IR Vir
Simbad link | IR Vir |
---|---|
Source publication | Gomez-Forrellad, Josep M. (1995) - The Overcontact Binary System NSV 05798 |
ADS link | 1995IBVS.4257....1G |
Name in Source publication | NSV 05798 |
Orbital period in days (P [d]) | 0.36942 |
Mass ratio (q) | 0.55 |
Mass ratio determination | Photometric |
Type | A |
Has total eclipse? | |
Has spots? | |
Has third light? | |
Has period variation? |
Solver | Binary Maker |
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Orbital period in days (P [d]) | 0.36942 |
Mass ratio (q) | 0.55 |
Orbital inclination in degrees (i [o]) | 79.8 |
Fillout (f) | 0.02 |
Primary temperature in Kelvins (T1 [K]) | 6620 |
Secondary temperature in Kelvins (T2 [K]) | 6600 |
Primary polar radius in units of orbital separation (r1p) | 0.4074 |
Secondary polar radius in units of orbital separation (r2p) | 0.3084 |
Surface potential (Ω) | 2.9642 |
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]) | 6620 |
Secondary temperature in Kelvins (T2 [K]) | 6600 |
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 3680529966125234304 |
---|---|
RA | 189:32:06.43056 |
DEC | -4:00:42.681586 |
l | 296.5354347 |
b | 58.7183592 |
G magnitude | 11.697268 |
G_bp magnitude | 12.029232 |
G_rp magnitude | 11.126459 |
Radial velocity [km/s] | |
Parallax | 3.308259603 |
Distance [pc] | 302.273739 |
Temperature [K] | 5412.63 |
Radius [R] | 1.3791922 |
Luminosity [L] | 1.4708813 |
Simbad link | IR Vir |
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J magnitude | 10.423 |
H magnitude | 10.106 |
K magnitude | 9.974 |
Johnson_U magnitude | |
Johnson_B magnitude | 12.2 |
Johnson_V magnitude | 11.92 |
Johnson_R magnitude | |
Johnson_I magnitude | |
Sloan_u magnitude | |
Sloan_g magnitude | 11.6973 |
Sloan_r magnitude | |
Sloan_i magnitude | |
Sloan_z magnitude |