BD+03 2562 b
Orbiting BD+03 2562
BD+03 2562 b is an exoplanet orbiting the star BD+03 2562, discovered in 2017 using the Radial Velocity method.
Minimum Mass (M sin i)
2034.11
Earth masses
Orbital Period
481.9
days
Distance
1070.6
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
2034.11
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Villaver et al. 2017
Orbital Period
481.900+2.700−2.800days
Semi-Major Axis
1.3000+0.1000−0.1000au
M sin(i) (Earth masses)
2034.11+413.18−413.18
M sin(i) (Jupiter masses)
6.4000+1.3000−1.3000
Eccentricity
0.2000+0.1200−0.0800
Epoch of Periastron
2453726.00+41.00−32.00days(JD)
Argument of Periastron
218.0+32.0−26.0deg
Radial Velocity Semi-Amplitude
155.70+1.00−3.30m/s
Distance from Earth
1070.6 pc (~3492 ly)
Spectral Type
Unknown
Temperature
4095 K
Mass (Solar)
1.14 M☉
Radius (Solar)
32.35 R☉
Luminosity
2.70 log L☉
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
177.5647°, 2.7601°
Discovery Method
Radial Velocity
Discovery Year
2017
Source ID: BD+03 2562 b
BD+03 2562 b orbits BD+03 2562 and was reported in 2017 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 2,034.11 Earth masses (M sin i) and an orbital period of 481.9 days.
Catalog data places the system at about 1,070.6 parsecs from Earth and 1 known planet in the system.
Host star
Explore the stellar record for this system to compare temperature, spectral type, and known planets.
Open BD+03 2562