AI & ChatGPT searches , social queriess for HYPERGIANT
Search references for HYPERGIANT. Phrases containing HYPERGIANT
See searches and references containing HYPERGIANT!
Search references for HYPERGIANT. Phrases containing HYPERGIANT
See searches and references containing HYPERGIANT!HYPERGIANT
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A hypergiant (luminosity class 0, Ia-0 or Ia+) is a very rare type
Hypergiant
Class of massive star with a spectral type of A to K
A yellow hypergiant (YHG) is a massive star with an extended atmosphere, a spectral class from A to K, and, starting with an initial mass of about 20–60
Yellow_hypergiant
Stars with a supergiant luminosity class with a spectral type of K or M
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) Stars are classified as supergiants on the
Red_supergiant
American technology company
Hypergiant is an Austin, Texas based technology company, founded in February 2018, and currently headed by CEO Mike Betzer. The company develops artificial
Hypergiant_Industries
Star in the constellation Scutum
UY Scuti (BD-12°5055) is a red supergiant or hypergiant star, located 5,900 light-years away in the constellation Scutum. It is also a pulsating variable
UY_Scuti
Yellow hypergiant star in the constellation Cassiopeia
Rho Cassiopeiae is a yellow hypergiant star in the constellation Cassiopeia. Its name is a Bayer designation, pronounced /ˌroʊ kæsiəˈpiːaɪ, -sioʊ-, -iː/
Rho_Cassiopeiae
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 typically
List_of_nearest_hypergiants
Binary star in the constellation Dorado
from Earth. The primary component is an extreme red supergiant or red hypergiant that may be the largest known star with a well-defined radius, calculated
WOH_G64
Zheng, X. W.; Brunthaler, A. (2012). "The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry". Astronomy & Astrophysics. 544:
List_of_largest_stars
Star in the constellation Scutum
as Stephenson 2-18 , is a red supergiant (RSG) or possible extreme red hypergiant (RHG) star in the constellation of Scutum. It lies near the open cluster
Stephenson_2_DFK_1
American entrepreneur
SaaS conversational bot technology (acquired by LivePerson in 2018); and Hypergiant Industries, a machine-learning artificial intelligence (acquired by Trive
Ben_Lamm
Substellar object
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) Five different theories for the formation of
Brown_dwarf
Stellar classification
Hertzsprung–Russell diagram Solar analog Star count, survey of stars Yellow hypergiant "Glossary term: Luminosity Class". IAU Office of Astrononomy for Education
G-type_main-sequence_star
Constellation in the northern celestial hemisphere
luminous stars known, including the yellow hypergiants Rho Cassiopeiae and V509 Cassiopeiae and white hypergiant 6 Cassiopeiae. In 1572, Tycho Brahe's supernova
Cassiopeia_(constellation)
Star in the constellation Canis Major
VY Canis Majoris (abbreviated to VY CMa) is an extreme oxygen-rich red hypergiant or red supergiant (O-rich RHG or RSG) and pulsating variable star 1.2
VY_Canis_Majoris
Type of star that is luminous, blue, and variable in brightness
variables as a group in 1974. LBVs are massive unstable supergiant (or hypergiant) stars that show a variety of spectroscopic and photometric variation
Luminous_blue_variable
Star in the constellation Centaurus
red supergiant (RSG) or recent post-red supergiant (Post-RSG) yellow hypergiant (YHG), both of which suggest it is one of the largest known stars. The
HR_5171
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
Yellow hypergiant in the constellation Scorpius
IRAS 17163−3907, also known as Hen 3-1379, is a yellow hypergiant star located 13,000 light years from Earth in the constellation of Scorpius. The star
IRAS_17163−3907
Star at the centre of the Solar System
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Sun
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
M.; Zheng, X. W. (January 2012). "Distance and Kinematics of the Red Hypergiant VY CMa: VLBA and VLA Astrometry". The Astrophysical Journal. 744 (1):
List_of_supernova_candidates
Type of large cool star
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A red giant is a luminous giant star of low
Red_giant
Star within the open cluster Stephenson 2
Stephenson 2 DFK 49 or St2-11 is a putative post-red supergiant hypergiant star in the constellation Scutum, in the massive open cluster Stephenson 2.
Stephenson_2_DFK_49
Star that has a supergiant luminosity class, with a spectral type of F or G
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) Yellow supergiants generally have spectral
Yellow_supergiant
Type of star, larger and brighter than the Sun
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A giant star has a substantially larger radius
Giant_star
Red supergiant star in the constellation Cepheus
Mu Cephei is a red supergiant or hypergiant star in the northern constellation Cepheus. It is officially named the Garnet Star; Mu Cephei is its Bayer
Mu_Cephei
Topics referred to by the same term
the 15th variable star named in a constellation: RW Cephei, an orange hypergiant located in the constellation Cepheus RW Cygni, a red supergiant located
RW
Metalcore band from Tennessee
2025) Give Me a Reason (Clear Minded, 2014) Orthodox / Breaking Wheel (Hypergiant, 2015) "Hell" (2014) "I'm Scared of You" (2017) "The Anticipation" (2018)
Orthodox_(band)
Constellation in the southern celestial hemisphere
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 is a slow irregular variable, with
Carina_(constellation)
Star in the constellation Sagittarius
VX Sagittarii (abbreviated to VX Sgr) is an extreme red supergiant or hypergiant pulsating variable star with an unusually large magnitude range located
VX_Sagittarii
Comparison of a wide range of lengths
diameter of HR 5171 A, a yellow hypergiant star. 1.5 Tm – 10 au – estimated diameter of VV Cephei A, a red hypergiant with a blue dwarf companion. 1.75
Orders_of_magnitude_(length)
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Lists of stars by constellation
Lists_of_stars_by_constellation
Classification of stars based on spectral properties
distinguish giant stars from dwarfs. Luminosity class 0 or Ia+ is used for hypergiants, class I for supergiants, class II for bright giants, class III for regular
Stellar_classification
Star in the Triangulum Galaxy
B324 is a yellow hypergiant in the Triangulum Galaxy, located near the giant H II region IC 142 around 2.7 million light years away. It is the brightest
B324
Variable star in the constellation Cygnus
Located about 5,300 light-years (1,560 parsecs) from Earth, it is a hypergiant luminous blue variable (LBV) star of spectral type B1-2 Ia-0ep that is
P_Cygni
Musical artist
full-length albums and one EP as a solo musician. Gowe debuted with We are Hypergiants in 2012 as an independent musician. Later that year, he released the
Gowe_(musician)
Hypergiant star in Sagittarius
The Pistol Star (or V4647 Sagittarii) is an extremely luminous blue hypergiant star, one of the most luminous and massive known stars in the Milky Way
Pistol_Star
Type of star larger than main-sequence but smaller than a giant
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A subgiant is a star that is brighter than
Subgiant
Binary system in the constellation Eridanus
Mothra consists of two supergiant stars, a yellow supergiant or a yellow hypergiant, and a blue supergiant. As of 2025, the orbital characteristics of the
Mothra_(star)
Fabien; et al. (October 2024). "CHARA Near-infrared Imaging of the Yellow Hypergiant Star ρ Cassiopeiae: Convection Cells and Circumstellar Envelope". The
List of stars with resolved images
List_of_stars_with_resolved_images
Star in the constellation Carina
V382 Carinae, also known as x Carinae (x Car), is a yellow hypergiant in the constellation Carina. It is a G-type star with a mean apparent magnitude of
V382_Carinae
Methods for estimating the age of a star
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Stellar_age_estimation
Feature of the Hertzsprung-Russell diagram
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Hertzsprung_gap
Structure formed by diffuse material in orbital motion around a massive central body
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Accretion_disk
Star in the constellation Cygnus
NML Cygni or V1489 Cygni (abbreviated to NML Cyg or V1489 Cyg) is a red hypergiant or red supergiant (RHG or RSG) in the constellation Cygnus. It is one
NML_Cygni
Gas and dust surrounding a newly formed star
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Protoplanetary_disk
Super star cluster in the Milky Way Galaxy
large number of rare, evolved, high-mass stars, including: 6 yellow hypergiants, 4 red supergiants including Westerlund 1 W26, one of the largest known
Westerlund_1
Constellation in the northern celestial hemisphere
important class of star known as a Cepheid variable. RW Cephei, an orange hypergiant, together with the red supergiants Mu Cephei, MY Cephei, VV Cephei, V381
Cepheus_(constellation)
Hypergiant star in the constellation Aquila
IRC +10420, also known as V1302 Aquilae, is a yellow hypergiant star located in the constellation of Aquila at a distance of 4-6 kiloparsecs of the Sun
IRC_+10420
Constellation in the southern celestial hemisphere
0, and white spectroscopic binary Zeta (Furud), also at 3.0. The red hypergiant VY CMa is one of the largest stars known, while the neutron star RX J0720
Canis_Major
Large self-illuminated object in space
size and is determined by their surface gravity. These range from 0 (hypergiants) through III (giants) to V (main-sequence dwarfs); some authors add VII
Star
Hypergiant star in the constellation Cepheus
RW Cephei is a K-type hypergiant and a semirregular variable star in the constellation Cepheus, at the edge of the Sharpless 132 H II region and close
RW_Cephei
Planetary system consisting of the Sun and objects orbiting it
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Solar_System
Topics referred to by the same term
vintage, a type of Port wine Luminous blue variable, a very bright, blue, hypergiant variable star Libreville International Airport (IATA: LBV), in Libreville
LBV
Star in the constellation Sagittarius
HD 168625 (V4030 Sagittarii) is a blue hypergiant star and candidate luminous blue variable located in the constellation of Sagittarius easy to see with
HD_168625
Overview of the scientific field of astronomy
Supergiant Blue supergiant Red supergiant Yellow supergiant Hypergiant Yellow hypergiant Blue straggler Stellar classification O-type main-sequence star
Outline_of_astronomy
Hypothetical hybrid star type
−22° 13′ 26.6327″ Sagittarius 2021 Classified as red supergiant, red hypergiant, or a possible but unlikely super-AGB star V595 Cassiopeiae 01h 43m 02
Thorne–Żytkow_object
Molecular cloud in the constellation Canis Major
2362, which is located near the nebula, while another member, the red hypergiant VY Canis Majoris, is located near the nebula's rim. "Sh 2-310". "Sharpless
Sh_2-310
Hypothesized alternative to a black hole
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Gravastar
Type of star
is an asymptotic giant branch (AGB), a red supergiant (RSG), or a red hypergiant (RHG) star that shows strong OH maser emission and is unusually bright
OH/IR_star
Emission nebula in Sagittarius
generally assumed to be associated with it; its close neighbor, the blue hypergiant HD 168625, may be too. The Swan portion of M17, the Omega Nebula in the
Omega_Nebula
Star in the constellation Sagittarius
HD 168607 (V4029 Sagittarii) is a blue hypergiant and luminous blue variable (LBV) star located in the constellation of Sagittarius, easy to see with amateur
HD_168607
Astrophysical phenomenon
that most will be from iron core collapse in luminous supergiants or hypergiants (including LBVs). The narrow spectral lines for which they are named
Supernova
Light from the stars
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Starlight
Hot, giant star of early spectral type
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) In astronomy, a blue giant is a hot star with
Blue_giant
Theoretical stellar remnant
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Black_dwarf
Star in the constellation Dorado
HD 33579 is a white/yellow hypergiant and one of the brightest stars in the Large Magellanic Cloud (LMC). It is a suspected variable star. HD 33579 lies
HD_33579
Astronomical category of stars
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Iron_star
Star in the constellation Ara
(commonly abbreviated to W26) or Westerlund 1 BKS AS is a red supergiant or hypergiant (RSG or RHG) star located at the outskirts of the Westerlund 1 super star
Westerlund_1_W26
Astrophysical limit on radiation from stars
B. Stothers (2003). "Turbulent pressure in the envelopes of yellow hypergiants and luminous blue variables". Astrophysical Journal. 589 (2): 960–967
Eddington_luminosity
Type of interstellar cloud
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Molecular_cloud
Disappearing red supergiant star in the galaxy NGC 6946
constellation of Cygnus. The star, either a red supergiant or a yellow hypergiant, was 25 times the mass of the Sun, and was 20 million light years distant
N6946-BH1
Star in the constellation Centaurus
Omicron1 Centauri is a yellow hypergiant star in the southern constellation of Centaurus. Its name is a Bayer designation that is Latinized from ο1 Centauri
Omicron1_Centauri
Supernova at least ten times more luminous than a standard supernova
to the observed supernova event. Such stars are likely candidates of hypergiants or LBVs that appear to be undergoing substantial mass loss, due to Eddington
Superluminous_supernova
Collapsed core of a massive star
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Neutron_star
Star in the constellation Cassiopeia
PZ Cassiopeiae is a red supergiant or hypergiant star located in the constellation of Cassiopeia, and a semi-regular variable star. PZ Cassiopeiae is a
PZ_Cassiopeiae
Stellar classification distinguished by bright blue luminosity
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) A B-type main-sequence star is a main-sequence
B-type_main-sequence_star
Main-sequence star of spectral type O
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) An O-type main-sequence star is a main-sequence—core
O-type_main-sequence_star
Stars that have properties between Asymptotic Giant Branch stars and red supergiants
Karl M; Zheng, Xingwu; Wang, Guangli (2018). "The Parallax of the Red Hypergiant VX Sgr with Accurate Tropospheric Delay Calibration". The Astrophysical
Super-AGB_star
Star in the constellation Perseus
S Persei is a red supergiant or hypergiant located near the Double Cluster in Perseus, north of the cluster NGC 869. It is a member of the Perseus OB1
S_Persei
Cavity of hot gas blown from a star
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Stellar-wind_bubble
Supernova close enough to affect Earth's biosphere
the oceanic life on Earth. Multiple supernovae in a cluster of dying hypergiant stars that occurred in rapid succession on an astronomical and geological
Near-Earth_supernova
Astronomical objects colder than red dwarfs
Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants absolute magni- tude (MV) Before 2MASS there were only six known objects
L_dwarf
Star of relatively small size and low luminosity
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Dwarf_star
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
2.091 5,400 2023 A binary consisting of a yellow supergiant or yellow hypergiant and a Blue supergiant. MACS J1149 Lensed Star 1 (Icarus) 1.49 4,410 2018
List_of_most_distant_stars
Study of the movement of stars
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Stellar_kinematics
List of nearest giant stars List of nearest supergiants List of nearest hypergiants List of novae in the Milky Way galaxy List of novae in 2018 List of novae
Lists_of_astronomical_objects
Stage of stellar evolution
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Horizontal_branch
Star in the constellation Crux
hypergiant and a pulsar. BP Crucis is considered as the optical counterpart to the X-ray source GX 301−2. The system consists of a massive hypergiant
BP_Crucis
Astronomical objects of planetary size that did not form in orbit around a star
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Sub-brown_dwarf
Stage of stellar evolution
execute a blue loop and return to being a red supergiant. Extreme red hypergiants VY Canis Majoris and NML Cygni are two such known candidates for a star
Blue_loop
Hypothetical class of star that develops from a red dwarf
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Blue_dwarf_(red-dwarf_stage)
Star whose brightness fluctuates, as seen from Earth
(LBV) are among the most luminous stars known. Examples include the hypergiants η Carinae and P Cygni. They have permanent high mass loss, but at intervals
Variable_star
Topics referred to by the same term
brand of Carrefour Iran Hyper Star, the subsidiary operating in Iran Hypergiant, a kind of star with extremely high luminosity Hypervelocity star, a star
Hyperstar
Compact exotic star which forms matter consisting mostly of quarks
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Quark_star
System of two stars orbiting each other
Hertzsprung gap Giant Blue Red Yellow Bright giant Supergiant Blue Red Yellow Hypergiant Yellow Carbon S CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn
Binary_star
2006 hypernova in constellation Perseus
of a quark star. Eta Carinae (η Carinae or η Car) is a highly luminous hypergiant star located approximately 7,500 light-years from Earth in the Milky Way
SN_2006gy
Topics referred to by the same term
infrared catalogue IRC -10414, a red supergiant star IRC +10420, a yellow hypergiant star Incrementally related carriers, a standard for video channel frequencies
IRC_(disambiguation)
HYPERGIANT
HYPERGIANT
HYPERGIANT
HYPERGIANT
Girl/Female
American, Australian, British, English
Meadow of Ash Trees
Female
Egyptian
, the daughter of an early unknown king.
Girl/Female
Biblical
House of deepness.
Boy/Male
British, English
Place Name; The Awesome One's Meadow
Girl/Female
Indian
Sweet; Innocent; Pretty; Lovely
Girl/Female
Hindu
Boy/Male
Hindu, Indian
One who can Read Your Mind
Boy/Male
Arabic, Muslim
Lion Cub
Girl/Female
Indian
Rain, Constant flow
Girl/Female
Biblical
Hedges.
HYPERGIANT
HYPERGIANT
HYPERGIANT
HYPERGIANT
HYPERGIANT