of Cassiopeia

    Star-forming_regions_of_Cassiopeia

  • Stellar density
  • Number of stars within a unit volume

    direction out of the galactic plane. The locations within the Milky Way that have the highest stellar density are the galactic core and the center of

    Stellar density

    Stellar_density

  • Serpens–Aquila Rift
  • Sky region containing dark interstellar clouds

    the nearby dark cloud of cosmic dust that obscures the middle of the galactic plane of the Milky Way, looking inwards and towards its other radial sectors

    Serpens–Aquila Rift

    Serpens–Aquila Rift

    Serpens–Aquila_Rift

  • Solar System
  • Planetary system consisting of the Sun and objects orbiting it

    Vega. The plane of the ecliptic lies at an angle of about 60° to the galactic plane. The Sun follows a nearly circular orbit around the Galactic Center (where

    Solar System

    Solar System

    Solar_System

  • Gould Belt
  • Ring of stars in the Milky Way galaxy

    Belt is a local ring of stars in the Milky Way, tilted away from the galactic plane by about 16–20 degrees, first reported by John Herschel and Benjamin

    Gould Belt

    Gould Belt

    Gould_Belt

  • Dark nebula
  • Type of interstellar cloud that obscures visible light

    Main dark nebulae of the solar apex half of the galactic plane

    Dark nebula

    Dark nebula

    Dark_nebula

  • NGC 1220
  • Open cluster in Perseus

    located at l = 143.04°, b = −3.96° in the galactic coordinate system, and is 120 parsecs above the galactic plane. It is approximately 6m 42s east and 10′

    NGC 1220

    NGC 1220

    NGC_1220

  • Galactic habitable zone
  • Region of a galaxy in which life might most likely develop

    astrophysics, the galactic habitable zone is the region of a galaxy in which life is most likely to develop. The concept of a galactic habitable zone analyzes

    Galactic habitable zone

    Galactic habitable zone

    Galactic_habitable_zone

  • Thick disk
  • Structural component of some galaxies

    number density between 1 and 5 kiloparsecs (3.3 and 16.3 kly) above the galactic plane and, in the solar neighborhood, is composed almost exclusively of older

    Thick disk

    Thick disk

    Thick_disk

  • Wow! signal
  • 1977 radio signal detected as part of SETI

    therefore about 19° toward the southeast of the galactic plane, and about 24° or 25° east of the Galactic Center. The region of the sky in question lies

    Wow! signal

    Wow! signal

    Wow!_signal

  • Jan Oort
  • Dutch astronomer (1900–1992)

    be present to account for the stellar motions perpendicular to the Galactic plane. Comparing this mass to the visible stars and gas, in 1932, he wrote

    Jan Oort

    Jan Oort

    Jan_Oort

  • G54.1+0.3
  • Supernova remnant in the constellation Sagitta

    Sagitta. It was identified as a supernova remnant in a study of the galactic plane in the radio continuum at wavelengths of 21 and 11 cm. SNR G054.1+00

    G54.1+0.3

    G54.1+0.3

    G54.1+0.3

  • Planet Nine
  • Hypothetical Solar System planet

    the emission from the galactic nebulae, making detection of Planet Nine thermal emission problematically close to the galactic plane or bulge. A 2025 paper

    Planet Nine

    Planet Nine

    Planet_Nine

  • Sun
  • Star at the centre of the Solar System

    "north" and "south" of the galactic plane with a different period, around 83 million years, moving about 99 parsecs away from the plane. The point around which

    Sun

    Sun

    Sun

  • The Eerie Silence
  • 2010 book by Paul Davies

    about habitability on the Galactic Plane. The theory is as such: the Solar System moves up and down relative to the Galactic Plane, in a cycle of 62 million

    The Eerie Silence

    The_Eerie_Silence

  • HESS J1731−347
  • Supernova remnant

    is a young supernova remnant (SNR) located in the southern Milky Way Galactic plane. It was discovered in very-high-energy (VHE) gamma rays by the High

    HESS J1731−347

    HESS J1731−347

    HESS_J1731−347

  • North Polar Spur
  • polarised emission, it extends into the northern galactic hemisphere, roughly perpendicular to the galactic plane. It cannot be seen at optical wavelengths,

    North Polar Spur

    North Polar Spur

    North_Polar_Spur

  • NGC 6946
  • Galaxy in the constellations Cepheus & Cygnus

    heavily obscured by interstellar matter due to its location close to the galactic plane of the Milky Way. Due to its prodigious star formation it has been classified

    NGC 6946

    NGC 6946

    NGC_6946

  • Galactic ridge
  • Region of space

    The galactic ridge is a region of the inner galaxy that is coincident with the galactic plane of the Milky Way. It can be seen from Earth as a band of

    Galactic ridge

    Galactic_ridge

  • Cosmic ray
  • High-energy particle, mainly originating outside the Solar System

    populations correlate with the motion of the Earth relative to the galactic plane and increases in exposure to cosmic rays. The researchers suggest that

    Cosmic ray

    Cosmic ray

    Cosmic_ray

  • Circinus Galaxy
  • Galaxy in the constellation Circinus

    in the constellation of Circinus. It is located 4 degrees below the Galactic plane, and, at a distance of 4.0 Mpc (13 Mly), is one of the closest major

    Circinus Galaxy

    Circinus Galaxy

    Circinus_Galaxy

  • Cluster
  • Topics referred to by the same term

    cluster, a spherical collection of stars that orbits a galaxy in the galactic plane Cancer cluster, in biomedicine, an occurrence of a greater-than-expected

    Cluster

    Cluster

  • Great Rift (astronomy)
  • Interstellar clouds of cosmic dust

    skies, the rift appears as clear as the bright bulge of stars around the Galactic Center does to the naked eye or binoculars. The rift is largely between

    Great Rift (astronomy)

    Great Rift (astronomy)

    Great_Rift_(astronomy)

  • Local Bubble
  • Milky Way superbubble

    to be narrower in the galactic plane, becoming somewhat egg-shaped or elliptical, and may widen above and below the galactic plane, becoming shaped like

    Local Bubble

    Local Bubble

    Local_Bubble

  • Corona Australis Molecular Cloud
  • Molecular cloud in constellation Corona Australis

    stretches roughly 8ly across. The cloud is located at about 18% below the galactic plane and covers an angular area of 16.0° × 6.5° on the celestial sphere.

    Corona Australis Molecular Cloud

    Corona Australis Molecular Cloud

    Corona_Australis_Molecular_Cloud

  • Messier 37
  • Open cluster in the constellation Auriga

    4 kpc) from, the Galactic Center. It reaches a peak distance above the galactic plane of 0.29 kly (0.089 kpc) and will cross the plane with a period of

    Messier 37

    Messier 37

    Messier_37

  • Westerhout 49
  • Strong radio source in the constellation of Sagittarius

    kpcs or 36,000 light years. and it lies in the galactic plane about the same distance from the Galactic Center as does the Sun. It has been compared to

    Westerhout 49

    Westerhout 49

    Westerhout_49

  • Messier 107
  • Globular cluster in Ophiuchus

    Ophiuchi. M107 is close to the galactic plane and about 20,900 light-years from Earth and 9,800 ly (3,000 pc) from the Galactic Center. Its orbit is partly

    Messier 107

    Messier 107

    Messier_107

  • RELIKT-1
  • Soviet cosmic microwave background experiment on the Prognoz 9 satellite

    Cosmic Background Explorer in 1989) and measured the CMB dipole, the Galactic plane, and gave upper limits on the quadrupole moment. A follow-up, RELIKT-2

    RELIKT-1

    RELIKT-1

  • Interacting galaxy
  • Galaxies with interacting gravitational fields

    fields result in a disturbance of one another. There are several types of galactic interactions, including major interactions, minor interactions, and galaxy

    Interacting galaxy

    Interacting galaxy

    Interacting_galaxy

  • Struve 2398
  • Binary star system in the constellation Draco

    as 9 kpc from the Galactic Center. The plane of their galactic orbit carries them as far as 463−489 pc away from the galactic plane. Both stars of the

    Struve 2398

    Struve_2398

  • NGC 4698
  • Galaxy in the constellation Virgo

    that is aligned perpendicularly to the galactic disk. The bulge likewise appears elongated out of the galactic plane. This unusual alignment may have been

    NGC 4698

    NGC 4698

    NGC_4698

  • Paul L. Hertz
  • American astrophysicist

    Harvard University, with a thesis titled "Surveys of Globular Cluster and Galactic Plane X-Ray Sources". Hertz received the Robert Trumpler award of the Astronomical

    Paul L. Hertz

    Paul L. Hertz

    Paul_L._Hertz

  • Messier 56
  • Globular cluster in the constellation Lyra

    It is about 31–32 kly (9.5–9.8 kpc) from the Galactic Center and 4.8 kly (1.5 kpc) above the galactic plane. This cluster has an estimated age of 13.70

    Messier 56

    Messier 56

    Messier_56

  • Draco Dwarf
  • Spheroidal galaxy in the constellation Draco

    situated in the direction of the Draco Constellation at 34.6° above the galactic plane. Paul W. Hodge analyzed the distribution of its stars in 1964 and concluded

    Draco Dwarf

    Draco Dwarf

    Draco_Dwarf

  • Radcliffe wave
  • Coherent, wave-shaped gaseous structure in the Milky Way

    wave in the galactic plane". Newsweek. "Something Appears to Have Collided with the Milky Way and Created a Huge Wave in the Galactic Plane". Radcliffe

    Radcliffe wave

    Radcliffe wave

    Radcliffe_wave

  • Planetary nebula
  • Type of emission nebula created by dying red giants

    concentrated in the galactic plane, probably produced by relatively young massive progenitor stars; and bipolars in the galactic bulge appear to prefer

    Planetary nebula

    Planetary nebula

    Planetary_nebula

  • LHS 1815 b
  • Exoplanet

    exoplanet discovered in 2020 by TESS. The planet is located outside the galactic plane. LHS 1815 b is a terrestrial planet (super-Earth) with a mass of 0.0132

    LHS 1815 b

    LHS_1815_b

  • IC 2631
  • Reflection nebula in Chamaeleon

    at a distance of ~630 light years. It can be found 14.9° above the galactic plane of the Milky Way. IC 2631 can be easily seen in the southern hemisphere

    IC 2631

    IC 2631

    IC_2631

  • VVV CL160
  • Globular cluster

    with in the galactic plane of the Milky Way galaxy. It is located 29 parsecs above the galactic plane and 4.2 kiloparsecs from the galactic center of the

    VVV CL160

    VVV_CL160

  • Necklace Nebula
  • Planetary nebula in the constellation Sagitta

    (IPHAS), a ground-based H-alpha planetary nebula study of the North Galactic Plane. The Necklace Nebula is the exploded aftermath of a giant star that

    Necklace Nebula

    Necklace Nebula

    Necklace_Nebula

  • Multi-messenger astronomy
  • Coordination of related astronomical observations

    the release of neutrinos from the galactic plane of the Milky Way galaxy, creating the first neutrino-based galactic map. Bartos, Imre; Kowalski, Marek

    Multi-messenger astronomy

    Multi-messenger astronomy

    Multi-messenger_astronomy

  • Vulpecula
  • Constellation in the northern celestial hemisphere

    nearly 100 OB stars and over 800 young stellar objects. It lies in the galactic plane, at a distance of about 2,300 parsec. It contains the emission-line

    Vulpecula

    Vulpecula

    Vulpecula

  • Caltech Submillimeter Observatory
  • Decommissioned radio telescope in Hawaii, US

    Effect. The Bolocam Galactic Plane Survey, a survey of continuum emission at 1.1 mm, which covered 170 square degrees of the galactic plane. This survey resulted

    Caltech Submillimeter Observatory

    Caltech Submillimeter Observatory

    Caltech_Submillimeter_Observatory

  • Far-infrared astronomy
  • Scientific study of celestial objects visible in wavelengths of 30-450 μm

    circumstellar envelopes around numerous old red giant stars. The Bolocam Galactic Plane Survey mapped the galaxy for the first time in the far-infrared. On

    Far-infrared astronomy

    Far-infrared astronomy

    Far-infrared_astronomy

  • 2026 in science
  • Binary Microlensing Event Revealing a Planetary Companion toward the Galactic Plane". The Astrophysical Journal Letters. 1005 (2): L33. arXiv:2607.01853

    2026 in science

    2026 in science

    2026_in_science

  • Messier 93
  • Open cluster in the constellation Puppis

    years. It is nearly on the galactic plane and has an orbit that varies between 28–29 kly (8.5–8.9 kpc) from the Galactic Center over a period of 242

    Messier 93

    Messier 93

    Messier_93

  • HIP 13044
  • Star in the constellation Fornax

    As a result, HIP 13044 circles the Galactic Center at a highly irregular orbit with respect to the galactic plane. HIP 13044 is slightly less massive

    HIP 13044

    HIP 13044

    HIP_13044

  • Messier 18
  • Open cluster in the constellation Sagittarius

    6.5 kpc to, and as far as 6.8 kpc from the galactic core. It passes vertically through the galactic plane once every 27.4 million years, ranging no more

    Messier 18

    Messier 18

    Messier_18

  • List of most luminous stars
  • Stars sorted by absolute magnitude

    completely swamped by the primary. Mercer 23 is an open cluster near Galactic plane. Mercer 30 is an open cluster in Dragonfish Nebula. The paper mistakenly

    List of most luminous stars

    List of most luminous stars

    List_of_most_luminous_stars

  • Midcourse Space Experiment
  • Space telescope

    piece of the rocket. Operational from 1996 to 1997, MSX mapped the galactic plane and areas either missed or identified as particularly bright by the

    Midcourse Space Experiment

    Midcourse Space Experiment

    Midcourse_Space_Experiment

  • Cassiopeia Dwarf
  • Galaxy in the constellation Cassiopeia

    Andromeda Galaxy (M31). In the sky, it appears behind the Milky Way's galactic plane, and so it is reddened by 0.194 magnitudes. With a luminosity of 1.8×107 L☉

    Cassiopeia Dwarf

    Cassiopeia Dwarf

    Cassiopeia_Dwarf

  • High Altitude Water Cherenkov Experiment
  • Gamma-ray and cosmic ray observatory in Puebla, Mexico

    energies) Galactic sources in the TeV with a sensitivity similar to that of Fermi in the GeV, detect diffuse emission from regions of the Galactic plane, have

    High Altitude Water Cherenkov Experiment

    High Altitude Water Cherenkov Experiment

    High_Altitude_Water_Cherenkov_Experiment

  • HM 1
  • Open cluster in the constellation Scorpius

    open cluster located in the constellation of Scorpius, close to the galactic plane. It was first observed by R. J. Havlen and A. F. J. Moffat in 1976.

    HM 1

    HM 1

    HM_1

  • Orion–Eridanus Superbubble
  • Structure in the Milky Way Galaxy

    outside. More recent studies suggest that the superbubble extends to the Galactic plane and that both Barnard's Loop and the λ Orionis Nebula lie inside. The

    Orion–Eridanus Superbubble

    Orion–Eridanus Superbubble

    Orion–Eridanus_Superbubble

  • List of astronomical catalogues
  • List from the Alphabet Direction (αβ)

    Gamma-Ray source IPHAS — The INT Photometric Hα Survey of the Northern Galactic Plane IPHASX — INT/WFC Photometric Hα Survey extended object IRAS — Infrared

    List of astronomical catalogues

    List_of_astronomical_catalogues

  • Stellar flyby
  • Astronomy phenomenon

    (6.8 parsecs) from the Sun in the constellation Monoceros near the galactic plane. The system passed through the Solar System's Oort cloud roughly 70

    Stellar flyby

    Stellar_flyby

  • Classical Cepheid variable
  • Type of variable star

    such as the local spiral arm structure and the Sun's distance from the galactic plane. Around 3,600 classical Cepheids are known in the Milky Way galaxy.

    Classical Cepheid variable

    Classical Cepheid variable

    Classical_Cepheid_variable

  • List of nearest known black holes
  • parameters for Gaia18cbf - a long gravitational microlensing event in the Galactic plane". Astronomy and Astrophysics. 662: A59. arXiv:2111.08337. Bibcode:2022A&A

    List of nearest known black holes

    List_of_nearest_known_black_holes

  • Dark Doodad Nebula
  • Nebula in the constellation Musca

    cluster NGC 4372, much closer than the centre of the galaxy and in the galactic plane, having a length of nearly three degrees of arc. Although officially

    Dark Doodad Nebula

    Dark Doodad Nebula

    Dark_Doodad_Nebula

  • High-velocity cloud
  • Large collections of gas found in the galactic halo of the Milky Way

    galactic plane. This was quite notable because the models of the Milky Way showed the density of gas decreasing with distance from the galactic plane

    High-velocity cloud

    High-velocity_cloud

  • Infrared dark cloud
  • Cold, dense region of a giant molecular cloud

    silhouette against the bright diffuse mid-infrared emission from the galactic plane. Infrared dark clouds have only been recently discovered in 1996 using

    Infrared dark cloud

    Infrared dark cloud

    Infrared_dark_cloud

  • MeerKAT
  • 64-antenna radio telescope in South Africa

    ASTRON, The Netherlands MeerGAL (MeerKAT High Frequency Galactic Plane Survey) – Galactic structure and dynamics, distribution of ionised gas, recombination

    MeerKAT

    MeerKAT

    MeerKAT

  • CWISE J1249+3621
  • Low-mass hypervelocity star

    is an extragalactic star, because its motion is confined within the galactic plane, which makes an origin within the Milky Way more likely. More research

    CWISE J1249+3621

    CWISE J1249+3621

    CWISE_J1249+3621

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GALACTIC PLANE

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GALACTIC PLANE