HIP 10618
HIP 10618 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 2,568 light-years, HIP 10618 is a distant star lying deep within the Milky Way galaxy.
HIP 10618 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 10618 has an apparent magnitude of +7.01, 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 +1.824.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.824 |
Observation
| Apparent Magnitude | +7.01 |
| Absolute Magnitude | -2.47 |
| Distance | 2,568 ly |
| Constellation | Cassiopeia |
Position
| Right Ascension | 2h 16.70m |
| Declination | 67° 17.03′ |
Frequently Asked Questions
What type of star is HIP 10618?
HIP 10618 is a Class K — K-type (Orange) star.
How far is HIP 10618 from Earth?
HIP 10618 is approximately 2,568.2 light-years from Earth.
Can you see HIP 10618 with the naked eye?
With an apparent magnitude of 7.01, HIP 10618 is not visible to the naked eye.
What constellation is HIP 10618 in?
HIP 10618 is located in the constellation Cassiopeia.