ZZ PsA
Simbad link | ZZ PsA |
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Source publication | Wadhwa, Surjit S. (2006) - Photometric Analysis of Southern Contact Binary Stars III: NSV 3497 and NSV 13890 |
ADS link | 2006Ap&SS.301..195W |
Name in Source publication | NSV 13890 |
Orbital period in days (P [d]) | 0.37388 |
Mass ratio (q) | 0.08 |
Mass ratio determination | Photometric |
Type | A |
Has total eclipse? | |
Has spots? | |
Has third light? | |
Has period variation? |
Solver | WD |
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Orbital period in days (P [d]) | 0.37388 |
Mass ratio (q) | 0.08 |
Orbital inclination in degrees (i [o]) | 76.2 |
Fillout (f) | 0.9 |
Primary temperature in Kelvins (T1 [K]) | 6510 |
Secondary temperature in Kelvins (T2 [K]) | 6426 |
Primary polar radius in units of orbital separation (r1p) | 0.5623 |
Secondary polar radius in units of orbital separation (r2p) | 0.1967 |
Surface potential (Ω) | 1.848 |
Orbital separation in solar radii (a [R]) | |
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Primary radius in solar units (R1 [R]) | |
Secondary radius in solar units (R2 [R]) | |
Primary mass in solar units (M1 [M]) | |
Secondary mass in solar units (M2 [M]) | |
Primary temperature in kelvins (T1 [K]) | 6510 |
Secondary temperature in Kelvins (T2 [K]) | 6426 |
Primary luminosity in solar units (L1 [L]) | |
Secondary luminosity in solar units (L2 [L]) | |
Distance in parsecs (d [pc]) | |
Age in gigayears (τ [gyr]) |
Designation | Gaia DR2 6810113274253206912 |
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RA | 327:38:46.84812 |
DEC | -28:11:24.657072 |
l | 21.13702461 |
b | -50.11120739 |
G magnitude | 9.261176 |
G_bp magnitude | 9.555877 |
G_rp magnitude | 8.829431 |
Radial velocity [km/s] | |
Parallax | 7.353142368 |
Distance [pc] | 135.996279 |
Temperature [K] | 6100 |
Radius [R] | 1.4659286 |
Luminosity [L] | 2.6806474 |
Simbad link | ZZ PsA |
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J magnitude | 8.376 |
H magnitude | 8.133 |
K magnitude | 8.062 |
Johnson_U magnitude | 8.739 |
Johnson_B magnitude | 9.956 |
Johnson_V magnitude | 9.35 |
Johnson_R magnitude | |
Johnson_I magnitude | |
Sloan_u magnitude | |
Sloan_g magnitude | 9.2612 |
Sloan_r magnitude | |
Sloan_i magnitude | 8.739 |
Sloan_z magnitude |