HIP 47409
HIP 47409 is a A-type (White) star.
At a distance of roughly 1,299 light-years, HIP 47409 is a distant star lying deep within the Milky Way galaxy.
HIP 47409 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 47409 has an apparent magnitude of +8.21, 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 hue, which corresponds to a B-V color index of -0.051.
Physikalische Eigenschaften
| Spektralklasse | A Class A — A-type (White) |
| Farbindex (B−V) | -0,051 |
Beobachtung
| Scheinbare Helligkeit | +8.21 |
| Absolute Helligkeit | 0,21 |
| Entfernung | 1,299 ly |
Position
| Rektaszension | 9h 39,63m |
| Deklination | -4° 12,76′ |
Frequently Asked Questions
What type of star is HIP 47409?
HIP 47409 is a Class A — A-type (White) star.
How far is HIP 47409 from Earth?
HIP 47409 is approximately 1,299.4 light-years from Earth.
Can you see HIP 47409 with the naked eye?
With an apparent magnitude of 8.21, HIP 47409 is not visible to the naked eye.