CSS J071813.2+505000
Simbad link | CSS J071813.2+505000 |
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Source publication | Kjurkchieva, D. P. (2017) - Observations and light curve solutions of the eclipsing W UMa binaries CSS J071813.2+505000, NSVS 2459652, NSVS 7178717 and NSVS 7377875 |
ADS link | 2017RMxAA..53..133K |
Name in Source publication | CSS J071813.2+505000 |
Orbital period in days (P [d]) | 0.38635 |
Mass ratio (q) | 0.49 |
Mass ratio determination | Photometric |
Type | A |
Has total eclipse? | |
Has spots? | |
Has third light? | |
Has period variation? |
Solver | PHOEBE |
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Orbital period in days (P [d]) | 0.38635 |
Mass ratio (q) | 0.49 |
Orbital inclination in degrees (i [o]) | 58.9 |
Fillout (f) | 0.01 |
Primary temperature in Kelvins (T1 [K]) | 6420 |
Secondary temperature in Kelvins (T2 [K]) | 6193 |
Primary polar radius in units of orbital separation (r1p) | 0.4171 |
Secondary polar radius in units of orbital separation (r2p) | 0.2977 |
Surface potential (Ω) | 2.845 |
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]) | 6420 |
Secondary temperature in Kelvins (T2 [K]) | 6193 |
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 980212112198364416 |
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RA | 109:33:18.8784 |
DEC | 50:49:59.968092 |
l | 166.6302473 |
b | 24.77580522 |
G magnitude | 14.257383 |
G_bp magnitude | 14.554535 |
G_rp magnitude | 13.793174 |
Radial velocity [km/s] | |
Parallax | 0.029500272 |
Distance [pc] | 33897.992534 |
Temperature [K] | 5803.475 |
Radius [R] | |
Luminosity [L] |
Simbad link | CSS J071813.2+505000 |
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J magnitude | |
H magnitude | |
K magnitude | |
Johnson_U magnitude | |
Johnson_B magnitude | |
Johnson_V magnitude | 14.29 |
Johnson_R magnitude | |
Johnson_I magnitude | |
Sloan_u magnitude | |
Sloan_g magnitude | 14.2574 |
Sloan_r magnitude | |
Sloan_i magnitude | |
Sloan_z magnitude |