HIP 7617
HIP 7617 is a G-type (Yellow) star located in the constellation Cassiopeia.
At a distance of roughly 1,744 light-years, HIP 7617 is a distant star lying deep within the Milky Way galaxy.
HIP 7617 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
With an apparent magnitude of +5.55, HIP 7617 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its orange hue, which corresponds to a B-V color index of +1.388.
Physical Properties
| Spectral Class | Class G — G-type (Yellow) |
| Color Index (B−V) | 1.388 |
Observation
| Apparent Magnitude | +5.55 |
| Absolute Magnitude | -3.09 |
| Distance | 1,744 ly |
| Constellation | Cassiopeia |
Position
| Right Ascension | 1h 38.13m |
| Declination | 57° 58.66′ |
Frequently Asked Questions
What type of star is HIP 7617?
HIP 7617 is a Class G — G-type (Yellow) star.
How far is HIP 7617 from Earth?
HIP 7617 is approximately 1,744.2 light-years from Earth.
Can you see HIP 7617 with the naked eye?
With an apparent magnitude of 5.55, HIP 7617 is visible to the naked eye.
What constellation is HIP 7617 in?
HIP 7617 is located in the constellation Cassiopeia.