Arcturus
Is Arcturus (α Boo, α Boötis, Alpha Boötis) sa réaltbhuíon Boötes an réalta is gile sa leathsféar thuaidh spéartha. Le mhéid radharcach de −0.05, s’é an ceathrú réalta is gile i spéir na hoíche ag leanúint Sirius de mhéid -1.46, Canopus de mhéid -0.86 agus Alpha Centauri de mhéid -0.27. Tá sé ina réalta i ngar go maith mar níl sé ach ar chianfhad de 36.7 solasbhliain ón Dhomhain agus mar aon le Vega agus Sirius is cheann de na réaltaí is lonraí i gcomharsanacht na Gréine é.
Cineál
[cuir in eagar | athraigh foinse]Tá Arcturus ina réalta oráisteach de chineál K0 III le dearbhmhéid de -0.30. Is dócha go bhfuil a hidrigin cáite óna chorplár agus go bhfuil sé anois ina réim loscaidh slige hidrigine. Leanfaidh sé ag méadú roimh dul isteach sa réim craobh cothrománach dá thimthriall beatha.
Tá Arcturus i réaltbhuíon Boötes.
Sonra Breathnaithe
[cuir in eagar | athraigh foinse]Réaltbhuíon Boötes
Fuaimneadh /ɑːrkˈtjʊərəs/
Ceartéirí 14u 15n 39.7s
Díochlaonadh +19° 10′ 56″
Méid fhollasach (breathnaithe) −0.05
Tréithe
[cuir in eagar | athraigh foinse]Cineál speictreach K0 III
Méid fhollasach (radharcach) −2.25
U−B innéacs dathach +1.28
B−V innéacs dathach +1.23
R−I innéacs dathach +0.65
Nóta (catagóir: athrógach): H and K astaíocht
Réaltmhéadracht
[cuir in eagar | athraigh foinse]Luas gathach (Rv) −5.19 km/s
Gluaiseacht ceart (μ) RA: −1093.45 mais/yr
Dec.: −1999.40[5] mais/bhl
Saobhdhiallas (π) 88.83 ± 0.54[1] mais
Cianfhad 36.7 ± 0.2 sbh ,, (11.26 ± 0.07 pc)
Dearbhmhéid (MV) −0.30±0.02
Mionphointí
[cuir in eagar | athraigh foinse]Mais 1.08±0.06 M☉
Ga 25.4±0.2 R☉
Lonrachas 170 L☉
Imtharraingt dromchlach (log g) 1.66±0.05 cgs
Teocht 4286±30 K
Cóimheas miotalach [Fe/H] −0.52±0.04 dex
Luas rothlaithe (v sin i) 2.4±1.0 km/s
Aois 7.1+1.5 | −1.2 Gbhl
Ainmchomharthaí eile
[cuir in eagar | athraigh foinse]Alramech, Abramech, α Boötis, 16 Boötes, BD+19°2777, GCTP 3242.00, GJ 541, HD 124897, HIP 69673, HR 5340, LHS 48, SAO 100944.
Tagairtí storshonracha SIMBAD sonra
- ↑ Olin J. Eggen (1962). "Space-velocity vectors for 3483 stars with proper motion and radial velocity": 79.
- ↑ Caroline Soubiran (Márta 2008). "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants" (as Béarla) (1): 91–101. doi: .
- ↑ Ráite i: Catalogue of Stellar Photometry in Johnson's 11-color system. Stated in source according to: SIMBAD. Teanga an tsaothair nó an ainm: Béarla. Dáta foilsithe: 2002.
- ↑ 4.0 4.1 Henrik Jönsson (8 Feabhra 2017). "Abundances of disk and bulge giants from high-resolution optical spectra. I. O, Mg, Ca, and Ti in the solar neighborhood and Kepler field samples" (as Béarla). doi: .
- ↑ 5.0 5.1 5.2 George David Gatewood (13 Meitheamh 2008). "Astrometric Studies of Aldebaran, Arcturus, Vega, the Hyades, and Other Regions" (as Béarla) (1): 452–460. doi: .
- ↑ David Latham (7 Nollaig 2007). "Rotational and radial velocities for a sample of 761 Hipparcos giants and the role of binarity" (as Béarla) (1): 209–231. doi: .
- ↑ Henrik Jönsson (8 Feabhra 2017). "Abundances of disk and bulge giants from high-resolution optical spectra. I. O, Mg, Ca, and Ti in the solar neighborhood and Kepler field samples" (as Béarla). doi: .
- ↑ 8.0 8.1 Floor van Leeuwen (2007). "Validation of the new Hipparcos reduction" (as Béarla) (2): 653–664. doi: .
- ↑ Richard J. Patterson (5 Nollaig 2012). "Identifying contributions to the stellar halo from accreted, kicked-out, and in situ populations" (as Béarla) (2): 161. doi: .