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Longer titles found: Giant stargazer (view)

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69 Ceti (301 words) [view diff] exact match in snippet view article find links to article

naked eye with an apparent visual magnitude of 5.3. This is an aging red giant star with a stellar classification of M1/2III. It is radiating 1,813 times

HD 218061 is a class K4III (orange giant) star in the constellation Aquarius. Its apparent magnitude is 6.16 and it is approximately 650 light years away

(930 pc) away with slightly more mass than the Sun. Kepler-56 is a red giant star. This means it is no longer fusing hydrogen in its core and is off the

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IZ Aquarii is a red giant star in the constellation Aquarius. It is a slow irregular variable that varies between magnitudes 6.23 and 6.47.

HD 130084, also known as HR 5510, is a variable red giant star in the constellation Boötes. Located around 730 light-years distant, it shines with a luminosity

HD 20468 is a class K2II (orange bright giant) star in the constellation Perseus. Its apparent magnitude is 4.82 and it is approximately 1180 light years

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as the first inverted coaster in the Philippines. Star City hosts the Giant Star Wheel Ferris wheel. It has 32 air-conditioned gondolas, each seating up

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HD 189831 is a class K5III (orange giant) star in the constellation Sagittarius. Its apparent magnitude is 4.77 and it is approximately 366 light years

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HD 18970 is a class G9.5III (yellow giant) star in the constellation Perseus. Its apparent magnitude is 4.77 and it is approximately 211 light years away

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HD 167818 is a class K3II (orange bright giant) star in the constellation Sagittarius. Its apparent magnitude is 4.66 and it is approximately 760 light

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HD 190056 is a class K1III (orange giant) star in the constellation Sagittarius. Its apparent magnitude is 4.99 and it is approximately 291 light years

constellation of Hydra. Its apparent magnitude is 4.87. This is an aging red giant star on the asymptotic giant branch with a stellar classification of M1III:Ba0

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This giant-star-related article is a stub. You can help Wikipedia by expanding it.

This giant-star-related article is a stub. You can help Wikipedia by expanding it.

This giant-star-related article is a stub. You can help Wikipedia by expanding it.

This giant-star-related article is a stub. You can help Wikipedia by expanding it.

This giant-star-related article is a stub. You can help Wikipedia by expanding it.

This giant-star-related article is a stub. You can help Wikipedia by expanding it.

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HD 157662 is a bright giant star in the southern constellation of Ara. It has a magnitude 10.91 companion at an angular separation of 76.4″ along a position

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velocity of −5 km/s. With an age of 420 million years, this is a red giant star with a stellar classification of G8 III, indicating it has consumed the

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Earth; λ And is a yellow-hued giant star of type G8, 86 light-years from Earth; ο And is a blue-white hued giant star of type B6, 679 light-years from

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HD 51799 is a class M1III (red giant) star in the constellation Puppis. Its apparent magnitude is 4.95 and it is approximately 860 light years away based

approximately 610 light years away from Earth. It is a solitary red giant star of the spectral type M0III, meaning it possesses a surface temperature

BD+20 2457 is a 10th-magnitude K-type bright giant star located approximately 4,800 light-years away in the constellation of Leo. The name refers to the

HD 63922 is a class B0III (blue giant) star in the constellation Puppis. Its apparent magnitude is 4.11 and it is approximately 1600 light years away

HD 63744 is a class K0III (orange giant) star in the constellation Puppis. Its apparent magnitude is 4.71 and it is approximately 232 light years away

186-day period planet orbits about 83% the Earth-Sun distance from the giant star 14 Andromedae. It has a minimum mass 4.8 times the mass of Jupiter. The

constellation of Andromeda. It is classified as a semiregular variable pulsating giant star, and varies from an apparent visual magnitude of 11.5 at minimum brightness

drifting closer with a radial velocity of −23 km/s. This is an aging red giant star with a stellar classification of M5III. It has an estimated 3.1 times

constellation Lyra, approximately 700 light years away from Earth. It is a red giant star of the spectral type M2III, meaning it possesses a surface temperature

drifting closer with a radial velocity of −64.4 km/s. This is an aging red giant star with a stellar classification of M1IIIab, It is currently on the asymptotic

Star Catalogue has this star classified as M0III, matching an aging red giant star that has consumed the hydrogen at its core and expanded. Houk and Swift

NGC 2423-3 is a red giant star approximately 3,040 light-years away in the constellation of Puppis. The star is part of the NGC 2423 open cluster (hence

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177 ly of the Sun around 6.3 million years ago. This is an evolved red giant star with a stellar classification of M2 IIIa. It is a semiregular variable

with a radial velocity of +13.3 km/s. This object is an aging bright giant star with a stellar classification of G6IIb With the supply of hydrogen at

spectral type F2V-IV, previous analyses have stated that the star is a G8III giant star and an F0V main-sequence star. Located in the constellation Cetus, the

variable, but there has not been any proof of binarity, yet. It is a red giant star with a spectral classification of K1III. OP Andromedae is one of the few

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Niedzielski et al. using the Hobby-Eberly Telescope. It orbits the K3 giant star HD 240210 in the constellation of Cassiopeia. Its average orbital separation

is less dense and rich. The brightest star of the cluster is a K5 III giant star, with 7.1 magnitude, but its membership is questionable. One more 7.9

structure, made up of gas and dust, reflecting light of the central red giant star HR 3126. This is rarely seen because the end-of-life phase of this type

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This giant-star-related article is a stub. You can help Wikipedia by expanding it.

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14 Aquarii (abbreviated 14 Aqr) is red giant star. 14 Aquarii is the Flamsteed designation; it also bears the variable star designation IW Aquarii. It

parsecs (317 lys) from the Sun. The 198-day period planet orbits the yellow giant star HD 104985 (Tonatiuh) at a distance of 0.78 AU. With a mass 61/3 times

HD 4732 is a red giant star of magnitude 5.9 located in the constellation Cetus. It is 189 light years from the Solar System. HD 4732 is located in the

massive stars that are forming at a rate similar to the most vigorous giant star-forming regions in our own Milky Way. Arp 302 is 450 million light-years

with a heliocentric radial velocity of −22 km/s. This is an aging red giant star with a stellar classification of K3 III CN2, a star that has used up its

with a heliocentric radial velocity of +19 km/s. This is an aging red giant star with a stellar classification of M2.5 III, which indicates it has exhausted

north and 60″.8 east of the galactic nucleus. The progenitor was a red giant star with 8.5–16.5 times the mass of the Sun. NGC 4030 imaged by the Hubble

constellation of Aquila. The planet was discovered orbiting the yellow giant star Xi Aquilae in 2008. The planet has a minimum mass of 2.8 Jupiter and a

with a heliocentric radial velocity of +19 km/s. This is an aging red giant star with a stellar classification of M2.5 III, which indicates it has exhausted

heliocentric radial velocity of −1.1 km/s. The visible component is an aging red giant star with a stellar classification of M0 III, which indicates it has consumed

Microscopii is a star in the constellation Microscopium. It is a red giant star of spectral type M3e-M5.5 that is also a Mira variable, with an apparent

pp. 891, 895. This DA-class white dwarf is the surviving core of a red giant star that ceased nuclear fusion while shedding its outer envelope. It has a

member of the Hyades Supercluster. The visible component is an aging red giant star on the asymptotic giant branch with a stellar classification of M1III

spectroscopic binary pairs. The first pair is made of a primary yellow giant star of spectral type G0III, and the secondary subgiant star of spectral type

spectroscopic binary pairs. The first pair is made of a primary yellow giant star of spectral type G0III, and the secondary subgiant star of spectral type

with a heliocentric radial velocity of −56 km/s. This is an aging red giant star on the asymptotic giant branch with a stellar classification of M2.5III

every 1,682 seconds and displays a strong magnetic field. The evolved red giant star is losing mass, since radiation pressure overcomes the low gravity on

Microscopii is a star in the constellation Microscopium. It is a red giant star of spectral type M4e that is also a Mira variable, with an apparent magnitude

cluster as the result of a binary–binary interaction. This is a blue giant star with a stellar classification of B2 III;, a massive star that has evolved

NGC 4349-127 is a probable red giant star approximately 6,100 light-years away in the constellation of Crux. It is a member of the open cluster NGC 4349

−3 km/s. It has an absolute magnitude of −1.51. This is an aging bright giant star with a stellar classification of G0II. It is a candidate Cepheid variable

with a heliocentric radial velocity of −1.5 km/s. This is an evolved red giant star with a stellar classification of M0.5 III, currently on the asymptotic

with a heliocentric radial velocity of −19 km/s. This is an aging red giant star on the asymptotic giant branch with a stellar classification of M3-SIII

30 Cygni (ο1 Cygni) is a class A5III (white giant) star in the constellation Cygnus. Its apparent magnitude is 4.83 and it is approximately 610 light

Moving Group but has since been excluded. This object is an aging red giant star on the asymptotic giant branch with a stellar classification of M3/4III

located roughly 480 light years from the Sun. This is an evolved red giant star with a stellar classification of M1 III, and is currently on the asymptotic

star with an apparent visual magnitude of 4.97. This is an aging red giant star on the asymptotic giant branch with a stellar classification of M3−III

prominent. The bright red/orange star near the center is HIP 32406, a giant star of spectral type K2, about 1500 ly away of magnitude 6.9. Center 2MASS/NASA

around 166 light-years distant. 39 Arietis (Lilii Borea) is an orange giant star of magnitude 4.51 and spectral type K1.5III that is around 171 light-years

magnitude of 10.7. The brighter magnitude 5.18 primary is an aging red giant star with a stellar classification of M1IIIab. Having exhausted the supply

ecliptic, it is subject to lunar eclipses. This object is an aging red giant star currently on the asymptotic giant branch with a stellar classification

heliocentric radial velocity of −8 km/s. The primary component is an ageing red giant star with a stellar classification of M2.5 III Ba0.5. The suffix notation indicates

star is a member of the HR 1614 supercluster. This is an evolved red giant star with a stellar classification of M5 III. It is classified as a semiregular

HD 65750, also known as V341 Carinae is a bright red giant star in the constellation Carina. It is surrounded by a prominent reflection nebula, known as

V723 Monocerotis is an eighth-magnitude ellipsoidal variable yellow giant star roughly the mass of the Sun, but 25 times its radius. The accompanying

of this star matches a stellar classification of M1 III. It is a red giant star with 54 times the radius of the Sun that is currently on the asymptotic

31 Comae Berenices (31 Com) is a yellow giant star in the constellation Coma Berenices. Its apparent magnitude is about 4.9 and slightly variable. It is

Aldebaran b is a candidate exoplanet orbiting the orange giant star Aldebaran, 65 light-years away. It was initially detected in 1993, but was considered

with an estimated period of 2,500 days. The primary component is a red giant star with a stellar classification of M1.5 III. The outer envelope of this

TX Piscium (19 Piscium) is a variable red giant star in the constellation Pisces. It is amongst the reddest naked eye stars, with a significant reddish

ultraviolet pulse. The companion star that was hit is suspected to be a red giant star.[citation needed] This detection of the UV signal represents the first

31 Comae Berenices (31 Com) is a yellow giant star in the constellation Coma Berenices. Its apparent magnitude is about 4.9 and slightly variable. It is

with an estimated period of 2,500 days. The primary component is a red giant star with a stellar classification of M1.5 III. The outer envelope of this

the Pleiades group of co-moving stars. This object is a massive bright giant star with a stellar classification of B5 II. It is 25 million years old and

naked eye with an apparent visual magnitude of about 5. This is a red giant star with a spectral classification of M3 III. The interferometry-measured

Aldebaran b is a candidate exoplanet orbiting the orange giant star Aldebaran, 65 light-years away. It was initially detected in 1993, but was considered

Electra /əˈlɛktrə/, designated 17 Tauri, is a blue-white giant star in the constellation of Taurus located approximately 400 light years away. It is the

63 Ophiuchi is an O-type giant star in the constellation Sagittarius, despite its name. During a 2009 survey for companions of massive stars, it was observed

northern constellation of Auriga, about 1,050 light years away. It is a red giant star with a stellar classification of M2III, and has expanded away from the

with a heliocentric radial velocity of −20 km/s. This is an ageing red giant star, currently on the asymptotic giant branch, with a stellar classification

member of the massive, possible open cluster Trumpler-27, where a blue giant star, a yellow supergiant star, and two Wolf–Rayet stars are also located.

in the constellation Cygnus, less than 4' from θ Cygni. This is a red giant star on the asymptotic giant branch located around 2,200 light years away.

component A, has a stellar classification of B5 III, matching an evolved blue giant star. It has 5.85 times the mass of the Sun and is radiating 1,105 times the

Association of co-moving stars. The visible component is an aging bright giant star with a stellar classification of B8/9II. The spectrum of the star displays

closer with a radial velocity of −38 km/s. This object is an aging red giant star with a stellar classification of M0.5III. After exhausting the supply

member of the massive, possible open cluster Trumpler-27, where a blue giant star, a yellow supergiant star, and two Wolf–Rayet stars are also located.

heliocentric radial velocity of −33 km/s. The visible component is an aging red giant star, currently on the asymptotic giant branch, with a stellar classification

as close as 204 ly in around 4.3 million years. This is an evolved red giant star with a stellar classification of M1 III, currently on the asymptotic giant

degenerate star (not including lifetime as main sequence star and as giant star) is 3.97 Gyr. Due almost equal to the Sun's temperature, GJ 1087 should

star. The primary (α2 Cap), 109 light-years from Earth, is a yellow-hued giant star of magnitude 3.6; the secondary (α1 Cap), 690 light-years from Earth,

further away with a radial velocity of +38 km/s. This is an evolved red giant star with a stellar classification of M0 III. It is a suspected variable star

as close as 204 ly in around 4.3 million years. This is an evolved red giant star with a stellar classification of M1 III, currently on the asymptotic giant

PU Puppis (PU Pup) is a class B8III (blue giant) star in the constellation Puppis. Its apparent magnitude is 4.69 and it is approximately 620 light years

HD 122563 is an extremely metal-poor red giant star, and the brightest metal-poor star in the sky. Its low heavy element content was first recognized by

approximately 4.39 at maximum brightness. Its primary is a G-type bright giant star and its secondary is an A-type main-sequence star. It is approximately

caused by interstellar gas and dust. Pi Aurigae is an evolved bright giant star with a stellar classification of M3 II. After exhausting the supply of

This giant-star-related article is a stub. You can help Wikipedia by expanding it.

by speckle interferometry. The primary component is an evolved bright giant star with a stellar classification of G5II. It has four times the mass of the

98 km/s. Currently on the asymptotic giant branch, this is an evolved red giant star with a stellar classification of M1+III Fe-1. The suffix notation indicates

the north of Senegal where Belel was located. HD 181342 is a K-type red giant star with a stellar classification of K0 III. It was formerly an A-type main-sequence

caused by interstellar gas and dust. Pi Aurigae is an evolved bright giant star with a stellar classification of M3 II. After exhausting the supply of

with a radial velocity of +28 km/s. The main component is an aging red giant star on the asymptotic giant branch with a stellar classification of M6/7pe

318 light years from the Sun based on parallax. This is an orange-hued red giant star with a stellar classification of K5 III. After exhausting the supply of

to 4.23m. Its companion, CS Camelopardalis B, is a magnitude 8.7m blue giant star located 2.4 arcseconds from the primary. Vallenari, A.; et al. (Gaia collaboration)

with a heliocentric radial velocity of +5.6 km/s. This is an aging red giant star with a stellar classification of M3− III, which indicates it has exhausted

type of M0Ia. Stars #28 and #105 are Wolf-Rayet stars. Star #27, a blue giant star with a spectral type of O8III((f)), may be one of the most luminous stars

drifting closer with a radial velocity of −14 km/s. This is an aging red giant star on the asymptotic giant branch with a stellar classification of M1.5III

Rho2 Arietis is an M-type red giant star in the northern constellation of Aries. With an annual parallax shift of 9.28 mas, it is approximately 350 light-years

with a heliocentric radial velocity of −1.2 km/s. This is an aging red giant star on the asymptotic giant branch with a stellar classification of M3 III

years. Estimated to be around 10 billion years old, this is an aging red giant star with a stellar classification of M3.5 III. It is a periodic variable with

small hot star (white dwarf or main sequence star) orbits around a red giant star. These systems are often surrounded by an envelope of gas or dust; those

light-years (27.2 parsecs) from the Sun. It is the nearest M-type red giant star to the Sun. γ Crucis (Latinised to Gamma Crucis) is the star's Bayer designation

radial velocity of −12 km/s. This object is a highly luminous bright giant star with a stellar classification of F5II. It has five times the mass of the

with a heliocentric radial velocity of −16 km/s. This is an aging bright giant star with a stellar classification of K2.5IIb, having exhausted the supply

English: the Fourth Star of Sickle.) Upsilon Ceti is an evolved red giant star with a stellar classification of M0III and is listed as a standard for

distance to this star is roughly 680 light-years. This is an evolved red giant star with a stellar classification of M1 III. It is a suspected variable star

with a radial velocity of +17 km/s. This is an aging, massive bright giant star with a stellar classification of A5 II. It is an estimated 30 million