CI Orionis
catalogues and names
catalogues and names | CI Ori, 31 Ori, HR 1834, HD 36167, SAO 132176, BD -1 913, WDS 05297-0106 |
constellation | Orion |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
position, motion, parallax:
position (J2000) | RA: 5h 29min 44sec | DEC: -1° 5' 32'' | ||
position (B1900) | RA: 5h 24min 39.2sec | DEC: -1° 10' 15'' | ||
proper motion (J2000) | RA: 0.004 arcsec/a | DEC: -0.023 arcsec/a | ||
radial velocity | 8 km/s note: spectroscopic binaries |
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rotational velocity | <19 km/s | |||
trigonometric parallax | 0.006 arcsec | |||
galactic coordinates | longitude: 204.31° | latitude: -18.62° |
magnitude
visual magnitude | 4.71 (V on UBV Johnson system) |
spectral / color information
spectral class | K5III |
B-V-magnitude | 1.57 |
U-B-magnitude | 1.85 |
R-I-magnitude | |
IR-note | object is infrared source (NASA merged infrared catalogue, Schmitz et al., 1978) |
variability information
variable star identification | CI Ori |
note (category: variability): | ADS 4097, cst? 4.67: -4.71V. |
double/multiple star system information
separation | 12.5 arcsec |
mag difference (of double or brightest multiple) | 5.4 |
note (category: double and multiple data): | CPM. Companion 9.70V, +0.71(B-V), +0.15(U-B), F7V. |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 5h 29min 43.969sec | DEC: -1° 5' 32.36'' | ±0.43 arcsec | source: 16 |
proper motion (J2000) | RA: 0 arcsec/a | DEC: -0.022 arcsec/a | source: 25 | |
radial velocity | 8 km/s | source: 25 | ||
trigonometric parallax | 0.006 arcsec | ±0.001 arcsec | source: 25 | |
galactic coord. (B1950) | longitude: 204.31° | latitude: -18.62° |
magnitude:
visual | 4.71 (observed) | source: 25 |
photovisual | 5 | source: 2 |
photographic | 6.9 | source: 16 |
spectral information:
spectral class | K5 | source: 96 | |
Morgan-Keenan | K5III | source: 25 | |
B-magnitude | 6.28 ±0.05 | B-V-magnitude | 1.57 |
U-magnitude | 8.13 ±0.05 | U-B-magnitude | 1.85 |
variability information:
variability type | 999 |
var. amplitude | 0.04 |
double/multiple star system information:
separation between brightest and second brightest component | 12.7 arcsec |
magnitude difference between brightest and second brightest component | 5.01 |
position angle | 87 ° |
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 | |
16 | PPM North and PPM South Catalogs and PPM Supplement |
Roser, S., and U. Bastian, "Catalogue of Positions and Proper Motions," A&AS, Vol. 74, p. 449, 1988, and Bastian, U., et al., "Catalogue of Positions and Proper Motions - South," 1993 | |
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 | |
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 27min 11.524sec | DEC: -1° 7' 48.08'' | ±0.019 arcsec |
position (J2000) | RA: 5h 29min 43.998sec | DEC: -1° 5' 31.71'' | |
proper motion B1950 (FK4) | RA: 0 arcsec/a | DEC: -0.022 arcsec/a | ±0.003 arcsec/a in RA ±0.003 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: 0.0003 arcsec/a | DEC: -0.023 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 5 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from Harvard or San Luis photometry. |
spectral information:
spectral class | K5 |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
remarks for duplicity and variability
Double star in Aitken's Double Star Catalogue (Aitken 1932) |
catalogues
source catalogue | GC, catalogue number: 6792 |
Durchmusterung | BD-01 913 |
Boss General Catalogue | 6792 |
Henry Draper Catalogue | 36167 |
data from The Washington Visual Double Star Catalog, 1996.0 (Worley+, 1996)
position and proper motion:
position (J2000) | RA: 5h 29.7min | DEC: -1° 6' |
proper motion (J2000) | RA: 0.007 arcsec/a | DEC: -0.034 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 |
- | 1829 | 14 | 87° | 12.7'' | 4.69 | 9.7 | K5III | STF 725 |
discoverer information:
discoverer code | discoverer | reference |
STF 725 | Struve, F.G.W. | - |
notes:
note | 31 Ori. A is the variable CI Ori. Proper motion of B +029 -030. |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 5h 27min 11.5sec | DEC: -1° 7' 48'' |
variability informations:
variability type | CST: |
magnitute at max. brightness | 4.67: |
magnitute at min. brightness | 4.71 |
photometric system | visual, photovisual or Johnson's V |
spectral information
spectral class | K5III |
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 | 60/110 |
constellation | Orion |
notes on existence | The star is equivalent to '0600111 CK'. |
There are notes in published catalog. |
variability type description
variability type | description |
CST | Nonvariable stars, formerly suspected to be variable and hastily designated. Further observations have not confirmed their variability. |