19360+2924 BKO  72AD

 
 
19h 36m 01.37s +29 24' 17.1" P.A. 307 sep 47 mag 9.47,13.50 Sp G5
 
 
Coord 2000
19360+2924
Discov num
BKO  72
Comp
AD
Coord arcsec 2000
19 36 01.37 +29 24 17.1
Date first
1997
Date last
2012
Obs
4
Pa first
307
Pa last
307
P.A. Now (θ)
307°
Sep first
46.8
Sep last
47.0
Sep. Now (ρ)
47"
Mag pri
9.47
Mag sec
13.50
delta mag (ΔM)
4.03
Spectral class
G5 (yellow)
Pri motion ra
-012
Sec motion ra
+001
Pri motion dec
-031
Sec motion dec
+032
Notes
N (See Notes)
rPM=1.935
This double is not physical.
 
 
19360+2924 SYSTEM COMPONENTS
 
 
Show name SAO coord_2000 discov# comp first last obs pa sep mag1 mag2 d_mag orb current
Show 19360+2924 SLE 647 AB 1895 2012 11 38 22.1 9.47 10.97 1.50
Show 19360+2924 SLE 647 AC 1895 2012 10 57 39.7 9.47 10.60 1.13
Show 19360+2924 BKO 72 AD 1997 2012 4 307 47.0 9.47 13.50 4.03 <===
Show 19360+2924 FYM 43 AE 1997 2012 3 318 46.0 9.47 14.50 5.03
Show 19360+2924 FYM 43 AF 1997 2012 3 335 41.0 9.47 13.70 4.23
Show 19360+2924 BKO 72 AG 1895 2012 8 117 81.5 9.47 11.00 1.53
Show 19360+2924 BKO 72 AH 1997 2012 4 94 93.0 9.47 14.24 4.77
Show 19360+2924 FYM 43 AJ 1997 2012 3 351 72.5 9.47 12.82 3.35
Show 19360+2924 FYM 43 AL 1997 2012 3 209 32.6 9.47 15.10 5.63
Show 19360+2924 BKO 72 DE 1997 2012 4 48 8.8 13.50 14.50 1.00
Show 19360+2924 BKO 72 DF 1895 2012 6 63 21.9 13.50 13.70 0.20
Show 19360+2924 BKO 72 HI 1997 2002 3 5 6.5 14.30 14.90 0.60
Show 19360+2924 FYM 43 JN 2012 2012 1 325 2.4 12.82 16.00 3.18
12-fold system
12 visible stars in this system
 
 
OTHER CATALOGS AND DESIGNATIONS
 
 
Precise pa
307
Precise sep
47
Cdsa2 id
BKO 72 AD
Constellation
Cygnus
Ra deg
19.600380555555557
De deg
29.40475
last precise pa
307
last precise sep
47
 
 
WDS HISTORIC DATA
 
 
coord_2000 discov_num comp epoch obs pa sep mag_pri mag_sec spectr notes coord_arcsec_2000
19360+2924 BKO 72 AD 2002 2 306 46.9 9.47 13.50 G5 D 193601.37+292417.1
19360+2924 BKO 72 AD 2012 4 307 47.0 9.47 13.50 G5 D 193601.37+292417.1

If you need more information about this double, apply for a data request form to the WDS.