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is a list of the nearest hypergiant stars to Earth, located at a distance of up to 10,000 light-years (3,100 parsecs) from Earth. While hypergiants are
List_of_nearest_hypergiants
nearest giant stars List of nearest supergiants List of nearest hypergiants List of nearest bright stars Historical brightest stars List of nearest exoplanets
List_of_nearest_stars
supergiants. Lists of stars List of nearest hypergiants Applying the Stefan–Boltzmann law with a nominal solar effective temperature of 5,772 K: ( 5 , 772
List_of_nearest_supergiants
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
supernovae or hypernovae (For hypergiants 30-40 solar masses). Notable examples of hypergiants include the Pistol Star, a blue hypergiant located close to the
Hypergiant
nearest supergiants List of nearest hypergiants List of star systems within 20–25 light-years List of star systems within 25–30 light-years List of star
Lists_of_stars
Galaxies within 3.8 megaparsecs of the Solar System
overlapping with each other. Lists of astronomical objects List of galaxies List of nearest stars and brown dwarfs List of spiral galaxies Canis Major Overdensity
List_of_nearest_galaxies
450–500 light-years List of most distant stars List of nearest giant stars List of nearest supergiants List of nearest hypergiants List of novae in the Milky
Lists_of_astronomical_objects
nearest supergiants List of nearest hypergiants Calculated using an angular diameter of 5.99 mas. Calculated using an angular diameter of 5.25 mas. Calculated
List_of_nearest_giant_stars
Class of massive star with a spectral type of A to K
Ia, although they were not referred to as hypergiants until the late 1970s. Another criterion for hypergiants was also suggested in 1979 for some other
Yellow_hypergiant
Star at the centre of the Solar System
Sun paradox – Paradox concerning water on early Earth List of brightest stars List of nearest stars Midnight sun – Natural phenomenon when daylight lasts
Sun
Ballegoij, E. J. (2019). "Pulsations, eruptions, and evolution of four yellow hypergiants". Astronomy and Astrophysics. 631: A48. arXiv:1910.02460. Bibcode:2019A&A
List_of_largest_stars
of 48.9 light years corresponds to a minimum parallax of 66.7 mas. Lists of astronomical objects Interstellar travel Lists of stars List of nearest stars
List_of_nearest_bright_stars
brightest stars List of Chinese star names List of nearest bright stars List of proper names of exoplanets Lists of stars by constellation – gives variant names
List_of_proper_names_of_stars
magnitude List of variable stars List of brightest natural objects in the sky List of most massive stars List of most luminous stars List of nearest bright
List_of_brightest_stars
which maps the magnetic fields of stars List of directly imaged exoplanets Angular resolution Angular diameter List of nearest stars Published 2024 based
List of stars with resolved images
List_of_stars_with_resolved_images
Classification of stars based on spectral properties
Supergiants Red supergiant Hypergiants absolute magni- tude (MV) The conventional colour description takes into account only the peak of the stellar spectrum
Stellar_classification
Constellation in the northern celestial hemisphere
constellation hosts some of the most luminous stars known, including the yellow hypergiants Rho Cassiopeiae and V509 Cassiopeiae and white hypergiant 6 Cassiopeiae
Cassiopeia_(constellation)
Star that has a supergiant luminosity class, with a spectral type of F or G
giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) Yellow supergiants generally have spectral types of F and G, although sometimes late
Yellow_supergiant
Stars with a supergiant luminosity class with a spectral type of K or M
giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) Stars are classified as supergiants on the basis of their spectral luminosity class
Red_supergiant
Type of star, larger and brighter than the Sun
supergiant Hypergiants absolute magni- tude (MV) A giant star has a substantially larger radius and luminosity than a main-sequence (or dwarf) star of the same
Giant_star
00986. Bibcode:2017ASPC..509....3D. Atlas of the Universe, "The Universe within 12.5 Light Years: The Nearest Stars", Richard Powell, 30 July 2006 (accessed
List_of_white_dwarfs
Overview of the scientific field of astronomy
stars List of largest known stars List of brightest stars Historical brightest stars List of most luminous stars List of nearest stars List of nearest bright
Outline_of_astronomy
Stellar classification
diagram Solar analog Star count, survey of stars Yellow hypergiant "Glossary term: Luminosity Class". IAU Office of Astrononomy for Education (OAE) - astro4edu
G-type_main-sequence_star
Type of large cool star
Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A red giant is a luminous giant star of low or intermediate mass (roughly 0
Red_giant
Light from the stars
higher than for ordinary stars, presumably because of multiple scattering from dust grains. List of brightest stars Purkinje effect Sunlight Moonlight
Starlight
largest stars List of most luminous stars List of nearest bright stars List of nearest galaxies List of nearest stars Lists of stars Lists of stars by constellation
List_of_star_extremes
Type of star larger than main-sequence but smaller than a giant
Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A subgiant is a star that is brighter than a normal main-sequence star of the same spectral class
Subgiant
Type of star that is luminous, blue, and variable in brightness
luminous of all stars. During a normal outburst the temperature decreases to around 8,500 K for all stars, slightly hotter than the yellow hypergiants. The
Luminous_blue_variable
Planetary system consisting of the Sun and objects orbiting it
the Sun, the larger the distance between its orbit and the orbit of the next nearest object to the Sun. For example, Venus is approximately 0.33 AU farther
Solar_System
Scientific projections regarding the far future
System List of future astronomical events List of future calendar events List of radioactive nuclides by half-life Location of Earth History of Earth Future
Timeline_of_the_far_future
visible without a telescope. List of nearest stars List of star systems within 25–30 light-years Lists of stars List of nearest bright stars Brown, A. G.
List of star systems within 20–25 light-years
List_of_star_systems_within_20–25_light-years
Hot, luminous star with a spectral type of A9 or earlier
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A blue supergiant (BSG) is a hot, luminous
Blue_supergiant
Type of star that is massive and luminous
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) The title supergiant, as applied to a star
Supergiant
Stellar core remnant
Supergiants Red supergiant Hypergiants absolute magni- tude (MV) White dwarfs have low luminosity and therefore occupy a strip at the bottom of the Hertzsprung–Russell
White_dwarf
Hypothetical early-universe star with a black hole core
hole star, is a hypothetical type of extremely massive and luminous star that may have existed early in the history of the universe. Unlike modern stars
Quasi-star
Ignace, R.; Todt, H.; Hainich, R. (2017). "On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12
List_of_most_massive_stars
Comparison of a wide range of lengths
Ballegoij, E. J. (2019). "Pulsations, eruptions, and evolution of four yellow hypergiants". Astronomy and Astrophysics. 631: A48. arXiv:1910.02460. Bibcode:2019A&A
Orders_of_magnitude_(length)
Star of luminosity class VI under the Yerkes spectral classification system
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A subdwarf, sometimes denoted by "sd", is a
Subdwarf
Hypothetical astronomical object
horizon. List of nearest black holes Supermassive black hole Intermediate-mass black hole Stellar black hole Micro black hole Neutron star "New Type of Star
Planck_star
Main-sequence star of spectral type O
Supergiants Red supergiant Hypergiants absolute magni- tude (MV) An O-type main-sequence star is a main-sequence—core hydrogen-burning—star of spectral type O.
O-type_main-sequence_star
Event wherein the Sun is obscured by the Moon
Lists of solar eclipses List of films featuring eclipses Apollo–Soyuz: First joint U.S.–Soviet space flight. Mission included an arranged eclipse of the
Solar_eclipse
Red dwarfs. This is a list of exceptional red dwarfs. This is a list of red dwarfs that currently hold records. This is a list of red dwarfs with names
List_of_red_dwarfs
Sargent, B.; Forrest, W. J. (2006). "SpitzerSpectroscopy of Dusty Disks around B\e] Hypergiants in the Large Magellanic Cloud". The Astrophysical Journal
List_of_exoplanet_extremes
Substellar object
giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) Five different theories for the formation of brown dwarfs have been proposed: A
Brown_dwarf
Changes to stars over their lifespans
the course of time. Depending on the mass of the star, its lifetime can range from a few million years for the most massive to trillions of years for the
Stellar_evolution
Collapsed core of a massive star
impression of a neutron star bending light IRAS 00500+6713 (in 10,000 y) List of neutron stars Neutron stars in fiction Stars in fiction § Neutron stars
Neutron_star
Type of star
a red hypergiant (RHG) star that shows strong OH maser emission and is unusually bright at near-infrared wavelengths. In the very late stages of AGB evolution
OH/IR_star
Astronomical category of stars
two observed types of star: Binary stars with highly variable emission and stellar spectral type Fe a blue supergiant with a forest of forbidden FeII lines
Iron_star
Constellation in the northern celestial hemisphere
magnitude of 2.5. Delta Cephei is the prototype of an important class of star known as a Cepheid variable. RW Cephei, an orange hypergiant, together with
Cepheus_(constellation)
This is a list of notable brown dwarfs. These are objects that have masses between heavy gas giants and low-mass stars. The first isolated brown dwarf
List_of_brown_dwarfs
Visible star that is nearly aligned with Earth's axis of rotation
is within a degree of the latitude of the observer. The celestial pole will be nearest Polaris in 2100. Due to the precession of the equinoxes (as well
Pole_star
Large self-illuminated object in space
A star is a luminous spheroid of plasma held together by self-gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked
Star
Central region of the Sun
the hottest part of the Sun and of the Solar System. It has a density of 150,000 kg/m3 (150 g/cm3) at the center, and a temperature of 15,000,000 K (27
Solar_core
Process by which stars are named
stars. The most voluminous modern catalogues list on the order of a billion stars, out of an estimated total of 200 to 400 billion in the Milky Way. Proper
Stellar designations and names
Stellar_designations_and_names
Hypothetical hybrid star type
conjectured type of hybrid star wherein a red giant or red supergiant contains a neutron star at its core, formed from the collision of the giant with the
Thorne–Żytkow_object
Age of the universe List of largest cosmic structures List of exoplanet extremes Lists of astronomical objects List of most distant stars Timeline of knowledge
List of the most distant astronomical objects
List_of_the_most_distant_astronomical_objects
Type of neutron star with beams of radiation
ensemble of pulsars, and will be thus detected. The pulsars listed here were either the first discovered of its type, or represent an extreme of some type
Pulsar
Gas and dust surrounding a newly formed star
A protoplanetary disk is a rotating circumstellar disc of dense gas and dust surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star
Protoplanetary_disk
Astrophysical limit on radiation from stars
2023-04-18. R. B. Stothers (2003). "Turbulent pressure in the envelopes of yellow hypergiants and luminous blue variables". Astrophysical Journal. 589 (2): 960–967
Eddington_luminosity
Hypothesized alternative to a black hole
In astrophysics, a gravastar (a blend word of "gravitational vacuum star") is an object hypothesized in a 2001 paper by Pawel O. Mazur and Emil Mottola
Gravastar
Supernova at least ten times more luminous than a standard supernova
candidates of hypergiants or LBVs that appear to be undergoing substantial mass loss, due to Eddington instability, for example, SN2005gl. Another type of suspected
Superluminous_supernova
Stage of stellar evolution
Humphreys, Roberta (July 2016). "LBVs, hypergiants and impostors — the evidence for high mass loss events". Journal of Physics: Conference Series. 728 (2)
Blue_loop
This is a list of Arabic star names. In Western astronomy, most of the accepted star names are Arabic, a few are Greek and some are of unknown origin.
List_of_Arabic_star_names
Astrophysical phenomenon
hypergiants (including LBVs). The narrow spectral lines for which they are named occur because the supernova is expanding into a small dense cloud of
Supernova
Triangulum Galaxy is around 3.2 Mly distant List of Wolf–Rayet stars List of luminous blue variable stars List of nearest stars by spectral type Barry, Don C
List_of_O-type_stars
Region of an astronomical diagram
variables. In the specific region of more luminous stars above the instability strip are found the yellow hypergiants which have irregular pulsations and
Instability_strip
Methods for estimating the age of a star
assignment of rough ages to a large number of stars present within. When one can determine the age of stars through other methods, such as the ones listed above
Stellar_age_estimation
This is a list of the most distant individually seen stars discovered, a list of the most distant stars that are separately known, resolved as individual
List_of_most_distant_stars
Hypothetical class of star that develops from a red dwarf
A blue dwarf is a hypothetical class of star that develops from a red dwarf after it has exhausted much of its hydrogen fuel supply. Because red dwarfs
Blue_dwarf_(red-dwarf_stage)
Star's outer shell from which light is radiated
becomes opaque, equivalent to an optical depth of approximately 2⁄3, or equivalently, a depth from which 50% of light will escape without being scattered.
Photosphere
Feature of the Hertzsprung-Russell diagram
Hertzsprung gap is a feature of the Hertzsprung–Russell diagram for a star cluster, notable for the relative absence of stars compared to nearby regions
Hertzsprung_gap
Dim, low mass stars on the main sequence
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) Red dwarfs are very-low-mass stars. As a result
Red_dwarf
Stars sorted by absolute magnitude
Najarro, F.; Ramachandran, V.; Vink, J. S. (April 2026). "The winds of OBA hypergiants and luminous blue variables: Dynamically consistent atmosphere models
List_of_most_luminous_stars
Curve on the Hertzsprung-Russell diagram representing stars of a particular age
curve on the Hertzsprung-Russell diagram, representing a population of stars of the same age but with different mass. The Hertzsprung-Russell diagram
Stellar_isochrone
Chemically peculiar stars
Carbon-enhanced metal-poor stars, usually referred to as CEMP stars, are a class of chemically peculiar star. CEMP stars have [C/Fe] > +1, which means compared
CEMP_star
Type of star
object, a quark star made of strange quark matter. Strange stars might exist without regard to the Bodmer–Witten assumption of stability at near-zero temperatures
Strange_star
Astronomical objects of planetary size that did not form in orbit around a star
planet Substellar object List of planet types Lists of astronomical objects Working Group on Extrasolar Planets – Definition of a "Planet" Archived 16 September
Sub-brown_dwarf
Hot, giant star of early spectral type
Supergiants Red supergiant Hypergiants absolute magni- tude (MV) In astronomy, a blue giant is a hot star with a luminosity class of III (giant) or II (bright
Blue_giant
Theoretical stellar remnant
current age of the universe (13.79 billion years), no black dwarfs are expected to exist in the universe at the present time. The temperature of the coolest
Black_dwarf
Cavity of hot gas blown from a star
high-velocity (several thousand km/s) stellar wind from a single massive star of type O or B. Weaker stellar winds also blow bubble structures, which are also
Stellar-wind_bubble
Heterogeneous class of stars with unusual spectra
explode while at the yellow hypergiant or LBV stage, but many become Wolf–Rayet stars. They have lost or burnt almost all of their hydrogen and are now
Wolf–Rayet_star
Isolated, small, and opaque nebula
nebula (IC 1590 cluster) Barnard 68, at a distance of only 410 light-years, is one of the nearest Bok globules. Its diameter is about 12,500 AU (0.198 ly)
Bok_globule
Stellar classification distinguished by bright blue luminosity
Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A B-type main-sequence star is a main-sequence (core hydrogen-burning) star of spectral type B.
B-type_main-sequence_star
Timeline of stellar astronomy 1200 BC — Chinese star names appear on oracle bones used for divination. 134 BC — Hipparchus creates the magnitude scale of stellar
Timeline_of_stellar_astronomy
Structure formed by diffuse material in orbital motion around a massive central body
compress and raise the temperature of the material, causing the emission of electromagnetic radiation. The frequency range of that radiation depends on the
Accretion_disk
Stars that have had their light output measured carefully
Photometric-standard stars are a series of stars that have had their light output in various passbands of photometric system measured very carefully.
Photometric-standard_star
Stars with strong methylidyne absorption bands in their spectra
CH stars are particular type of carbon stars which are characterized by the presence of exceedingly strong absorption bands due to CH (methylidyne) in
CH_star
Supernova that ejects a large mass at unusually high velocity
used to describe hypothetical explosions from diverse events such as hypergiants, extremely massive population III stars in the early universe, or from
Hypernova
Peculiar star with unusually low amount of iron
A Lambda Boötis star is a type of chemically peculiar star which has an unusually low abundance of iron peak elements in its surface layers. One possible
Lambda_Boötis_star
Star not gravitationally bound to any galaxy
hundreds of thousands of light-years from the nearest star or galaxy. Most intergalactic star candidates found in the neighborhood of the Milky Way seem
Intergalactic_star
Process where a red giant star engulfs a planet
in which a star at the end of its main sequence phase of its life expands into a red giant star and engulfs some or all of the planets or brown dwarfs
Stellar_engulfment
Mass of a star in astronomy
requires |journal= (help)CS1 maint: multiple names: authors list (link) LiveScience.com, "Mystery of the 'Monster Stars' Solved: It Was a Monster Mash", Natalie
Stellar_mass
System of two stars orbiting each other
observing how quickly the brightness changes as the disc of the nearest star slides over the disc of the other star. If it is also a spectroscopic binary
Binary_star
Structure of stars
structure of a star in detail and make predictions about the luminosity, the color and the future evolution of the star. Different classes and ages of stars
Stellar_structure
Pattern of stars recognized on Earth's night sky
background of Aldebaran the Hyades, the nearest star cluster and one of five first-magnitude deep-sky objects, two of which can be seen just north-east of the
Asterism_(astronomy)
Astronomical object without the mass to sustain hydrogen fusion
as small as 8 Jupiter masses have been called brown dwarfs. Brown dwarf List of planet types Planet Red dwarf Sub-brown dwarf Quoted as Chabrier and Baraffe:
Substellar_object
Constellation in the southern celestial hemisphere
magnitude of 4.2 and a maximum magnitude of 3.3; it has a period of 35.5 days. V382 Carinae is a yellow hypergiant, one of the rarest types of stars. It
Carina_(constellation)
Small number of stars that orbit each other
(2005). Modern Dictionary of Astronomy and Space Technology. New Delhi: Deep & Deep Publications. ISBN 81-7629-741-0. "The 100 Nearest Star Systems". Archived
Star_system
Hypothetical types of stars
excluded from the list of quark star candidates. An electroweak star is a hypothetical type of exotic star in which the gravitational collapse of the star is
Exotic_star
Set of non-stellar objects in orbit around a star
contain high numbers of population II stars. In 2014, the first planets around a halo star were announced around Kapteyn's star, the nearest halo star to Earth
Planetary_system
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LIST OF-NEAREST-HYPERGIANTS
LIST OF-NEAREST-HYPERGIANTS
LIST OF-NEAREST-HYPERGIANTS
LIST OF-NEAREST-HYPERGIANTS
LIST OF-NEAREST-HYPERGIANTS
LIST OF-NEAREST-HYPERGIANTS
LIST OF-NEAREST-HYPERGIANTS
LIST OF-NEAREST-HYPERGIANTS
LIST OF-NEAREST-HYPERGIANTS
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