V1032 Orionis
catalogues and names
catalogues and names | V1032 Ori, 11 Ori, HR 1638, HD 32549, SAO 94290, BD +15 732, FK5: 1140 |
constellation | Orion |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
position, motion, parallax:
position (J2000) | RA: 5h 4min 34.1sec | DEC: +15° 24' 15'' | ||
position (2000.72) | RA: 5h 4min 36sec | DEC: +15° 24' 18'' | ||
position (B1900) | RA: 4h 58min 51.2sec | DEC: +15° 15' 54'' | ||
proper motion (J2000) | RA: 0.016 arcsec/a | DEC: -0.034 arcsec/a | ||
radial velocity | 17 km/s note: variable radial velocity |
|||
rotational velocity | 36 km/s (uncertain) (variable) | |||
trigonometric parallax | 0.018 arcsec | |||
galactic coordinates | longitude: 186.18° | latitude: -15.35° |
magnitude
visual magnitude | 4.68 (V on UBV Johnson system) |
spectral / color information
spectral class | A0pSi |
B-V-magnitude | -0.06 |
U-B-magnitude | -0.09 |
R-I-magnitude |
variability information
variable star identification | V1032 Ori |
note (category: variability): | Alpha CV, 4.65 - 4.69V, amp. 0.03y, 4.6398d. |
miscellaneous information
note (category: group membership): | Member of Pleiades group. |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 5h 4min 34.143sec | DEC: +15° 24' 14.65'' | ±0.06 arcsec | source: 15 |
position (2000.72) | RA: 5h 4min 36sec | DEC: +15° 24' 18'' | JD: 2451809.25 | |
proper motion (J2000) | RA: 0.0011 arcsec/a | DEC: -0.034 arcsec/a | source: 25 | |
radial velocity | 17 km/s | source: 25 | ||
trigonometric parallax | 0.018 arcsec | ±0.002 arcsec | source: 25 | |
galactic coord. (B1950) | longitude: 186.19° | latitude: -15.35° |
magnitude:
visual | 4.68 (observed) | source: 25 |
photovisual | 4.7 | source: 2 |
spectral information:
spectral class | B9 | source: 96 | |
Morgan-Keenan | A0pSi | source: 25 | |
B-magnitude | 4.62 ±0.05 | B-V-magnitude | -0.06 |
U-magnitude | 4.53 ±0.05 | U-B-magnitude | -0.09 |
variability information:
variability type | 160 |
var. amplitude | 0.04 |
var. period | 4.64 |
var. epoch | 2443865 22. December 1978, 12:00:00 UT |
next max light | 2451813.32 25. September 2000, 19:40:48 UT |
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 | |
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 | |
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 (B1950) | RA: 5h 1min 42.545sec | DEC: +15° 20' 10.18'' | ±0.005 arcsec |
position (2000.72) | RA: 5h 4min 37sec | DEC: +15° 24' 20'' | JD: 2451809.25 |
position (J2000) | RA: 5h 4min 34.144sec | DEC: +15° 24' 14.54'' | |
proper motion B1950 (FK4) | RA: 0.0011 arcsec/a | DEC: -0.035 arcsec/a | ±0.001 arcsec/a in RA ±0.001 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: 0.0011 arcsec/a | DEC: -0.035 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 4.6 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from the "Henry Draper Catalogue". |
spectral information:
spectral class | B9 |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
catalogues
source catalogue | FK4, catalogue number: 1140 |
Durchmusterung | BD+15 732 |
Boss General Catalogue | 6191 |
Henry Draper Catalogue | 32549 |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 5h 1min 42.5sec | DEC: +15° 20' 10'' |
variability informations:
variability type | ACV | rotating variable star |
magnitute at max. brightness | 4.65 | |
magnitute at min. brightness | 4.69 | |
photometric system | visual, photovisual or Johnson's V | |
epoch for maximum light [JD] | 2443864.78 22. December 1978, 06:43:12 UT |
|
period [d] | 4.6398 | |
next maximum light [JD] | 2451812.7574 25. September 2000, 06:10:39 UT |
|
rising time | 50 % of period |
spectral information
spectral class | B9p(Si) |
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 | 60/1032 |
constellation | Orion |
notes on existence | The star is equivalent to '0601033 V1033'. |
variability type description
variability type | description |
ACV | Alpha2 Canum Venaticorum variables. These are main-sequence stars with spectral types B8p-A7p and displaying strong magnetic fields. Spectra show abnormally strong lines of Si, Sr, Cr, and rare earths whose intensities vary with rotation. They exhibit magnetic field and brightness changes (periods of 0.5-160 days or more). The amplitudes of the brightness changes are usually withine 0.01-0.1 mag in V. ACVO Rapidly oscillating Alpha2 CVn variables. These are nonradially pulsating, rotating magnetic variables of Ap spectral type (DO Eri). Pulsation periods are in the range of 6-12 mmag (0.004-0.01 days), while amplitudes of light variation caused by the pulsation are about 0.01 mag in V. The pulsational variations are superposed on those caused by rotation. |