List of stars in Ursa Minor
Encyclopedia
This is the list of notable star
Star
A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...

s in the constellation
Constellation
In modern astronomy, a constellation is an internationally defined area of the celestial sphere. These areas are grouped around asterisms, patterns formed by prominent stars within apparent proximity to one another on Earth's night sky....

 Ursa Minor
Ursa Minor
Ursa Minor , also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, whence the name Little Dipper...

, sorted by decreasing brightness.
Name B
Bayer designation
A Bayer designation is a stellar designation in which a specific star is identified by a Greek letter, followed by the genitive form of its parent constellation's Latin name...

F
Flamsteed designation
Flamsteed designations for stars are similar to Bayer designations, except that they use numbers instead of Greek letters. Each star is assigned a number and the Latin genitive of the constellation it lies in...

HD
Henry Draper Catalogue
The Henry Draper Catalogue is an astronomical star catalogue published between 1918 and 1924, giving spectroscopic classifications for 225,300 stars; it was later expanded by the Henry Draper Extension , published between 1925 and 1936, which gave classifications for 46,850 more stars, and by the...

HIP RA
Right ascension
Right ascension is the astronomical term for one of the two coordinates of a point on the celestial sphere when using the equatorial coordinate system. The other coordinate is the declination.-Explanation:...

Dec
Declination
In astronomy, declination is one of the two coordinates of the equatorial coordinate system, the other being either right ascension or hour angle. Declination in astronomy is comparable to geographic latitude, but projected onto the celestial sphere. Declination is measured in degrees north and...

vis.
mag.
Apparent magnitude
The apparent magnitude of a celestial body is a measure of its brightness as seen by an observer on Earth, adjusted to the value it would have in the absence of the atmosphere...

abs.
mag.
Absolute magnitude
Absolute magnitude is the measure of a celestial object's intrinsic brightness. it is also the apparent magnitude a star would have if it were 32.6 light years away from Earth...

Dist. (ly) Sp. class
Stellar classification
In astronomy, stellar classification is a classification of stars based on their spectral characteristics. The spectral class of a star is a designated class of a star describing the ionization of its chromosphere, what atomic excitations are most prominent in the light, giving an objective measure...

Notes
Polaris
Polaris
Polaris |Alpha]] Ursae Minoris, commonly North Star or Pole Star, also Lodestar) is the brightest star in the constellation Ursa Minor. It is very close to the north celestial pole, making it the current northern pole star....

 
α 1 8890 11767 1.97 −3.64 431 F7:Ib-IIv SB Pole Star
Pole star
The term "Pole Star" usually refers to Polaris, which is the current northern pole star, also known as the North Star.In general, however, a pole star is a visible star, especially a prominent one, that is approximately aligned with the Earth's axis of rotation; that is, a star whose apparent...

, Lodestar
Lodestar
A lodestar or guiding star may be:*Polaris*any star used in celestial navigation*metaphorically, any guiding principle*Guiding Star...

, Alruccabah, Cynosura
Cynosura
In Greek mythology, Cynosura was a nymph on Mount Ida, Crete. Cynosura nursed Zeus when he was being hidden from his father, Cronus. In gratitude, Zeus placed her in the heavens as the constellation Ursa Minor; according to folk etymology and the myth, Kynosoura is from κυνὸς οὐρά "dog's tail...

, Phoenice
Phoenice
Phoenice or Phoenike was an ancient Greek city in Epirus and capital of the Chaonians. It was also the location of the Treaty of Phoenice which ended the First Macedonian War, as well as one of the wealthiest cities in Epirus until the Roman conquest. During the early Byzantine period, Phoenice...

, Tramontana
Tramontana
Tramontana or Tramontane can refer to:*Tramontane, a northern wind *the Pole Star*Tramontane, a science fiction novel by Emil Petaja...

, Angel Stern, Navigatoria, Star of Arcady, Yilduz, Mismar, Polyarnaya; Cepheid variable
Cepheid variable
A Cepheid is a member of a class of very luminous variable stars. The strong direct relationship between a Cepheid variable's luminosity and pulsation period, secures for Cepheids their status as important standard candles for establishing the Galactic and extragalactic distance scales.Cepheid...

; Dhruva
Dhruva
In the Hindu mythology, Dhruva is a devotee of the god Vishnu, who blessed to attain the position of the polar star, also known as Dhruva in Sanskrit. Dhruva was the son of Uttānapāda...

β UMi
Beta Ursae Minoris
Beta Ursae Minoris is the second brightest star in the bowl of the "Little Dipper,"the constellation Ursa Minor. It has the traditional name Kochab. Kochab's magnitude is 2.07. It is 16 degrees from Polaris. The star is an orange giant and is 126.4 ± 2.5 light years from Earth. It is 130 times...

 
β 7 131873 72607 2.07 −0.87 126 K4IIIvar Kochab, Kokab, Kochah
γ UMi
Gamma Ursae Minoris
Gamma Ursae Minoris is a slightly variable star in the constellation Ursa Minor. It also has the common name Pherkad. Together with Beta Ursae Minoris, Gamma forms the end of the dipper pan of the "Little Dipper"...

 
γ 13 137422 75097 3.00 −2.84 480 A3II-III Pherkad, Pherkad Major; δ Sct variable
Delta Scuti variable
A Delta Scuti variable is a variable star which exhibits variations in its luminosity due to both radial and non-radial pulsations of the star's surface. Typical brightness fluctuations are from 0.003 to 0.9 magnitudes in V over a period of a few hours, although the amplitude and period of the...

ε UMi
Epsilon Ursae Minoris
Epsilon Ursae Minoris is a triple star system in the constellation Ursa Minor. It is approximately 347 light years from Earth....

 
ε 22 153751 82080 4.21 −0.92 346 G5IIIvar Urodelus; RS CVn variable
RS Canum Venaticorum variable
RS Canum Venaticorum variables are a type of variable star. They are close binary stars having active chromospheres which can cause large stellar spots. These spots are believed to cause variations in their observed luminosity...

5 UMi  5 127700 70692 4.25 −0.87 345 K4III
ζ UMi
Zeta Ursae Minoris
Zeta Ursae Minoris is a star in the constellation Ursa Minor. It has the traditional name Akhfa al Farkadain, from the Arabic أخفى الفرقدين aḫfa al-farqadayn "the dimmer of the two calves", as opposed to Anwar al Farkadain "the brighter of the two calves"...

 
ζ 16 142105 77055 4.29 −1.02 376 A3Vn Ahfa al Farkadain
δ UMi
Delta Ursae Minoris
Delta Ursae Minoris is a star in the constellation Ursa Minor. It has the traditional name Yildun , from the Turkish yıldız "star"...

 
δ 23 166205 85822 4.35 0.61 183 A1Vn Yildun, Gildun, Vildiur, Yilduz, Pherkard
RR UMi  132813 73199 4.63 −0.80 398 M5III variable star
Variable star
A star is classified as variable if its apparent magnitude as seen from Earth changes over time, whether the changes are due to variations in the star's actual luminosity, or to variations in the amount of the star's light that is blocked from reaching Earth...

4 UMi  4 124547 69112 4.80 −1.13 500 K3III
η UMi
Eta Ursae Minoris
Eta Ursae Minoris is a star in the constellation Ursa Minor. It has the traditional names Anwar al Farkadain and Alasco...

 
η 21 148048 79822 4.95 2.58 97 F5V Anwar al Farkadain, Alasco
θ UMi
Theta Ursae Minoris
Theta Ursae Minoris is a star in the constellation Ursa Minor.Theta Ursae Minoris is an orange K-type giant with an apparent magnitude of +5.00. It is approximately 830 light years from Earth....

 
θ 15 139669 76008 5.00 −2.03 832 K5III
11 UMi
11 Ursae Minoris
11 Ursae Minoris or 11 UMi is a 5th magnitude K-type giant star located approximately 398 light years away in the constellation Ursa Minor. It is sometimes named Pherkard or Pherkad Minor, the later name to distinguish it from Pherkad which is Gamma Ursae Minoris...

 
11 136726 74793 5.02 −0.37 389 K4III Pherkad Minor; has a planet
Extrasolar planet
An extrasolar planet, or exoplanet, is a planet outside the Solar System. A total of such planets have been identified as of . It is now known that a substantial fraction of stars have planets, including perhaps half of all Sun-like stars...

 (b
11 Ursae Minoris b
11 Ursae Minoris b is an extrasolar planet which orbits the K-type giant star 11 Ursae Minoris, located approximately 390 light years away in the constellation Ursa Minor. This planet has mass 10.5 MJ. However, since the mass is at lower limit and since inclination is not known, the actual mass is...

)
136064 74605 5.15 3.13 83 F9IV
124730 69373 5.18 −0.50 445 M2III
19 UMi  19 146926 79280 5.48 −1.07 665 B8V
118904 66435 5.50 0.05 400 K2III
149681 80480 5.55 2.42 138 F0V
133002 72573 5.63 2.45 141 F9V
140227 76519 5.65 −1.51 881 M0III
145622 78661 5.73 −0.53 581 A3V
158996 84769 5.74 −1.67 991 K5III
24 UMi  24 166926 85699 5.78 2.38 156 A2m
117187 65536 5.82 −1.63 1009 M1III
120084 66903 5.91 0.96 318 G7III:
152303 81854 5.99 3.21 117 F4V
147321 79601 6.02 −0.78 748 A3V
HD 155154 VX UMi 155154 83317 6.17 2.91 146 F0IVn γ Doradus variable
Gamma Doradus variable
Gamma Doradus variables are variable stars which display variations in luminosity due to non-radial pulsations of their surface. The stars are typically young, early F or late A type main sequence stars, and typical brightness fluctuations are 0.1 magnitudes with periods on the order of one day...

135384 74272 6.18 0.23 504 A8Vn
133994 73706 6.22 0.45 464 A2Vs
UY UMi 107192 59767 6.27 2.93 152 F2V γ Doradus variable
129245 71196 6.27 0.52 461 K3III
λ UMi
Lambda Ursae Minoris
Lambda Ursae Minoris is a star in the constellation Ursa Minor.Lambda Ursae Minoris is a M-type red giant with a mean apparent magnitude of +6.31. It is classified as a semiregular variable star and its brightness varies by 0.10 magnitudes. It is approximately 888 light years from Earth....

 
λ 183030 84535 6.31 −0.84 876 M1III
107113 59879 6.33 3.34 129 F4V
151623 81428 6.33 0.81 414 G9III
150275 80850 6.35 0.87 408 K1III
20 UMi  20 147142 79420 6.36 −0.49 765 K2IV
113889 63822 6.43 1.01 396 F0V
3 UMi  3 124063 68956 6.43 0.79 438 A7V
5914 7283 6.46 1.49 321 A3V
π1 UMi A
Pi Ursae Minoris
The Bayer designation Pi Ursae Minoris is shared by two star systems, π¹ Ursae Minoris and π² Ursae Minoris, in the constellation Ursa Minor. They are separated by 0.64° on the sky.-π¹ Ursae Minoris:...

 
π1 139777 75809 6.57 4.85 72 G8IV-V+...
9 UMi  9 133621 73440 6.64 4.00 110 G0
8 UMi  8 133086 73136 6.83 0.95 489 K0
π2 UMi
Pi Ursae Minoris
The Bayer designation Pi Ursae Minoris is shared by two star systems, π¹ Ursae Minoris and π² Ursae Minoris, in the constellation Ursa Minor. They are separated by 0.64° on the sky.-π¹ Ursae Minoris:...

 
π2 18 141652 76695 6.89 1.54 384 F2
HD 150706
HD 150706
HD 150706 is a 7th magnitude star in the constellation of Ursa Minor. It is a remarkably Sun-like yellow dwarf being only 2% less massive than the Sun....

 
150706 80902 7.03 4.85 89 G0 has an unconfirmed planet
π1 UMi B
Pi Ursae Minoris
The Bayer designation Pi Ursae Minoris is shared by two star systems, π¹ Ursae Minoris and π² Ursae Minoris, in the constellation Ursa Minor. They are separated by 0.64° on the sky.-π¹ Ursae Minoris:...

 
π1 139813 75829 7.30 5.62 71 G5
14 UMi  14 137686 75152 7.38 3.51 194 F5
Calvera
Calvera (neutron star)
Calvera is the nickname of an X-ray source known as 1RXS J141256.0+792204in the ROSAT All-Sky Survey Bright Source Catalog . It lies in the constellation Ursa Minor and is identified as an isolated neutron star.-References:...

 
625 X Neutron star
Neutron star
A neutron star is a type of stellar remnant that can result from the gravitational collapse of a massive star during a Type II, Type Ib or Type Ic supernova event. Such stars are composed almost entirely of neutrons, which are subatomic particles without electrical charge and with a slightly larger...


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