HIP 18499
HIP 18499 is a A-type (White) star located in the constellation Perseus.
Located approximately 394.9 light-years from Earth, HIP 18499 resides within the broader disk of our Milky Way galaxy.
HIP 18499 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 18499 has an apparent magnitude of +6.84, 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 blue-white hue, which corresponds to a B-V color index of +0.115.
Physical Properties
| Spectral Class | Class A — A-type (White) |
| Color Index (B−V) | 0.115 |
Observation
| Apparent Magnitude | +6.84 |
| Absolute Magnitude | 1.42 |
| Distance | 395 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 57.27m |
| Declination | 41° 52.84′ |
Frequently Asked Questions
What type of star is HIP 18499?
HIP 18499 is a Class A — A-type (White) star.
How far is HIP 18499 from Earth?
HIP 18499 is approximately 394.9 light-years from Earth.
Can you see HIP 18499 with the naked eye?
With an apparent magnitude of 6.84, HIP 18499 is not visible to the naked eye.
What constellation is HIP 18499 in?
HIP 18499 is located in the constellation Perseus.