HIP 7499
HIP 7499 is a K-type (Orange) star located in the constellation Andromeda.
At a distance of roughly 1,152 light-years, HIP 7499 is a distant star lying deep within the Milky Way galaxy.
HIP 7499 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 7499 has an apparent magnitude of +8.10, 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 orange hue, which corresponds to a B-V color index of +1.138.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.138 |
Observation
| Apparent Magnitude | +8.10 |
| Absolute Magnitude | 0.36 |
| Distance | 1,152 ly |
| Constellation | Andromeda |
Position
| Right Ascension | 1h 36.65m |
| Declination | 48° 4.38′ |
Frequently Asked Questions
What type of star is HIP 7499?
HIP 7499 is a Class K — K-type (Orange) star.
How far is HIP 7499 from Earth?
HIP 7499 is approximately 1,152.5 light-years from Earth.
Can you see HIP 7499 with the naked eye?
With an apparent magnitude of 8.10, HIP 7499 is not visible to the naked eye.
What constellation is HIP 7499 in?
HIP 7499 is located in the constellation Andromeda.