18500+1519 YSC 12 AB (HD 174457)
18h 50m 02.00s +15° 18' 40.3" P.A. 35.00 sep 0.5 mag 7.60,11.30 Sp F8+M2V dist. 53.22 pc (173.6 l.y.)
Coord 2000 |
18500+1519 |
|
Discov num |
YSC 12 |
|
Comp |
AB |
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Coord arcsec 2000 |
18 50 02.00 +15 18 40.3 |
|
Date first |
2001 |
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Date last |
2019 |
|
Obs |
19 |
|
Pa first |
77 |
|
Pa last |
35 |
|
P.A. Now (θ) |
35° |
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Sep first |
0.4 |
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Sep last |
0.479 |
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Sep. Now (ρ) |
0.479" |
|
Mag pri |
7.60 |
|
Mag sec |
11.30 |
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delta mag (ΔM) |
3.7 |
|
Spectral class |
F8+M2V (yellow-white/red) |
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Pri motion ra |
+102 |
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Sec motion ra |
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Pri motion dec |
+131 |
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Sec motion dec |
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Notes |
N
O
(See Notes, Orbital solution) |
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This double is physical.
18500+1519 SYSTEM COMPONENTS
Show |
name |
SAO |
coord |
wds_name |
last |
obs |
pa |
sep |
mag1 |
mag2 |
d_mag |
orb |
current |
Show |
HD 174457 |
104160 |
18 50 02 +15 18 40 |
YSC 12 AB |
2019 |
19 |
35 |
0.5 |
7.60 |
11.30 |
3.70 |
Y |
<=== |
Show |
|
104160 |
18 50 02 +15 18 40 |
LLO 16 AC |
2001 |
2 |
19 |
11.1 |
5.99 |
13.30 |
7.31 |
|
|
Show |
|
104160 |
18 50 02 +15 18 40 |
LLO 16 AD |
2015 |
4 |
225 |
15.7 |
5.99 |
13.50 |
7.51 |
|
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Quadruple system
4 estimated visually detectable stars in this system
OTHER CATALOGS AND DESIGNATIONS
Name |
HD 174457 |
|
Constellation |
Hercules |
|
SAO |
104160 |
|
HIP |
92418 |
|
Tycho2 |
1584-00540-1 |
|
Gaia DR2 |
4507523307652284288 |
|
HD |
174457 |
|
GC |
25831 |
|
BD |
BD+15 3584 |
|
Distance |
53.22 |
|
Distance ly |
173.6 |
|
ORBITAL ELEMENTS
Period (P) | 105y | |
Periastron (T) | 2121.131y | |
Semi-major axis (a) | 0.486a | |
Eccentricity (e) | 0 | |
Inclination (i) | 143.4° | |
Longitude of periastron (ω) | 0° | |
Node (Ω) | 45.4° | |
Notes | | |
Reference | Tok2018e | |
Equinox | 2000 | |
Last observation | 2018 | |
Grade | 5 | (1=Definitive, 9=Indet.) |
label |
theta |
rho |
2000 |
94.6 |
0.424 |
2001 |
91.1 |
0.429 |
2002 |
87.6 |
0.435 |
2003 |
84.2 |
0.441 |
2004 |
80.9 |
0.446 |
2005 |
77.6 |
0.452 |
2006 |
74.5 |
0.457 |
2007 |
71.4 |
0.462 |
2008 |
68.4 |
0.467 |
2009 |
65.5 |
0.471 |
2010 |
62.5 |
0.475 |
2011 |
59.7 |
0.478 |
2012 |
56.9 |
0.481 |
2013 |
54.1 |
0.483 |
2014 |
51.3 |
0.485 |
2015 |
48.5 |
0.486 |
2016 |
45.8 |
0.486 |
2017 |
43.0 |
0.486 |
2018 |
40.2 |
0.485 |
2019 |
37.5 |
0.483 |
2020 |
34.7 |
0.481 |
2021 |
31.9 |
0.479 |
2022 |
29.0 |
0.476 |
2023 |
26.1 |
0.472 |
2024 |
23.2 |
0.468 |
2025 |
20.2 |
0.463 |
2026 |
17.1 |
0.458 |
2027 |
14.0 |
0.453 |
2028 |
10.8 |
0.448 |
2029 |
7.5 |
0.442 |
2030 |
4.1 |
0.436 |
|
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Note: Theta is PA, Rho is Sep. For yearly orbits, data refer to Jan 1st.
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Measures: green=micrometric, blue=interferometric, purple=photographic |
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