HIP 40618
HIP 40618 is a K-type (Orange) star.
At a distance of roughly 1,744 light-years, HIP 40618 is a distant star lying deep within the Milky Way galaxy.
HIP 40618 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 40618 has an apparent magnitude of +8.45, 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 +1.025.
Physikalische Eigenschaften
| Spektralklasse | K Class K — K-type (Orange) |
| Farbindex (B−V) | 1,025 |
Beobachtung
| Scheinbare Helligkeit | +8.45 |
| Absolute Helligkeit | -0,19 |
| Entfernung | 1,744 ly |
Position
| Rektaszension | 8h 17,54m |
| Deklination | -72° 17,14′ |
Frequently Asked Questions
What type of star is HIP 40618?
HIP 40618 is a Class K — K-type (Orange) star.
How far is HIP 40618 from Earth?
HIP 40618 is approximately 1,744.2 light-years from Earth.
Can you see HIP 40618 with the naked eye?
With an apparent magnitude of 8.45, HIP 40618 is not visible to the naked eye.