A light curve for Lambda Ursae Minoris, plotted from Hipparcos data[1]
Observation data Epoch J2000.0 Equinox J2000.0
Constellation
Ursa Minor
Right ascension
17h 16m 56.4107s[2]
Declination
+89° 02′ 15.734″[2]
Apparent magnitude (V)
+6.38[3]
Characteristics
Spectral type
M3+ IIIa[4]
U−B color index
+1.79[5]
B−V color index
+1.57[5]
Variable type
SRb[6]
Astrometry
Radial velocity (Rv)
+0.19[2] km/s
Proper motion (μ)
RA: −23.989[2] mas/yr Dec.: 3.463[2] mas/yr
Parallax (π)
3.7084 ± 0.1329 mas[2]
Distance
880 ± 30 ly (270 ± 10 pc)
Absolute magnitude (MV)
−0.85[7]
Details
Radius
64[2]R☉
Luminosity
741[2]L☉
Temperature
3,772[2] K
Other designations
HR 7394, HD 183030, BD+88°112, FK5 914, HIP 84535, SAO 3020
Database references
SIMBAD
data
Lambda Ursae Minoris (λ UMi, λ Ursae Minoris) is a star in the constellation Ursa Minor. It is an M-type red giant with an apparent magnitude of +6.38 and is approximately 880 light years from Earth.
Lambda Ursae Minoris is an asymptotic giant branch (AGB) star, a star that has exhausted its core hydrogen and helium and is now fusing material in shells outside its core.[8] AGB stars are often unstable and tend to pulsate, and Lambda Ursae Minoris is classified as a semiregular variable star and its brightness varies by about 0.1 magnitudes.[6] Its variability was discovered from Hipparcos astrometry and it was entered into the General Catalogue of Variable Stars in 1999.[9]
This star was used from 1882 as a reference to measure the magnitudes of stars in the northern hemisphere for the 1908 Revised Harvard Photometry catalogue. Sigma Octantis was used for the southern hemisphere. It was then noted that "Neither of these stars appears to vary perceptibly" but that, due to the procedures used "if they did, the variation would have no effect on the final measures."[10]
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and 14 Related for: Lambda Ursae Minoris information
the night sky, ranging in apparent magnitude from 1.97 to 2.00. Beta UrsaeMinoris, also known as Kochab, is an aging star that has swollen and cooled...
the 1908 Revised Harvard Photometry catalogue. The Pole Star and LambdaUrsaeMinoris were used for the northern hemisphere. It was then noted that "Neither...
around 1700 BC until just after 300 AD, Kochab (Beta UrsaeMinoris) and Pherkad (Gamma UrsaeMinoris) were twin northern pole stars, though neither was...
considered the pole star until about 1800 BC, when the much brighter Beta UrsaeMinoris (Kochab) began to approach the pole as well. Having gradually drifted...
Sigma Sagittarii Star 2.07 Alpha Ophiuchi Binary star system 2.08 Beta UrsaeMinoris Star 2.10 Gamma Andromedae Quadruple star system 2.11 2.0 Beta Gruis...
Puppis Azmidi Alternatively rendered Asmidiske. /ˈæzmᵻdi/ Ursa Minor 8 UrsaeMinoris Baekdu IAU new 2019 South Korean proposal; named after the highest mountain...
with a period of 547,000 (+66,000/-40,000) years. Polaris or Alpha UrsaeMinoris (α UMi), the north star, is a triple star system in which the closer...
values as of 2015: H0=67.74 and OmegaM=0.3089 (see Table/Planck2015 at "Lambda-CDM model#Parameters" ) Staff (2018). "UCLA Cosmological Calculator". UCLA...
(1999-06-01). "Masses and Other Parameters of the Post-Common Envelope Binary BE Ursae Majoris". The Astrophysical Journal. 518 (2): 866–872. Bibcode:1999ApJ....