| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Ursa Major [1] |
| 23 UMa A | |
| Right ascension | 09h 31m 31.70873s [2] |
| Declination | +63° 03′ 42.7013″ [2] |
| Apparent magnitude (V) | +3.65 [1] |
| 23 UMa B | |
| Right ascension | 09h 31m 28.36401s [3] |
| Declination | +63° 03′ 41.8990″ [3] |
| Apparent magnitude (V) | +9.19 [4] |
| Characteristics | |
| 23 UMa A | |
| Evolutionary stage | main sequence [5] |
| Spectral type | F0IV [6] |
| B−V color index | 0.360±0.015 [1] |
| 23 UMa B | |
| Evolutionary stage | main sequence [4] |
| Spectral type | K5V [7] |
| Astrometry | |
| 23 UMa A | |
| Radial velocity (Rv) | −10.4±0.7 [1] km/s |
| Proper motion (μ) | RA: +107.99 [2] mas/yr Dec.: +27.15 [2] mas/yr |
| Parallax (π) | 41.99±0.16 mas [2] |
| Distance | 77.7 ± 0.3 ly (23.82 ± 0.09 pc) |
| Absolute magnitude (MV) | +1.77 [1] |
| 23 UMa B | |
| Radial velocity (Rv) | −2.55±0.13 [3] km/s |
| Proper motion (μ) | RA: +108.861 [3] mas/yr Dec.: +13.972 [3] mas/yr |
| Parallax (π) | 42.2161±0.0166 mas [3] |
| Distance | 77.26 ± 0.03 ly (23.688 ± 0.009 pc) |
| Details | |
| 23 UMa A | |
| Mass | 1.44 [8] M☉ |
| Radius | 2.84 [8] R☉ |
| Luminosity | 15.1 [8] L☉ |
| Surface gravity (log g) | 3.69 [8] cgs |
| Temperature | 6,748 [8] K |
| Metallicity [Fe/H] | 0.17 [6] dex |
| Rotational velocity (v sin i) | 154 [5] km/s |
| Age | 1.3 [6] Gyr |
| 23 UMa B | |
| Mass | 0.69 [8] M☉ |
| Radius | 0.68 [8] R☉ |
| Luminosity | 0.16 [8] L☉ |
| Surface gravity (log g) | 4.61 [8] cgs |
| Temperature | 4,436 [8] K |
| Metallicity [Fe/H] | 0.06 [9] dex |
| Other designations | |
| h UMa, 23 UMa, BD+63°845, FK5 355, GJ 3534, HD 81937, HIP 46733, HR 3757, SAO 14908, CCDM J09315+6303A/B [10] | |
| Database references | |
| SIMBAD | data |
23 Ursae Majoris, or 23 UMa, is a binary star system in the constellation Ursa Major, [10] located is approximately 77.7 light years from the Sun. [2] It has the Bayer designation h Ursae Majoris; 23 Ursae Majoris is the Flamsteed designation. The system is visible to the naked eye as a yellow-white hued star with an apparent visual magnitude of +3.65. [1] It is moving closer to the Earth with a heliocentric radial velocity of −10 km/s. [1]
The primary component is a yellow-white F-type subgiant with an apparent magnitude of +3.65. It has 1.9 times the Sun's mass, 2.9 times the Sun's radius and is emitting 15 times the luminosity of the Sun [11] at an effective temperature of 6,651 K. [6] Orbiting at an angular separation of 22.7 arcseconds is the 9th magnitude secondary companion. There is a magnitude +10.5 optical companion at an angular separation of 99.6 arcseconds.
With τ, υ, φ, θ, e and f, it composed the Arabic asterism Sarīr Banāt al-Na'sh, the Throne of the daughters of Na'sh, and Al-Haud, the Pond. [12] According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al-Haud was the title for seven stars : f as Alhaud I, τ as Alhaud II, e as Alhaud III, this star (h) as Alhaud IV, θ as Alhaud V, υ as Alhaud VI and φ as Alhaud VII . [13]