System: HR 5025 - All bodies
Distance to Sol: 205.49 ly
Spectral Class: A - Scoopable
Luminosity Class: IV - Subgiant
Age: 568 Million years
Solar Masses: 1.8594
Solar Radius: 1.5622
Surface Temperature: 9,344 K
Orbital Period: 6,042.4 D
Semi Major Axis: 2.87 AU
Orbital Eccentricity: 0.1344
Orbital Inclination: -4.10 °
Arg Of Periapsis: 340.28 °
Absolute Magnitude: 2.2200
Attractions: None

Class A stars are hot white or bluish white main sequence stars. They range in mass from 1.4 to 2.1 solar masses and have a surface temperature reaching 10,000 K.

A subgiant is a star that is slightly brighter than a normal main-sequence (dwarf) star of the same spectral class, but not as bright as true giant stars. Although certain subgiants appear to be simply unusually bright metal-rich hydrogen-fusing stars (in the same way subdwarfs are unusually dim metal-poor hydrogen-fusing stars), they are generally believed to be stars that are ceasing or have already ceased fusing hydrogen in their cores. In stars of roughly a solar mass (M), this causes the core to contract, which increases the star's central temperature enough to move hydrogen fusion into a shell surrounding the core. This swells the star on the way to becoming a true giant.