HIP 2430
HIP 2430 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 2,118 light-years, HIP 2430 is a distant star lying deep within the Milky Way galaxy.
HIP 2430 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 2430 has an apparent magnitude of +8.41, 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 red hue, which corresponds to a B-V color index of +1.486.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.486 |
Observation
| Apparent Magnitude | +8.41 |
| Absolute Magnitude | -0.65 |
| Distance | 2,118 ly |
| Constellation | Cassiopeia |
Position
| Right Ascension | 0h 30.99m |
| Declination | 61° 26.32′ |
Frequently Asked Questions
What type of star is HIP 2430?
HIP 2430 is a Class K — K-type (Orange) star.
How far is HIP 2430 from Earth?
HIP 2430 is approximately 2,117.9 light-years from Earth.
Can you see HIP 2430 with the naked eye?
With an apparent magnitude of 8.41, HIP 2430 is not visible to the naked eye.
What constellation is HIP 2430 in?
HIP 2430 is located in the constellation Cassiopeia.