2 Ursae Minoris

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search

Template:Short description

2 Ursae Minoris
Observation data
Epoch J2000      Equinox J2000
Constellation Cepheus[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 4.244[3]
Characteristics
Spectral type K2 II-III[4]
B−V Template:Engvar Script error: No such module "val".[1]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: Script error: No such module "val".[2] mas/yr
Dec.: Script error: No such module "val".[2] mas/yr
Parallax (π)11.64±0.15 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.43[1]
Details
MassScript error: No such module "val".[6] Template:Solar mass
RadiusScript error: No such module "val".[5] Template:Solar radius
LuminosityScript error: No such module "val".[5] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[3] cgs
TemperatureScript error: No such module "val".[5] K
Metallicity [Fe/H]Script error: No such module "val".[3] dex
Rotational velocity (v sin i)1.0[7] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

Script error: No such module "Check for unknown parameters".

2 Ursae Minoris (2 UMi) is a single[9] star a few degrees away from the northern celestial pole. Despite its Flamsteed designation, the star is actually located in the constellation Cepheus. This change occurred when the constellation boundaries were formally set in 1930 by Eugene Delporte. Therefore, the star is usually referred only by its catalog numbers such as HR 285 or HD 5848. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.244.[3] This object is located 280 light years away and is moving further from the Earth with a heliocentric radial velocity of +8 km/s.[5] It is a candidate member of the Hyades Supercluster.[3]

This is an aging K-type star with a stellar classification of K2 II-III,[4] showing a luminosity class with blended traits of a giant and a bright giant. It has 2.3[6] times the mass of the Sun and has expanded to 24[5] times the Sun's radius. The star is radiating around 215[5] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,513 K.[5]

References

<templatestyles src="Reflist/styles.css" />

  1. a b c Template:Cite XHIP
  2. a b c d e Script error: No such module "citation/CS1".
  3. a b c d e Script error: No such module "citation/CS1".
  4. a b Script error: No such module "citation/CS1".
  5. a b c d e f g h Template:Cite DR2
  6. a b Script error: No such module "citation/CS1".
  7. Script error: No such module "citation/CS1".
  8. Template:Cite simbad
  9. Script error: No such module "citation/CS1".

Script error: No such module "Check for unknown parameters".

External links

Template:Stars of Cepheus