HIP 116618
HIP 116618 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 2,104 light-years, HIP 116618 is a distant star lying deep within the Milky Way galaxy.
HIP 116618 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 116618 has an apparent magnitude of +7.98, 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 +1.612.
Physikalische Eigenschaften
| Spektralklasse | K Class K — K-type (Orange) |
| Farbindex (B−V) | 1,612 |
Beobachtung
| Scheinbare Helligkeit | +7.98 |
| Absolute Helligkeit | -1,07 |
| Entfernung | 2,104 ly |
| Sternbild | Cassiopeia |
Position
| Rektaszension | 23h 37,99m |
| Deklination | 52° 49,32′ |
Frequently Asked Questions
What type of star is HIP 116618?
HIP 116618 is a Class K — K-type (Orange) star.
How far is HIP 116618 from Earth?
HIP 116618 is approximately 2,104.2 light-years from Earth.
Can you see HIP 116618 with the naked eye?
With an apparent magnitude of 7.98, HIP 116618 is not visible to the naked eye.
What constellation is HIP 116618 in?
HIP 116618 is located in the constellation Cassiopeia.