V0338 Dra
Simbad link | V0338 Dra |
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Source publication | Kjurkchieva, Diana P. (2018) - Observations and light curve solutions of a selection of shallow-contact W UMa binaries |
ADS link | 2018NewA...62...46K |
Name in Source publication | V0338 Dra |
Orbital period in days (P [d]) | 0.235189 |
Mass ratio (q) | 0.53 |
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]) | 0.235189 |
Mass ratio (q) | 0.53 |
Orbital inclination in degrees (i [o]) | 88.2 |
Fillout (f) | 0.17 |
Primary temperature in Kelvins (T1 [K]) | 4417 |
Secondary temperature in Kelvins (T2 [K]) | 4417 |
Primary polar radius in units of orbital separation (r1p) | 0.418 |
Secondary polar radius in units of orbital separation (r2p) | 0.3134 |
Surface potential (Ω) | 2.8819 |
Orbital separation in solar radii (a [R]) | |
---|---|
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]) | 4417 |
Secondary temperature in Kelvins (T2 [K]) | 4417 |
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 1627177398363670656 |
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RA | 237:17:48.36588 |
DEC | 60:38:04.572348 |
l | 93.79791218 |
b | 45.1546747 |
G magnitude | 16.607676 |
G_bp magnitude | 17.442348 |
G_rp magnitude | 15.367367 |
Radial velocity [km/s] | |
Parallax | 3.742742944 |
Distance [pc] | 267.183725 |
Temperature [K] | 3958.5925 |
Radius [R] | |
Luminosity [L] |
Simbad link | V0338 Dra |
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J magnitude | 11.594 |
H magnitude | 11.03 |
K magnitude | 10.892 |
Johnson_U magnitude | |
Johnson_B magnitude | 13.3 |
Johnson_V magnitude | 13.38 |
Johnson_R magnitude | |
Johnson_I magnitude | |
Sloan_u magnitude | |
Sloan_g magnitude | 13.3866 |
Sloan_r magnitude | |
Sloan_i magnitude | |
Sloan_z magnitude |