Vega
catalogues and names | Vega, a Lyr, alf Lyr, 3 Lyr, HR 7001, HD 172167, SAO 67174, FK5: 699, WDS 18369+3846A |
other names | Wega, Fidis, Harp Star |
constellation | Lyra |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
note (category: star names): | VEGA; Wega; Fidis; Harp Star. |
position, motion, parallax:
position (J2000) | RA: 18h 36min 56,3sec | DEC: +38° 47' 1'' |
position (J1900) | RA: 18h 33min 33,1sec | DEC: +38° 41' 26'' |
proper motion (J2000) | RA: 0,202 arcsec/a | DEC: 0,286 arcsec/a |
radial velocity | -14 km/s note: variable radial velocity |
|
rotational velocity | 15 km/s (uncertain) (variable) | |
trigonometric parallax | 0,123 arcsec |
note (category: radial and/or rotational velocities): | Pulsation 0.1903d. |
magnitude
visual magnitude | 0,03 (V on UBV Johnson system) |
spectral / color information
spectral class | A0Va |
B-V-magnitude | 0 |
U-B-magnitude | -0,01 |
R-I-magnitude | -0,03 |
note (category: spectra): | Cadmium found for first time in spectra from COPERNICUS. |
note (category: colors): | Color excess E(B-V) = 0.00. Displays IR excess, however, attributed to possible proto-planetary debris. |
variability information
variable star identification | Alp Lyr |
note (category: variability): | Delta Sct -0.02 to +0.07V, 0.19d. |
double/multiple star system information
number of components of multiple star system | 5 |
separation | 62,8 arcsec |
mag difference (of double or brightest multiple) | 10,4 |
component ID | AB |
note (category: double and multiple data): | Companions in IDS optical. BD=+38d3231, 8.6v, 23' N. prec., may be CPM. |
miscellaneous information
note (category: stellar radii or diameters): | Diam. = 0.00308 - 0.00324". |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 18h 36min 56,332sec | DEC: +38° 47' 1,17'' | ±0,06 arcsec | source: 15 |
proper motion (J2000) | RA: 0,0173 arcsec/a | DEC: 0,286 arcsec/a | source: 25 | |
radial velocity | -14 km/s | source: 25 | ||
trigonometric parallax | 0,123 | ±0,012 arcsec | source: 25 | |
galactic coord. (B1950) | longitude: 67,45° | latitude: 19,24° | ||
GCI unit vector (J2000) | X: 0,125096 | Y: -0,769413 | Z: 0,626381 |
magnitude:
visual | 0 (observed) | source: 31 |
photovisual | 0,1 | source: 2 |
spectral information:
spectral class | A0 | source: 96 | |
Morgan-Keenan | A0Va | source: 25 | |
B-magnitude | 0,03 ±0,05 | B-V-magnitude | 0 |
U-magnitude | 0,02 ±0,05 | U-B-magnitude | -0,01 |
variability information:
variability type | 10 |
var. amplitude | 0,09 |
var. period | 0,19 |
double/multiple star system information:
separation between brightest and second brightest component | 62,8 arcsec |
magnitude difference between brightest and second brightest component | 9,5 |
position angle | 173 ° |
sources:
2 | HD and HDE Catalogs |
Cannon, A.J., and E.C. Pickering, Harvard Annals, Vols 91-99, 1918-24, Cambridge, Massachusetts: Harvard University; Cannon, A.J., Harvard Annals, Vol. 100, 1925-36, Cambridge, Massachusetts: Harvard University; and Cannon, A.J., and M. Walton Mayall, Harvard Annals, Vol. 112, 1949, Cambridge, Massachusetts: Harvard University | |
15 | FK5, FK5 Extension and FK5 Supplement |
Fricke, W., H. Schwan and T. Lederle, "Fifth Fundamental Catalogue (FK5), Part I. The Basic Fundamental Stars," Veroff. Astronomisches Recheninstitut, No. 32, Heidelberg, Germany, 1988, and Fricke, W., H. Schwan, and T.E. Corbin, "Fifth Fundamental Catalogue (FK5), Part II. The FK5 Extension," Veröff. Astronomisches Recheninstitut, No. 33, Heidelberg, Germany, 1991 | |
19 | WDS Catalog |
Worley, C.E., and G.G. Douglass, Washington Catalog of Visual Double Stars 1996.0, United States Naval Observatory, 1996 | |
25 | Bright Star Catalogue, 5th edition |
Hoffleit, D. and Warren, W.H. Jr., The Bright Star Catalogue, 5th Revised Edition, Version 2, 1994 | |
30 | GCVS, 4th edition |
Kholopov, P.N., et al., General Catalogue of Variable Stars, fourth edition, Moscow: Nauka Publishing House, 1985-88 | |
31 | CRM' (non-GCVS variable data) |
Warren, W.H. Jr., Northern Hemisphere Catalog of Red Magnitudes, 1994 | |
96 | SAO or HD/HDE Catalog |
Reference from Value 1 or Reference from Value 2 |
data from Smithsonian Astrophysical Observatory Star Catalog (SAO Staff 1966; USNO, ADC 1990)
position and proper motion:
position (J1950) | RA: 18h 35min 14,655sec | DEC: +38° 44' 9,68'' | ±0,003 arcsec |
position (J2000) | RA: 18h 36min 56,336sec | DEC: +38° 47' 1,18'' | |
proper motion J1950 (FK4) | RA: 0,0171 arcsec/a | DEC: 0,285 arcsec/a | ±0,001 arcsec/a in RA ±0,001 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: 0,0173 arcsec/a | DEC: 0,286 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 0,1 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from the "Henry Draper Catalogue". |
spectral information:
spectral class | A0 |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
catalogues
source catalogue | FK4, catalogue number: 699 |
Durchmusterung | BD+38 3238 |
Boss General Catalogue | 25466 |
Henry Draper Catalogue | 172167 |
data from The Washington Visual Double Star Catalog, 1996.0 (Worley+, 1996)
position and proper motion:
position (J2000) | RA: 18h 36,9min | DEC: +38° 46' |
proper motion (J2000) | RA: 0,202 arcsec/a | DEC: 0,286 arcsec/a |
double/multiple star system information:
component | year | number of measures | position angle | angular separation | magnitude of 1st component | magnitude of 2nd component | spectral class(es) | discoverer code |
AB | 1836 | 43 | 138° | 43'' | 0,03 | 9,5 | A0Va | H 39 |
1946 | 173° | 62,8'' | ||||||
AC | 1864 | 4 | 299° | 46,9'' | 0 | 11 | - | STF 9 |
1899 | 285° | 54,4'' | ||||||
AE | 1905 | 3 | 39° | 124,5'' | 0 | 9,5 | - | STF 9 |
1921 | - | 118,5'' | ||||||
BC | 1864 | 1 | 314° | 89,6'' | - | - | - | STF |
CD | 1897 | 1 | 35° | 31,3'' | 11 | - | - | STF 9 |
discoverer information:
discoverer code | discoverer | reference |
H 39 | Herschel, W. | - |
STF 9 | Struve, F.G.W. | - |
STF | Struve, F.G.W. |
notes:
note | AB: H V 39. Alpha Lyr. Proper motion of B +004 -006. Proper motion of B +002 +013. AE: Proper motion of E +007 -004. The components are optical. |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (J1950) | RA: 18h 35min 14,7sec | DEC: +38° 44' 10'' |
variability informations:
variability type | DSCTC | pulsating variable star |
magnitute at max. brightness | -0,02 | |
magnitute at min. brightness | 0,07 | |
photometric system | visual, photovisual or Johnson's V | |
period [d] | 0,19 |
spectral information
spectral class | A0V |
references
to a study | Vol. I GCVS (see Kholopov et al. 1985-1988) |
to a chart/photograph | no chart is avaible, but the star is contained in the 'Bonner Durchmusterung' |
miscanellous
ID in the GCVS catalogue | 52/9001 |
constellation | Lyra |
notes on existence | The star is equivalent to '0529002 bet'. |
There are notes in published catalog. |
variability type description
variability type | description |
DSCTC | Variables of the Delta Scuti type. These are pulsating variables of spectral types A0-F5 III-V displaying light amplitudes from 0.003 to 0.9 mag in V (usually several hundredths of a magnitude) and periods from 0.01 to 0.2 days. The shapes of the light curves, periods, and amplitudes usually vary greatly. Radial as well as nonradial pulsations are observed. The variability of some members of this type appears sporadically and sometimes completely ceases, this being a consequence of strong amplitude modulation with the lower value of the amplitude not exceeding 0.001 mag in some cases. The maximum of the surface layer expansion does not lag behind the maximum light for more than 0.1 periods. DSCT stars are representatives of the galactic disk (flat component) and are phenomenologically close to the SX Phe variables. DSCTC Low amplitude group of Delta Sct variables (light amplitude <0.1 mag in V). The majority of this type's representatives are stars of luminosity class V; objects of this subtype generally are representative of the Delta Sct variables in open clusters. |