HIP 1717
HIP 1717 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,418 light-years, HIP 1717 is a distant star lying deep within the Milky Way galaxy.
HIP 1717 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 1717 has an apparent magnitude of +8.87, 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 +1.510.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.510 |
Observation
| Apparent Magnitude | +8.87 |
| Absolute Magnitude | 0.68 |
| Distance | 1,418 ly |
| Constellation | Cassiopeia |
Position
| Right Ascension | 0h 21.59m |
| Declination | 57° 19.68′ |
Frequently Asked Questions
What type of star is HIP 1717?
HIP 1717 is a Class K — K-type (Orange) star.
How far is HIP 1717 from Earth?
HIP 1717 is approximately 1,418.1 light-years from Earth.
Can you see HIP 1717 with the naked eye?
With an apparent magnitude of 8.87, HIP 1717 is not visible to the naked eye.
What constellation is HIP 1717 in?
HIP 1717 is located in the constellation Cassiopeia.