HIP 10457
HIP 10457 is a K-type (Orange) star located in the constellation Andromeda.
At a distance of roughly 1,000 light-years, HIP 10457 is a distant star lying deep within the Milky Way galaxy.
HIP 10457 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 10457 has an apparent magnitude of +8.91, placing it beyond naked-eye visibility. A good pair of binoculars or a small telescope is required to observe this star. Observers will note its yellow hue, which corresponds to a B-V color index of +0.922.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 0.922 |
Observation
| Apparent Magnitude | +8.91 |
| Absolute Magnitude | 1.48 |
| Distance | 1,000 ly |
| Constellation | Andromeda |
Position
| Right Ascension | 2h 14.78m |
| Declination | 41° 54.35′ |
Frequently Asked Questions
What type of star is HIP 10457?
HIP 10457 is a Class K — K-type (Orange) star.
How far is HIP 10457 from Earth?
HIP 10457 is approximately 1,000.5 light-years from Earth.
Can you see HIP 10457 with the naked eye?
With an apparent magnitude of 8.91, HIP 10457 is not visible to the naked eye.
What constellation is HIP 10457 in?
HIP 10457 is located in the constellation Andromeda.