Megrez
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| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Ursa Major |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | +3.312[2] |
| Characteristics | |
| Spectral type | A3 V[3] |
| U−B Template:Engvar | +0.067[2] |
| B−V Template:Engvar | +0.075[2] |
| Astrometry | |
| Radial velocity (Rv) | -20.2[4] km/s |
| Proper motion (μ) | RA: +104.11[1] mas/yr Dec.: 7.30[1] mas/yr |
| Parallax (π) | 40.51±0.15 mas[1] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Absolute magnitude (MV) | +1.39[5] |
| Details[6] | |
| Mass | Script error: No such module "val". Template:Solar mass |
| Radius | 2.512 (equatorial) 1.921 (polar) Template:Solar radius |
| Luminosity | Script error: No such module "val". Template:Solar luminosity |
| Surface gravity (log g) | 4.49[7] cgs |
| Temperature | 6,909 (equatorial) 10,030 (polar) K |
| Rotation | 3.1[6]Template:Efn hours |
| Rotational velocity (v sin i) | Script error: No such module "val". km/s |
| Age | Script error: No such module "val". Myr |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| Template:Odlist, IDS 12105+5735 A[8] | |
| Database references | |
| SIMBAD | data |
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Megrez Template:IPAc-en, also called Delta Ursae Majoris (δ Ursae Majoris, abbreviated Delta UMa, δ UMa),[9][10] is a star in the northern constellation of Ursa Major. With an apparent magnitude of +3.3,[2] it is the dimmest of the seven stars in the Big Dipper asterism. Parallax measurements yield a distance estimate of Script error: No such module "convert". from the Sun.[1]
Stellar properties
Megrez has two times more mass than the Sun and is about 23 times more luminous.[6] It has a stellar classification of A3 V,[3] which means it is an A-type main sequence star that is generating energy at its core through the nuclear fusion of hydrogen. It rotates rapidly, taking 3.1 hours to complete a rotation across its equator, causing Megrez to have an oblate shape and hotter temperatures at the poles due to gravity darkening.[6]
This star has an excess emission of infrared radiation, indicating the presence of circumstellar matter. This forms a debris disk around an orbital radius of 16 astronomical units from the star. This radius is unusually small for the estimated age of the disk, which may be explained by drag from the Poynting–Robertson effect causing the dust to spiral inward.[11]
It has two faint companions, a 10th magnitude star and an 11th magnitude star, both at an angular separation of two arcminutes from the primary.[12]
Delta Ursae Majoris is a member of the Ursa Major moving group, an association of stars that share a common motion through space and likely formed in the same molecular cloud. The space velocity components of Delta Ursae Majoris in the galactic coordinate system are [U, V, W] = [+15.35, +1.17, –11.52] km s−1.[13]
Nomenclature
δ Ursae Majoris (Latinised to Delta Ursae Majoris) is the star's Bayer designation.
It bore the traditional name Megrez Template:IPAc-en and the historical name Kaffa. Megrez comes from the Template:Langx al-maghriz 'the base [of the bear's tail]'. Professor Paul Kunitzch has been unable to find any clues as to the origin of the name Kaffa, which appeared in a 1951 publication, Atlas Coeli (Skalnate Pleso Atlas of the Heavens) by Czech astronomer Antonín Bečvář.[14]
The Hindus knew this star as Atri, one of the Seven Rishis.[15]
In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Northern Dipper, refers to an asterism equivalent to the Big Dipper. Consequently, the Chinese name for Delta Ursae Majoris itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx) and Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx).[16]
Namesakes
USS Megrez (AK-126) was a United States Navy Crater class cargo ship named after the star.
Notes
References
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- ↑ Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 15 日 Script error: No such module "webarchive".
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- Pages with script errors
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- A-type main-sequence stars
- Triple star systems
- Ursa Major moving group
- Stars with proper names
- Bayer objects
- Big Dipper
- Ursa Major
- Durchmusterung objects
- Flamsteed objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Bright Star Catalogue objects
- Gliese and GJ objects