HIP 1727
HIP 1727 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 1,812 light-years, HIP 1727 is a distant star lying deep within the Milky Way galaxy.
HIP 1727 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
At an apparent magnitude of +10.91, HIP 1727 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its white hue, which corresponds to a B-V color index of +0.450.
Physikalische Eigenschaften
| Spektralklasse | B Class B — B-type (Blue-White) |
| Farbindex (B−V) | 0,450 |
Beobachtung
| Scheinbare Helligkeit | +10.91 |
| Absolute Helligkeit | 2,19 |
| Entfernung | 1,812 ly |
| Sternbild | Cassiopeia |
Position
| Rektaszension | 0h 21,76m |
| Deklination | 58° 20,37′ |
Frequently Asked Questions
What type of star is HIP 1727?
HIP 1727 is a Class B — B-type (Blue-White) star.
How far is HIP 1727 from Earth?
HIP 1727 is approximately 1,812.0 light-years from Earth.
Can you see HIP 1727 with the naked eye?
With an apparent magnitude of 10.91, HIP 1727 is not visible to the naked eye.
What constellation is HIP 1727 in?
HIP 1727 is located in the constellation Cassiopeia.